wrote:
> |
How do you know that the speed of gravity is 299792458 m/sec?
Did you actual perform an experiment to test that?
Of course you can claim that the speed of gravity and the speed of light
are the same, but physical they are completely different phenomena.
In fact, this difference, is the topic of this thread.
IMO the speed of gravity can be declared as being a constant.
The speed of light IMO not, the reason is gravity.
|
In general relativity the speed of gravity is the same as the speed
of light -- that's a mathematical consequence of the structure of the
(Einstein) equations. (IMPORTANT: In this paragraph I'm making a
purely *mathematical* statement; I'm not saying anything at all about
how well or poorly those equations might model the physical world.)
But what about the actual physical world (universe) in which we live?
The question of the speed at which gravitational waves (or other effects)
propagate is ultimately one which must (can hopefully) be answered by
experimental/observational measurement and analysis. Since general
relativity mathematically hard-wires the speed of gravity be identical
to the speed of light, the previous sentence's analyses can't be done
using solely general relativity. Rather, other relativistic gravity
theories must be used.
There's a very clear and readable discussion of this in section 7.4
("Speed of gravitational waves") of the superb (open-access!) paper
Clifford M. Will
"The Confrontation between General Relativity and Experiment"
Living Reviews in Relativity 17 (2014), 4
http://www.livingreviews.org/lrr-2014-4
I think a direct link to that section is
http://relativity.livingreviews.org/Articles/lrr-2014-4/articlese7.html#x10-750007.4
I encourage anyone interested in this subject to read that section,
and indeed that entire paper!
As Will describes, current observational/experimental data are all
consistent with the speed of gravity being identical to the speed of
light, and [this is a stronger statement which implies the previous one]
consistent with general relativity.
ciao,
- show quoted text -
14 The two postulates in Special Relativity - part 2
From: Gregor Scholten
Datum: Thursday 28 july 2016
Nicolaas Vroom wrote:
> |
This article requires carefull study.
At page 33 we read:
"Black holes contain physical spacetime singularities, regions where
the gravitational tidal field (curvature) becomes infinite. It is
crucial, but hardly easy, to choose a computational technique that
avoids encountering those singularities."
The issue where are these supposed mathematical singularities? IMO
inside the BH at the center of the BH. When you use Newton's law
you can also get infinite result when the distance between two
objects is zero. However physical you will never reach this condition
because at the distance r=3D0 the two objects do not exist any more.
Thus why worry?
|
Because we are not in Newtonian Gravity, but in GR. GR permits - or
better say: even forces - the condition of a singularity being reached
physically. Imagine a star collapsing to a black hole. According to GR,
the collaps of the star's matter reaches the state of a singularity,
i.e. of infinite density, within finite proper time.
> |
At page 33 we also read:
"Finally, different formulations of Einstein's equations behave very
differently when implemented numerically, and we numerical relativists
had to find suitable formulations that generate stable solutions"
I like this honesty, but I'am worried.
The issue is if the Einstein equations have solutions. The fact if
they are stable is of less importance. When the situation you
describe is not stable than the solutions should reflect that.
|
This is not about described situations being unstable, but the
*simulation* of such situations being unstable. I once programmed a
simulation of the time evolution of a wave function, ruled by
Schroedinger equation, based on solving the Schroedinger equation
numerically. Several times, I found the simulated wave function rapidly
diverging to infinity. This happened when I chosed the time steps too
rough, what caused to numerical procedure to become unstable. The
situation which I was describing itself isn't unstable, though.
> |
At page 33 we also read:
"The structure of the 3 + 1 decomposition is familiar from Maxwell's
equations, which similarly consist of a set of constraint equations for
the electric (E) and magnetic (B) fields,"
IMO the physical behaviour of the (E) and (B) fields (because they
are inter-twined) is completely different as the gravitational (or
matter) field.
|
According to GR, your opinion is wrong. In the 3+1 decomposition of GR's
equations, the bevaviour of the gravitational field is quite similar to
the electromagnetic field.
> |
IMO, a gravitational field is also simpler as an E/B field. The
cause of the gravitational field are objects with masses mn and
possitions xn and velocities vn at a sequence of time events tn.
|
That might be true for Newtonian Gravity. But in GR, this is surely not
the case. The gravitational field is rather more complicated than the
electromagnetic field there.
> |
In such a system all objects are like blackholes.
|
You mean because you can handle celestial bodies like mass points? You
can do that in Newtonian Gravity, but not in GR.
To program a simulation based on Newtonian Gravity, you can apply a
numerical mechanics approach where you simulate the movement of
particles that are sufficiently described by positions, but in GR, this
does not work pretty well. You are rather obliged to apply a numerical
field theory approach, where space is discretized and you calculate the
participating fields (gravitational field and at least one matter field
that describes the celestial bodies) at the discrete space points.
> |
The fact that some emit
light is of almost no importance.
|
Indeed. But the fact that the gravitational field has dynamical degrees
of freedom in GR is of great importance.
> |
Also in such a system baryonic matter
and nonbaryonic matter is handled at equal footing.
|
One matter field might be sufficient for baryonic and nonbaryonic matter
in first order, yes. But besides, you need to simulate the gravitational
field, too.
> |
In such a system the speed of light is not considered.
|
Little correction: the propagation of electromagnetic signals is not
considered. The speed of light, however, is considered, since it is the
speed with which changes in gravitational field do propagate.
> |
There is no
issue if this speed is constant or not. The most(?) important
parameter is cg the speed of gravity propagation. IMO this speed
can be considered constant.
|
In GR, cg is equal to c. Measured with respect to a general coordinate
system, c may be variable, and so may be cg.
> |
In such a system you can use Newton's Law.
|
If you prefer to program a simulation based on Newtonian Gravity, you
can Newtonian Gravity, that's right (trivially). But in the article you
are referring to, they talk about a simulation based on GR. Not only
that, they talk about the simulation of a black hole merger. A
simulation based on Newtonian Gravity would be highly inappropriate for
such a situation.
> |
However this law does
not handlethe movement of Mercury
|
Or the processes that run during a black hole merger.
> |
At page 34 we read:
"and showed that only about 0.1% of the total mass of the blackholes is
radiated away in the collision as gravitational waves"
|
See you? If you would simulate a black hole merger based on Newtonian
Gravity, there wouldn't be any gravitational waves at all, since
Newtonian Gravity does not know gravitational waves. So, obviously,
Newtonian Gravity is highly inappropriate here.
> |
I can understand that after any collision there is a loss in total mass,
but not as gravitational waves.
|
If you program a black hole merger based on Newtonian Gravity, there
does not occur any emission of gravitational waves, that's true. But in
a simulation based on GR, such an emissions does occur.
> |
At page 35 we read:
"In particular, some formulations satisfy criteria that guarantee
stable or otherwise well-behaved solutions, while others do not."
I find this remark disturbing. See above question 1. Suppose the two
objects (BHs?) do not merge, but move apart. Is that wrong?
|
It is quite obvious that this would be wrong. If two bodies (no matter
if black holes or other celestial bodies) orbit each other initially due
to some attractive force, and then start to move apart, without influx
of energy from outside, then energy conversation must be violated.
> |
At page 35 we read:
"After decades of effort and anticipation, the combination of the above
techniques enabled the first successful simulations of binary black hole
inspiral and merger,"
Based on which previous observations?
|
This questions does not make sense: simulations are based on theories
(and on numerical methods), not on observations. Except in that sense
that the theories are based on observations themselves. In this case,
the theory is GR, and the observations are those observations that have
been the motivation to delevelop GR.
> |
At page 36 we read:
"For symmetric binaries, the emissions (gravitational waves) from the two
companions cancel each other, but for asymmetric binaries they do not."
I do not understand. IMO the emission of gravitational energy
for any body of mass M is the same. When they merge (2M) it doubles.
|
Gravitational waves can interfer, just like EM waves. Imagine two
sources of EM waves, e.g. two accelerated charges. The emitted EM waves
can interfer destructively, making the emitted energy lower than twice
the energy that would be emitted if only one of the two charges were
present.
For the emission of EM radiation, one distinguishes between coherent and
incoherent emission. For incoherent emission, interference effects are
neglectable, and the intensities (energy per time and surface) just sum
up. For coherent emission, on the other hand, destructive interference
can lower the total intensity.
15 The two postulates in Special Relativity - part 2
From: Nicolaas Vroom
Datum: Saturday 30 july 2016
On Wednesday, 27 July 2016 00:29:16 UTC+2, Gregor Scholten wrote:
> > |
How do you know that the speed of gravity is 299792458 m/sec?
Did you actual perform an experiment to test that?
|
> |
It follows from GR that the "speed of gravity", i.e. the speed with
which changes in the gravitational field do propagate, is equal to the
speed of light. So, if you intend to program a simulation based on GR,
you have to implement this. Of coure, you can as well feel free to
reject GR, but then you have to find an alternative theory of gravity to
found your simulation on.
|
I will not reject GR. I try to understand what is involved in the
movement of objects (as simple as possible)
> > |
Of course you can claim that the speed of gravity and the speed of light
are the same, but physical they are completely different phenomena.
|
> |
As already pointed out, in Relativity (SR as well as GR), the speed of
light is not only the speed of light in the sense of a quantity that is
special to electrodynamics, but a much more general quantity that is
related to the structure of spacetime. So, the speed of light does not
only concern electrodynamic phenomena, but as well completely different
phenomena.
|
All of this is important to handle observations, but IMO
less important for the actual simulations.
> |
Take a point P in spacetime. There are two spacetime regions, one of
them composed by points that are time-like seperated from that point P,
and the other one composed by points that are space-like seperated from
P. Now take a signal that is travelling along the boundary between both
regions. The speed of such a signal is what we call the speed of light
(and the boundary itself we call the light cones).
|
I fully agree with you. The issue is why do you need a light cone
inorder to understand the movement of objects (planets).
Ofcourse you need light to make observations, but that does not mean
you need the speed of light in order to describe the trajectories
of the objects. (Except if the physical quantities change of the objects
studied as a function or speed)
> > |
In fact, this difference, is the topic of this thread.
|
> |
Is it? The title of this thread rather let me think that the topic would
be the two postulates of SR?
|
> > |
IMO the speed of gravity can be declared as being a constant.
The speed of light IMO not, the reason is gravity.
|
> |
If we follow GR, the speed of gravity is in the same sense constant or
non-constant like the speed of light:
- Measured with respect to a local inertial frame, the speed of light is
constant, and since the speed of gravity is equal to the speed of light,
the speed of gravity measured with respect to that local inertial frame
is constant, too.
|
This document http://arxiv.org/abs/gr-qc/0403060 points out that
you can also start from a theory where c and cg are different.
> |
- Measured with respect to a general coordinate system, the speed of
light may be variable (non-constant), and the speed of gravity as well,
since it is equal to the speed of light.
Both, changes in electromagnetic field and changes in gravitational
field, propagate along null-geodesics, i.e. worldlines in spacetime of
length zero (spacetime length, i.e. proper time, not spatial length!).
So, the speed is the same for both, no matter if measured with respect
to a local inertial frame or with respect to a general coordinate system.
|
For me the most important issue to understand is why do you need
c in order to describe the movement of objects i.e. Einstein equations.
SR is primarily based around the speed of light, moving clocks,
length contraction and simultaneity
For me the question is why do you need these concepts in order to
describe the movement of the stars in our galaxy and the galaxy's
in the Universe. (Assuming no electric or magnetic fields)
How important are the lorentz transformations?
When you study this document: http://arxiv.org/pdf/gr-qc/9810065
they use a grid. That means you have one coordinate system, which
makes everything much simpler.
Nicolaas Vroom
16 The two postulates in Special Relativity - part 2
From: Gregor Scholten
Datum: Saturday 30 july 2016
Translate message into English
Nicolaas Vroom wrote:
>>> |
How do you know that the speed of gravity is 299792458 m/sec?
Did you actual perform an experiment to test that?
|
>> |
It follows from GR that the "speed of gravity", i.e. the speed with
which changes in the gravitational field do propagate, is equal to the
speed of light. So, if you intend to program a simulation based on GR,
you have to implement this. Of coure, you can as well feel free to
reject GR, but then you have to find an alternative theory of gravity to
found your simulation on.
|
Let's note that.
>>> |
Of course you can claim that the speed of gravity and the speed of light
are the same, but physical they are completely different phenomena.
|
>> |
As already pointed out, in Relativity (SR as well as GR), the speed of
light is not only the speed of light in the sense of a quantity that is
special to electrodynamics, but a much more general quantity that is
related to the structure of spacetime. So, the speed of light does not
only concern electrodynamic phenomena, but as well completely different
phenomena.
|
> |
All of this is important to handle observations, but IMO
less important for the actual simulations.
|
In the actual simulations, you want to simulate the gravitational field.
Or at least the movement of celestial bodies under the regime of
gravity. So, for the gravitational field, c is relevant, because it is
the propagation velocity of changes in the gravitational field. Of
course, you can neglect that if you restrict yourself to consider the
Newtonian limit.
>> |
Take a point P in spacetime. There are two spacetime regions, one of
them composed by points that are time-like seperated from that point P,
and the other one composed by points that are space-like seperated from
P. Now take a signal that is travelling along the boundary between both
regions. The speed of such a signal is what we call the speed of light
(and the boundary itself we call the light cones).
|
> |
I fully agree with you. The issue is why do you need a light cone
inorder to understand the movement of objects (planets).
|
Because the movement of celestial bodies is ruled by gravity. And the
speed of light is relevant for the gravitational field. Once again: as
long as you restict yourself to the Newtonian limit, you do not need the
speed of light.
> |
Ofcourse you need light to make observations, but that does not mean
you need the speed of light in order to describe the trajectories of
the objects.
|
That is trivial. But as already pointed out: in Relativity, c is not
only the speed with which electromagnetic waves propagate, but rather a
general quantity that concerns all laws of physics, e.g. the laws of
mechanics, i.e. the equations that rule the movement of bodies, or the
laws of field theory: the field equations of all interaction-carrying
field (EM field, gravitational field, nuclear fields, ...) incorporate
the quantity c.
>>> |
IMO the speed of gravity can be declared as being a constant.
The speed of light IMO not, the reason is gravity.
|
>> |
If we follow GR, the speed of gravity is in the same sense constant or
non-constant like the speed of light:
- Measured with respect to a local inertial frame, the speed of light is
constant, and since the speed of gravity is equal to the speed of light,
the speed of gravity measured with respect to that local inertial frame
is constant, too.
|
However, such theories are different from GR. And above, you claimed
that you do not intend you reject GR.
>> |
- Measured with respect to a general coordinate system, the speed of
light may be variable (non-constant), and the speed of gravity as well,
since it is equal to the speed of light.
Both, changes in electromagnetic field and changes in gravitational
field, propagate along null-geodesics, i.e. worldlines in spacetime of
length zero (spacetime length, i.e. proper time, not spatial length!).
So, the speed is the same for both, no matter if measured with respect
to a local inertial frame or with respect to a general coordinate system.
|
> |
For me the most important issue to understand is why do you need
c in order to describe the movement of objects i.e. Einstein equations.
|
Einstein field equations incorporate that changes in the gravitational
field propagate with c. Not only that, Einstein field equations are
based on a four-formalism that is founded on the concept of spacetime,
where c is the connector quantity between space and time. So, any
simulation based on calculations that incorporate Einstein field
equations incorporates the quantity c.
> |
SR is primarily based around the speed of light, moving clocks,
length contraction and simultaneity
For me the question is why do you need these concepts in order to
describe the movement of the stars in our galaxy and the galaxy's
in the Universe.
|
The concepts of SR considered on its own are hardly needed, at least as
long as the stars move with velocities << c, but Einstein field
equations are needed.
> |
(Assuming no electric or magnetic fields)
How important are the lorentz transformations?
|
Except in SR limit, Lorentz transformations are rather unimportant in
GR. However, Lorentz transformations formulas are not the only
relativistic equations where c occurs. Einstein field equations contain
c as well.
It gets rid of coordinate transformations, but not of Einstein field
equations (which contain c).
17 The two postulates in Special Relativity - part 2
From: Nicolaas Vroom
Datum: Saturday 30 july 2016
On Monday, 25 July 2016 23:48:35 UTC+2, Jonathan Thornburg wrote:
> > |
I agree with the physical implications (that means there is no
singularity involved),
|
> |
More precisely, the physical implication is that any singularity or
singularities *inside* the BH, can't affect the (singularity-free)
exterior region *outside* the BH.
|
This does not explain why physicists use the concept of singularity.
Singularities IMO are only mathematical constructs, inside the radius
of the BH. That means you should stay outside this radius.
> > |
The article amazes me because it discusses a BH encounter with a neutron
star (P37). IMO these type of mergers do "not" produce gravitational waves
|
> |
According to our best understanding of the Einstein equations, you're
mistaken: BH-NS encounters do indeed produce gravitational waves.
(In fact, any time you accelerate massive objects in a non-sphericall
-symmetric fashion you produce gravitational waves.)
|
In principle they do not have to be massif.
> > |
and they are extremely difficult, because the merging process is "slow".
Instead "you" study BH BH mergers which are "fast".
|
> |
For various technical reasons it is indeed harder to simulate BH-NS
mergers in detail than it is to simulate BH-BH mergers in detail.
But that's not because of the time scales. Rather, the problem is
that the usual means used to avoid singularities have trouble handling
matter (like the NS), and the usual numerical schemes that can handle
matter can't handle singularities.
|
I can imagine when you want to simulate BH-NS like in Figure 5
page 37 this is extremely tricky. To simulate BH-BH mergers is "much"
simpler. Still I do not understand the issue of singularities
for BH's.
> > |
This article requires carefull study.
At page 33 we read:
"Black holes contain physical spacetime singularities, regions where
the gravitational tidal field (curvature) becomes infinite.
|
etc
> |
In fact, using the usual numerical-relativity techniques it's already
quite a hard problem to just simulate a single BH sitting undisturbed
in an otherwise-empty spacetime. It took many years of research before
techniques were developed to perform simulations of this type which
could run for long times without crashing or suffering rapidly-growing
numerical instabilties.
|
The physical issue is what is the difference between a gravitational
field of a star with mass m0 and a BH with mass m0.
Both at r=0 have a singularity?
> > |
At page 33 we also read:
"Finally, different formulations of Einstein's equations behave very
differently when implemented numerically, and we numerical relativists
had to find suitable formulations that generate stable solutions"
I like this honesty, but I'am worried.
The issue is if the Einstein equations have solutions.
|
> |
Proving the *existence* and *uniqueness* of solutions to the Einstein
equations (for some finite nonzero time interval) is a separate (hard)
mathematical problem, which numerical relativists customarily ignore.
I.e., numerical relativists typically *assume* that such solutions
exist and take it as our task to try to find numerical approximations
to these solutions.
|
Which make it very difficult to test if the solutions are physical
correct.
> > |
The fact if
they are stable is of less importance. When the situation you
describe is not stable than the solutions should reflect that.
|
> |
Suppose the true solution to the Einstein equations is f(t,x,y,z) ,
while the output of our numerical computation is f(t,x,y,z) + g(t,x,y,z)
where g represents the errors (inaccuracies) in our computation.
|
Only the sum is known.
In a sense this means you should start with simulations where
the solution of the Einstein equations are known.
> |
It turns out that for lots of otherwise-plausible numerical schemes, the
error g grows exponentially with time! This means that pretty quickly
the numerical output will be dominated by the error term g , and our
results will bear little or no resemblence to the actual solution f .
(And, our calculation may crash due to (e.g.) floating-point overflow
when g gets big enough.)
|
I had similar problems when I try to simulate stable galaxy rotation
curves.
> |
The problem which Baumgarte and Shapiro are discussing here is that of
trying to prevent this exponential-growth-of-the-error from happening,
i.e., the problem of designing a numerical scheme (including a formulation
of the Einstein equations)
|
How difficult this is I think I got an idea when you try to compute
the equations 15.30, 15.27 15.25 15.18/19/20 and 15.17 in that order
which are shown in the book "Introducing Einstein's Relativity". In these
exercises (in refers order) you know the solution. (Perihelion of Mercury)
> |
While BHs may have (be surrounded by) dynamically-important magnetic
fields, this article is primarily focused on simulations of "vacuum"
BHs (with no electromagnetic fields)
|
> > |
That is why IMO what the article should
show is the description/discussion of the Gravitational field.
|
> |
That would be considerably more complicated; that level of technical
detail wouldn't be appropriate for an article in Physics Today.
|
The following document is also interesting:
https://arxiv.org/abs/gr-qc/0507014
Evolution of Binary Black Hole Spacetimes by Frans Pretorius
The system studied consists of 2BH of equal mass M0.
At page 2 we read:
" We use scalar field gravitational collapse to prepare initial
data that will evolve towards a binary black hole system."
That means they use (it seems) special initial conditions
such that the two BH's will merge.
> > |
At page 34 we read:
"Unlike Maxwell's equations, however, Einstein's equations are nonlinear,
and so they introduce a new set of phenomena and challenges."
Also we read: "In finite-difference applications, the spacetime continuum
is represented as a discrete lattice or grid,"
and: One class is initial data problems"
To start from the correct initial conditions in any simulation is a
difficult issue.
Consider two objects of identical mass which revolve around each other in
a circle. The question (1) is how do they behave?
Is this a stable configuration?
|
> |
Again, the details of how to compute this are rather complicated.
Continuing the Maxwell-equations analogy, etc.
|
The book by Ray d'Inverno mentioned above in paragraph 15.3 explains
the "Advance of the perihelion of Mercury"
The impression I get is that it is very difficult to simulate more (all?)
planets using GR. (Independent GR is required)
> > |
At page 34 we read:
"and showed that only about 0.1% of the total mass of the blackholes is
radiated away in the collision as gravitational waves"
I can understand that after any collision there is a loss in total mass,
but not as gravitational waves.
|
> |
Well, these simulations are being done assuming general relativity.
And in GR, such a collision produces gravitational waves, which carry
away some mass/energy (as well as linear and angular momentum). That
means that the mass of the final remanent BH is indeed less than the
sum of the masses of the two initial BHs.
|
See next comment
> > |
At page 35 we read:
"In particular, some formulations satisfy criteria that guarantee
stable or otherwise well-behaved solutions, while others do not."
I find this remark disturbing. See above question 1. Suppose the two
objects (BHs?) do not merge, but move apart. Is that wrong?
|
> |
For these simulations the initial conditions are set up so that the two
initial BHs form a bound system. It's thus mathematically guaranteed
that the two BHs will eventually merge.
|
This is the same (more or less) as the example above.
For example you can use Newton's Law to give the two BH's initial
conditions such that they move in a circle (using Newton's Law)
The issue is what happens when you use GR?
Will they merge?
(If yes why don't the planets of our solar system merge)
> > |
At page 35 we read:
"After decades of effort and anticipation, the combination of the above
techniques enabled the first successful simulations of binary black hole
inspiral and merger,"
Based on which previous observations? These observations should
demonstrate that binary BH actual merge and that no third companion
is involved.
|
> |
Baumgarte and Shapiro are describing (numerical) *simulations*, i.e.,
numerically-constructed (approximate) solutions of the Einstein equations.
They're saying that after decades of effort, the various techniques
they describe allowed the first successful *simulations* of binary BH
inspiral/merger in 2005. This was (is) a purely mathematical and
computational result -- the researchers constructed an (approximate)
solution of the Einstein equations having certain properties.
|
Some of this is described in: https://arxiv.org/abs/gr-qc/050701
"Evolution of Binary Black Hole Spacetimes" by Frans Pretorius
Page 4 :"V Conclusion" is a good starting point of this document!
At page 1 we read:
"The code has several features of note, some or all of
which may be responsible for its stability properties:"
Generally speaking when you use Newton's Law there are no stability
issues in the sense of software issues.
It is possible that the system you try to simulate is not stable.
For example you can try a comet which collides with the sun.
In that case your software should show the same results.
When you try to solve Einstein's equations and there are stability
issues with the software you have to be very carefully,
because it is possible that the system itself is non stable.
At page 2 we read:
"We use scalar field gravitational collapse to prepare initial
data that will evolve towards a binary black hole system."
This sentence worries me, because it gives the impression that
the code is modified to force that the 2 BH's will merge.
> |
Observations of actual astrophysical BHs and their inspiral/mergers
are a whole separate topic, which I'm not going to get into here.
|
But this is actual very important.
I mean are we sure that BH's actual merge?
When you simulate binary systems using Newton's Law they are stable.
(No energy loss)
When there is an increase in mass they start to merge.
When the opposite the average distance will increase. Such a binary system is
not stable, but is not caused by computational (error) constraints.
> > |
At page 36 we read:
"For symmetric binaries, the emissions (gravitational waves) from the two
companions cancel each other, but for asymmetric binaries they do not."
I do not understand. IMO the emission of gravitational energy
for any body of mass M is the same. When they merge (2M) it doubles.
|
> |
You're mistaken. Baumgarte and Shapiro have a beautiful eplanation of
this by analogy to an S-shaped rotating lawn sprinkler with asymmetric
arms (pages 35-36 of their article). I really can't do much more than
to urge you to re-read their explanation (which is clearer than anything
I could write).
|
To compare revolving BH's with sprinkler heads IMO is tricky.
IMO the subject below is more realistic.
> |
More generally, the emission of gravitational waves is NOT the same
for any body of mass M. For example, if you have a spherical shell of
matter, of total mass M, and that shell expands in a spherically symmetric
manner, NO gravitational waves are emitted at all!
|
I agree. In this case you have a static gravitational field.
When there is a revolving object at radius r2 you will not detect
"any" difference.
> |
In contrast, if you
have a pair of non-spinning BHs of mass M/2 falling together along a line
(i.e., a head-on collision) from an initial state where they're at rest
far apart, then about 0.1% of the total mass is radiated in gravitational
waves.
|
What is the situation when you compare the above with two stars of mass M/2?
Before they collide is there also a 0.1% decrease in total mass?
> |
But if you have that same pair of BHs falling together in an
ingoing spiral (where the initial state is that they're in a very far
apart almost-circular orbit around each other), then on the order of 4%
of the total mass is radiated in gravitational waves!
|
Again what is the difference with this example when you have two stars
under identical initial conditions?
How much of the total mass is radiated away?
Figure 4 in the "binary black hole mergers.pdf" is interesting because
it shows the merging of equal-mass non-spinning BH's. This simulation
is interesting because it shows a circumbinary gaseous disk.
I have also tried to simulate revolving BH's using Newton's Law.
I did not succeed.
However such a simulation can completely change when a third object
is involved. This third object will approach such a binary system towards
the center of its mass, but does not always immediate collide
with any of the two. Instead its speed will increase drastically
and the third object has chance to evaporate (explode) and
form a gaseous disk. (which can merge slowly with both BH's). This slowly
increase in mass of both can result in the final merging of the 2 BH's
Nicolaas Vroom
18 The two postulates in Special Relativity - part 2
From: Gregor Scholten
Datum: Sunday 31 july 2016
Nicolaas Vroom wrote:
> |
For me the most important issue to understand is why do you need
c in order to describe the movement of objects i.e. Einstein equations.
SR is primarily based around the speed of light, moving clocks,
length contraction and simultaneity
For me the question is why do you need these concepts in order to
describe the movement of the stars in our galaxy and the galaxy's
in the Universe. (Assuming no electric or magnetic fields)
How important are the lorentz transformations?
|
A remark concerning SR and Lorentz transformation, since this seems to a
crucial issue for you:
On the one hand, Lorentz transformation is the transformation from one
inertial frame to the other. So, when considering only one single frame,
one could assume that Lorentz transformation is of little relevance
(like you seem to assume). However, that is not correct: SR does not
only tell us that inertial frames are transformed to one another by
Lorentz transformation, but also tells us that the laws of physics are
the same in all inertial frames.
This requires that the laws of physics are Lorentz-covariant, i.e. keep
their form when transforming from one inertial frame to the other. Take
e.g. Maxwell equations. Using the four-potential A^mu and the Lorentz
gauge, one can write the Maxwell equations as
\partial_mu \partial^mu A^nu = j^nu
where j^nu is the electric four flux density. Now transform these
equations from inertial frame to the other: the four flux density j^nu
is transformed, the four potential A^nu is transformed, and the
derivatives \partial_mu, \partial^mu are transformed:
j^nu -> j'^nu = L^nu_mu j^mu
A^nu -> A'^nu = L^nu_mu A^mu
partial_mu -> partial'_mu = L^nu_mu partial_nu
partial^mu -> partial'^mu = L^mu_nu partial^nu
where L_mu^nu is the Lorentz transformation matrix. Due to the
Lorentz-covariance of the Maxwell equations, the new equations in the
new inertial frame:
\partial'_mu \partial'^mu A'^nu = j'^nu
must be satisfied. This is only possible because the Maxwell equations
have a special form, namely a Lorenz covariant form. Take as
counter-example the non-relativistic Schroedinger equation: after
Lorentz transformation of its terms into a new inertial frame, the
Schroedinger equation is no longer satisfied.
So now, when considering the upper form of the Maxwell equations more in
detail, we see the quantity c occuring: partial_mu is an abbreviation
for partial / (partial x^mu), where x^mu is defined by
x^mu = (ct, x, y, z)
So, the term \partial_mu \partial^mu is nothing but
-c^2 partial^2/(partial t^2) + partial^2/(partial x^2) +
partial^2/(partial y^2) + partial^2/(partial z^2)
what contains the quantity c (as c^2). The same is true for any other
equation that satisfied the requirements of Lorentz covariance: the
quantity c is always present.
So, even if you restrict yourself to consider only one single frame of
reference, you need to incorporate the quantity c when doing
calculations, e.g. solving field equations or equations of motion for
particles or bodies.
Now, when we change from SR to GR, Lorentz covariance is only relevant
in the SR limit. In general, we have to consider general covariance
instead. But requirement of covariance still yields the occurance of c
in all equations.
19 The two postulates in Special Relativity - part 2
From: Nicolaas Vroom
Datum: Sunday 31 july 2016
On Wednesday, 27 July 2016 09:13:16 UTC+2, Jonathan Thornburg wrote:
> > |
How do you know that the speed of gravity is 299792458 m/sec?
In fact, this difference, is the topic of this thread.
IMO the speed of gravity can be declared as being a constant.
The speed of light IMO not, the reason is gravity.
|
> |
In general relativity the speed of gravity is the same as the speed
of light -- that's a mathematical consequence of the structure of the
(Einstein) equations. (IMPORTANT: In this paragraph I'm making a
purely *mathematical* statement; I'm not saying anything at all about
how well or poorly those equations might model the physical world.)
|
I fully understand. IMO the laws of physics should be a description
of the physical reality. The parameters used should also correspond
to the (measurable) physical reality.
> |
But what about the actual physical world (universe) in which we live?
The question of the speed at which gravitational waves (or other effects)
propagate is ultimately one which must (can hopefully) be answered by
experimental/observational measurement and analysis. Since general
relativity mathematically hard-wires the speed of gravity be identical
to the speed of light, the previous sentence's analyses can't be done
using solely general relativity. Rather, other relativistic gravity
theories must be used.
|
What I try to do is to discuss the movement of objects (simulations)
independent of observations. As such the equations that describe
these movements should be strictly based on the parameter cg and not
on the parameter c except when the movement is influenced by
electromagnetic effects.
> |
There's a very clear and readable discussion of this in section 7.4
("Speed of gravitational waves") of the superb (open-access!) paper
Clifford M. Will
"The Confrontation between General Relativity and Experiment"
Living Reviews in Relativity 17 (2014), 4
http://www.livingreviews.org/lrr-2014-4
|
In this document also the speed of gravity is discussed at page 45.
At page 45 there is a link to: http://arxiv.org/abs/gr-qc/0403060
by S. Carlip. This document also makes a clear distinction between
c and cg, and recognizes that the two could be different.
At page 2 of that document we read:
"Suppose we have a theory in which light and gravity propagate at
fixed speeds, but in which c <> cg."
What is wrong with the following:
"Suppose we have a theory in which light has average speed c and
gravity propagate at average speed cg, but in which c <> cg."?
(Because the speed c is influenced by gravity)
The Shapiro time delay issue (however very interesting)
is not the primary topic in this posting.
At page 85 we read:
"Because the frequency of the gravitational radiation sweeps from low
frequency at the initial moment of observation to higher frequency at
the final moment, the speed of the gravitons emitted will vary, from
lower speeds initially to higher speeds (closer to c) at the end."
Interesting. Is this a general accepted fact?
That's why I mention average value of cg.
> |
I encourage anyone interested in this subject to read that section,
and indeed that entire paper!
As Will describes, current observational/experimental data are all
consistent with the speed of gravity being identical to the speed of
light, and [this is a stronger statement which implies the previous one]
consistent with general relativity.
|
"Difficult"
To evaluate this you must have a very good understanding which
physical phenomena are influenced by the speed of light and
which by the speed of gravitation.
In a sense what you should do is to observe the evolution of
the perihelion of the planet Mercury over a very long period
in order to to study the influence of the parameter cg.
Nicolaas Vroom.
20 The two postulates in Special Relativity - part 2
From: Nicolaas Vroom
Datum: Sunday 31 july 2016
On Thursday, 28 July 2016 12:02:06 UTC+2, Gregor Scholten wrote:
> > |
This article requires carefull study.
At page 33 we read:
"Black holes contain physical spacetime singularities, regions where
the gravitational tidal field (curvature) becomes infinite. It is
crucial, but hardly easy, to choose a computational technique that
avoids encountering those singularities."
|
> |
Because we are not in Newtonian Gravity, but in GR. GR permits - or
better say: even forces - the condition of a singularity being reached
physically. Imagine a star collapsing to a black hole. According to GR,
the collaps of the star's matter reaches the state of a singularity,
i.e. of infinite density, within finite proper time.
|
GR (as all laws) should be a description of the physical reality.
When a star collapses, somewhere it stops to contract, meaning that the
density physical does not reach infinity i.e a singularity.
As such a BH does not contain a singularity.
For a colliding star the same issue exists. The distance never reaches
zero, as such during the collision and merging there is no singularity issue,
http://www.physics.utoronto.ca/~phy189h1/binary%20black%20hole%20mergers.pdf
When you study page 35 you read:
"Simulating black holes, however, necessarily requires careful handling of
their interior spacetime singularities. One approach invokes black hole
excision, whereby the interior of a black hole is removed from the
computational mesh. That surgery is justified physically since, by definition,
the black hole interior cannot affect the exterior."
In a sense this means: We "know" there is a singularity, but we don't care.
> > |
At page 33 we also read:
"Finally, different formulations of Einstein's equations behave very
differently when implemented numerically, and we numerical relativists
had to find suitable formulations that generate stable solutions"
|
> |
This is not about described situations being unstable, but the
*simulation* of such situations being unstable. I once programmed a
simulation of the time evolution of a wave function, ruled by
Schroedinger equation, based on solving the Schroedinger equation
numerically. Several times, I found the simulated wave function rapidly
diverging to infinity. This happened when I chosed the time steps too
rough, what caused to numerical procedure to become unstable. The
situation which I was describing itself isn't unstable, though.
|
IMO there are different problems: 1. The situation can be unstable,
2. the equations are unstable, 3. the numerical solution can be unstable,
4. or any combination
Step size problems belong in cathegory 3.
The problems I had with implementing the equations outlined in
chapter 15.3 of the book "Introducing Einstein's relativity" belong
in cathegory 2. In these cases the solution is known.
> > |
IMO, a gravitational field is also simpler as an E/B field. The
cause of the gravitational field are objects with masses mn and
possitions xn and velocities vn at a sequence of time events tn.
|
> |
That might be true for Newtonian Gravity. But in GR, this is surely not
the case. The gravitational field is rather more complicated than the
electromagnetic field there.
|
In part that is what I want to discuss. See also my previous answers
> > |
In such a system all objects are like blackholes.
|
> |
You mean because you can handle celestial bodies like mass points? You
can do that in Newtonian Gravity, but not in GR.
To program a simulation based on Newtonian Gravity, you can apply a
numerical mechanics approach where you simulate the movement of
particles that are sufficiently described by positions, but in GR, this
does not work pretty well. You are rather obliged to apply a numerical
field theory approach, where space is discretized and you calculate the
participating fields (gravitational field and at least one matter field
that describes the celestial bodies) at the discrete space points.
|
Each such fields must be a 3D field and grid used must have the same
accuracy (or better) as the step size used with Newton's Law.
Not only that after every calculation (dt) the fields change.
A different issue is to what extend you have to take size of the objects
involved into account. Paragraph 15.3 mentioned above does not.
Starting point is that all objects are spheres.
> > |
In such a system the speed of light is not considered.
|
> |
Little correction: the propagation of electromagnetic signals is not
considered. The speed of light, however, is considered, since it is the
speed with which changes in gravitational field do propagate.
|
In that sense, when studying the gravitational field, always the parameter
cg should be mentioned and not the parameter c. This is important because
their physical behavior can be different.
> > |
There is no
issue if this speed is constant or not. The most(?) important
parameter is cg the speed of gravity propagation. IMO this speed
can be considered constant.
|
> |
In GR, cg is equal to c. Measured with respect to a general coordinate
system, c may be variable, and so may be cg.
|
I assume that this coordinate system is the same as the grid discussed.
The reason that c varies can be gravity (mass).
For cg I do not think that this applies.
> > |
At page 34 we read:
"and showed that only about 0.1% of the total mass of the blackholes is
radiated away in the collision as gravitational waves"
|
> |
See you? If you would simulate a black hole merger based on Newtonian
Gravity, there wouldn't be any gravitational waves at all, since
Newtonian Gravity does not know gravitational waves. So, obviously,
Newtonian Gravity is highly inappropriate here.
|
Gravitational waves only become "visible" around binary systems when
test objects are used. Such a test object (at large distance) in circular
orbit shows a sinus function (or wave). The periodicity is the same as the
revolution of the binary system.
In the case of Newton's law the forces involved act instantaneous.
GR assumes that this is not the case; there is a delay.
If you consider gravitons than in the case of GR the speed is finite.
Under Newton's Law the speed is infinite.
> > |
I can understand that after any collision there is a loss in total mass,
but not as gravitational waves.
|
> |
If you program a black hole merger based on Newtonian Gravity, there
does not occur any emission of gravitational waves, that's true. But in
a simulation based on GR, such an emissions does occur.
|
See my comments above.
> > |
At page 35 we read:
"In particular, some formulations satisfy criteria that guarantee
stable or otherwise well-behaved solutions, while others do not."
I find this remark disturbing. See above question 1. Suppose the two
objects (BHs?) do not merge, but move apart. Is that wrong?
|
> |
It is quite obvious that this would be wrong. If two bodies (no matter
if black holes or other celestial bodies) orbit each other initially due
to some attractive force, and then start to move apart, without influx
of energy from outside, then energy conversation must be violated.
|
That not what I have in mind. It has to do with the physical behaviour.
How do we know that BH's (natural) merge?
Is it not possible that they (natural) move apart?
> > |
At page 36 we read:
"For symmetric binaries, the emissions (gravitational waves) from the two
companions cancel each other, but for asymmetric binaries they do not."
I do not understand. IMO the emission of gravitational energy
for any body of mass M is the same. When they merge (2M) it doubles.
|
> |
Gravitational waves can interfer, just like EM waves. Imagine two
sources of EM waves, e.g. two accelerated charges. The emitted EM waves
can interfer destructively, making the emitted energy lower than twice
the energy that would be emitted if only one of the two charges were
present.
|
Electric fields are based around positive and negative charges.
By comparison, gravitational fields do not have this distinction.
They are one of a kind.
Nicolaas Vroom.
21 The two postulates in Special Relativity - part 2
From: Nicolaas Vroom
Datum: Monday 1 augustus 2016
On Saturday, 30 July 2016 18:48:02 UTC+2, Gregor Scholten wrote:
> > |
I will not reject GR.
|
You can only reject something if you "fully" understand it.
> |
In the actual simulations, you want to simulate the gravitational field.
Or at least the movement of celestial bodies under the regime of
gravity. So, for the gravitational field, c is relevant, because it is
the propagation velocity of changes in the gravitational field.
|
Please let us call this speed cg.
> |
Of course, you can neglect that if you restrict yourself to consider
the Newtonian limit.
|
Under Newton's law the speed cg is infinite (instantaneous)
> |
Because the movement of celestial bodies is ruled by gravity. And the
speed of light is relevant for the gravitational field. Once again: as
long as you restict yourself to the Newtonian limit, you do not need the
speed of light.
|
Consider a world in which all objects are darkmatter object.
You could also consider a world with only BH's.
Why do you need the speed of light?
Consider also that you know all the present positions.
> > |
Ofcourse you need light to make observations, but that does not mean
you need the speed of light in order to describe the trajectories of
the objects.
|
> |
That is trivial. But as already pointed out: in Relativity, c is not
only the speed with which electromagnetic waves propagate, but rather a
general quantity that concerns all laws of physics, e.g. the laws of
mechanics, i.e. the equations that rule the movement of bodies, etc.
|
"I know what Relativity says", but physical photons and gravitons
are completely different "objects" and IMO you should try to study
them independently.
At page 170 of th earlier book discussed by Ray d'Inverno we read:
"The non-linearity reveals itself physically in the following way:
the gravitational field produced by some source contains energy and
hence, by SR, mass, and this mass in turn is itself a source of a
gravitational field: that is to say that the gravitational field
is coupled to itself. This non-linearity means that the equations
are very difficult to solve in general."
This raises immediate two questions: How do you than know
that the equations are correct and how do you calculate the
parameters of the equations.
A different question is what does it mean: that you have solved the
equations. In many cases there are no continuous solutions.
The best you can do is to use a numerical solution and solve
the equation step by step in a timewise manner.
What is the most difficult part to simulate a billiard game:
the collision between the balls.
That means we temporarily exclude collisions.
IMO why celestial problems are so difficult is because of lack of
information about the actual gravitational field.
The actual gravitational field here is some type of "superposition" of
the subset gravitational fields caused by all the objects considered.
The problem is that each of these fields we observe here is caused
by the objects in the past.
The same for all actual fields for each of the objects considered.
This interaction (delay) is what everything makes so difficult.
> |
However, such theories are different from GR. And above, you claimed
that you do not intend you reject GR.
|
Reading all about numerical solutions and how difficult this is,
you start thinking are there no different, more simpler solutions
to do a correct simulation of the evolution of the planets.
> > |
For me the most important issue to understand is why do you need
c in order to describe the movement of objects i.e. Einstein equations.
|
> |
Einstein field equations incorporate that changes in the gravitational
field propagate with c. Not only that, Einstein field equations are
based on a four-formalism that is founded on the concept of spacetime,
where c is the connector quantity between space and time. So, any
simulation based on calculations that incorporate Einstein field
equations incorporates the quantity c.
|
I agree, however the issue when you consider numerical solutions, when
you consider that the initial positions and velocities are known,
to what extend do you need the quantity c and cg.
IMO only cg. The quantity c is only used as part of the observations
or when there are electromagnetic fields involved.
A typical case where you need c is when you want to calculate
the Schwarzschild Radius. See chapter 16.9 of the mentioned book.
Ofcourse you could claim that they have the same strength and are
mathematical indistinquishable, but physical they are not.
For example it is possible that you can solve gravitational fields
in one coordinate system and without moving clocks.
IMO such a consideration would make the equations simpler.
> > |
(Assuming no electric or magnetic fields)
How important are the lorentz transformations?
|
> |
Except in SR limit, Lorentz transformations are rather unimportant in
GR. However, Lorentz transformations formulas are not the only
relativistic equations where c occurs. Einstein field equations contain
c as well.
|
That means when you want to simulate the movements of the planets
using GR you do not need the Lorentz transformations.
> |
It gets rid of coordinate transformations, but not of Einstein field
equations (which contain c).
|
But does it also get rid of moving clocks?
Nicolaas Vroom.
22 The two postulates in Special Relativity - part 2
From: Gregor Scholten
Datum: Friday 5 augustus 2016
Nicolaas Vroom wrote:
>> |
More precisely, the physical implication is that any singularity or
singularities *inside* the BH, can't affect the (singularity-free)
exterior region *outside* the BH.
|
> |
This does not explain why physicists use the concept of singularity.
Singularities IMO are only mathematical constructs, inside the radius
of the BH.
|
If we follow GR, singularities are not only mathematical constructs, but
exist unavoidably. Of course, one can hope that in a theory of quantum
gravity, singularities can be avoided, e.g. by the gravitational collaps
stopping at some finite density, like Planck density (10^94 g/cm^3), but
if one programs a simulation based on GR, one has to implement the
statements of GR, not of a theory of quantum gravity.
>> |
In fact, using the usual numerical-relativity techniques it's already
quite a hard problem to just simulate a single BH sitting undisturbed
in an otherwise-empty spacetime. It took many years of research before
techniques were developed to perform simulations of this type which
could run for long times without crashing or suffering rapidly-growing
numerical instabilties.
|
> |
The physical issue is what is the difference between a gravitational
field of a star with mass m0 and a BH with mass m0.
Both at r=0 have a singularity?
|
No. The black hole has a singularity at r = 0 (according to GR), but the
the ordinary star does not. The ordinary star has a non-zero radius and
a finit mass density.
If you describe the movement of the ordinary star in terms of a
mechanical approach, you can handle the star as a mass point in some
sense, i.e. you do not need to take its non-zero radius into account,
but as soon as you want to consider the star's gravitational field, you
can no longer apply this description. You need to incorporate the star's
finite size then.
> |
The following document is also interesting:
https://arxiv.org/abs/gr-qc/0507014
Evolution of Binary Black Hole Spacetimes by Frans Pretorius
The system studied consists of 2BH of equal mass M0.
At page 2 we read:
" We use scalar field gravitational collapse to prepare initial
data that will evolve towards a binary black hole system."
That means they use (it seems) special initial conditions
such that the two BH's will merge.
|
No, that does not mean that. The use initial conditions that result in a
collaps to two black holes, which do not immediately merge. Such initial
conditions can e.g. be two ordinary stars that each undergo a collaps to
a black hole. The merger of the two black holes is something that
happens in the later evolution of the binary black hole system.
>>> |
At page 34 we read:
"Unlike Maxwell's equations, however, Einstein's equations are nonlinear,
and so they introduce a new set of phenomena and challenges."
Also we read: "In finite-difference applications, the spacetime continuum
is represented as a discrete lattice or grid,"
and: One class is initial data problems"
To start from the correct initial conditions in any simulation is a
difficult issue.
Consider two objects of identical mass which revolve around each other in
a circle. The question (1) is how do they behave?
Is this a stable configuration?
|
>> |
Again, the details of how to compute this are rather complicated.
Continuing the Maxwell-equations analogy, etc.
|
> |
The book by Ray d'Inverno mentioned above in paragraph 15.3 explains
the "Advance of the perihelion of Mercury"
The impression I get is that it is very difficult to simulate more (all?)
planets using GR.
|
You should note that paragraph 15.3 depicts a mechanical approach: the
equations describe the movement of a body (Mercury), not the evolution
of fields. The configuration of the gravitational field is presumed as
known there (namely as being the Schwarzschild solution), so it needn't
be calculated.
In the simulation of a black hole merger as well as in the
Maxwell-equations analogy, things are totally different: the evolution
of the gravitational (or electromagnetic) field itself is what needs to
be calculated, not the movement of bodies under the regime of a known
field configuration.
>>> |
At page 35 we read:
"In particular, some formulations satisfy criteria that guarantee
stable or otherwise well-behaved solutions, while others do not."
I find this remark disturbing. See above question 1. Suppose the two
objects (BHs?) do not merge, but move apart. Is that wrong?
|
>> |
For these simulations the initial conditions are set up so that the two
initial BHs form a bound system. It's thus mathematically guaranteed
that the two BHs will eventually merge.
|
> |
This is the same (more or less) as the example above.
For example you can use Newton's Law to give the two BH's initial
conditions such that they move in a circle (using Newton's Law)
The issue is what happens when you use GR?
|
The first difference that occurs that you can no longer apply a
mechanical approach like in Newtonian theory or for the advance of the
Mercury perihelion. You need to calculate the field configuration
applying a field theory approach.
For the advance of the Mercury perihelion, although it belongs to GR,
the mechanical approach is sufficient because the field configuration is
known (from an analytical field theory approach applies by Karl
Schwarzschild in 1917 that yielded Schwarzschild solution). For the
blach hole merger, the field configuration is not known analytically,
therefore a numerical field theory approach is required.
According to the result of the simulation we are talking about: yes.
Accordint to a mechanical approach comparable to the approach for the
advance of the Mercury perihelion: there is no such approach, therefore
is question does not make sense.
> |
(If yes why don't the planets of our solar system merge)
|
In fact, according to GR, the planets of our solar system do merge:
during their movement around the sun, they emit gravitational waves and
therefore loose energy, making them fall into the sun spirally. However,
the intensity of the emitted gravitational waves is very low, so the
energy loss per time unit is very low, too, and by this, it takes some
10^24 years until all planets have fallen into the sun.
In a close binary black hole system, the energy loss due to
gravitational wave emissions is much higher, so the merger is very much
quicker.
> |
Some of this is described in: https://arxiv.org/abs/gr-qc/050701
"Evolution of Binary Black Hole Spacetimes" by Frans Pretorius
Page 4 :"V Conclusion" is a good starting point of this document!
At page 1 we read:
"The code has several features of note, some or all of
which may be responsible for its stability properties:"
Generally speaking when you use Newton's Law there are no stability
issues in the sense of software issues.
|
For Newton's law, numerical mechanics is sufficient. For GR, you need to
apply a numerical field theory approach (except situations that are as
simple as the advance of the Mercury perhelion). That's very different.
> |
It is possible that the system you try to simulate is not stable.
For example you can try a comet which collides with the sun.
|
For that, you can assume the gravitational field of the comet as being
neglectable, so that you only need to consider the gravitational field
of the sun, for which you can assume the known Schwarzschild solution,
like for the advance of the Mercury perihelion (where you neglect the
gravitational field of Mercury), enabling you to apply a numerical
mechanics approach.
For a black holer merger, however, you need to consider the
gravitational field of both black holes, requiring a field theory approach.
> |
In that case your software should show the same results.
When you try to solve Einstein's equations and there are stability
issues with the software you have to be very carefully,
because it is possible that the system itself is non stable.
|
There are good reasons to assume that a two-body system, even with
taking a limited speed of gravity into account, is stable.
> |
At page 2 we read:
"We use scalar field gravitational collapse to prepare initial
data that will evolve towards a binary black hole system."
This sentence worries me, because it gives the impression that
the code is modified to force that the 2 BH's will merge.
|
That impression is wrong, though. As already discussed, the initial data
are prepared to make two black holes, not a black hole merger.
>> |
Observations of actual astrophysical BHs and their inspiral/mergers
are a whole separate topic, which I'm not going to get into here.
|
> |
But this is actual very important.
I mean are we sure that BH's actual merge?
|
No, we aren't. However, we are sure that according to GR, they do. And
we have recent observations of gravitational waves that match the
predictions that GR makes concerning gravitational waves emitted during
a black hole merger.
> |
When you simulate binary systems using Newton's Law they are stable.
(No energy loss)
|
But we know that Newton's law is not fully correct. We know that GR is
more correct than Newton's theory.
> |
When there is an increase in mass they start to merge.
|
You mean in Newton's theory? Then your statement is not correct. In
Newton's theory, it depends on the way the mass is increased. Imagine
two celestial bodies orbitting each other. Imagine the mass of one body
is increased by infalling comets. If the comets fall in that direction
that is opposite to the orbitting direction, they slow down the body
when hitting it, resulting in the orbit becoming closer, like in a
merger scenarion. If the comets fall in the other direction, however,
the body is accelerated, so that the orbit becomes wider.
> |
When the opposite the average distance will increase. Such a binary system is
not stable, but is not caused by computational (error) constraints.
|
You mean you consider the merger itself as instability? When talking
about instabilities related to the simulation of a black hole merger,
one means something different. The merger itself is no instability.
Instability means that the results of the numerical computation become
more and more different from the analytical solution, the longer the
simulation runs.
>> |
But if you have that same pair of BHs falling together in an
ingoing spiral (where the initial state is that they're in a very far
apart almost-circular orbit around each other), then on the order of 4%
of the total mass is radiated in gravitational waves!
|
> |
Again what is the difference with this example when you have two stars
under identical initial conditions?
|
You mean two stars that are no black holes but have radii >> their
Schwarzschild radii? Then the difference is that the two stars behave
different from two black holes at the latest when their surfaces touch
each other.
23 The two postulates in Special Relativity - part 2
From: Gregor Scholten
Datum: Sunday 7 augustus 2016
Nicolaas Vroom wrote:
>> |
Gravitons are assumed to occur in quantum gravity, when quantizing a
gravitational field with finite propagation speed, i.e. like the
gravitational field of GR. On the one hand, there would be real
gravitations, which would be quantized gravitational waves, and on the
other hand virtual gravitons, appearing when applying perturbation
theory on scattering processes intermediated by gravitational field.
|
> |
I like your comments. For me the problem is when do you speak of GR and when
of quantum gravity. I more or less thought that GR always involves
a gravitational field which propagates and what propagates are the gravitons.
|
Then you thought something wrong. A field itself does not propagate. A
field is everywhere at every time, in that sense that at any point (x,t)
in spacetime, there is a value of this field, let's call it A(x,t). What
may propagate are *changes* in the field.
Let's consider the electromagnetic field. Imagine an electric charge q
being at rest at a position x0. In a wide range around the charge, the
configuration of the electromagnetic field is that of an electrostatic
field caused by the charge, i.e. the magnetic field is zero and the
electric field at a point x is E(x) = q / (4 pi eps0 |x - x0|^2). Since
that field configuration is static, there does not propagate anything.
Now imagine the charge is accelerated for a short time. After the
acceleration phase, the charge is moving with constant velocity away
from it initial position x0. In a small range around the position x0,
the electromagnetic field already "knows" that the charge is moving away
from x0. The field configuration in this range has already changed: the
electric field at some point x in this range has a new value E(x,t) = q
/ (4pi eps0 |x - x'(t)|^2), where x'(t) is the position of the charge at
the time t, and the magnetic field is non-zero.
Outside this range, the electromagnetic field still has its old
configuration, it does knot "know" yet that the charge has been
accelerated. So, there are two regions, one where the field
configuration is already modified and one where it is not yet. Between
both, there is a boundary at which the field configuration is currently
changing from the old to the new configuration. This boundary is a thin
spherical shell of radius (t - t0) * c, where t is the current time and
t0 is the time at which the charge was accelerated (we assume that the
duration of the acceleration phase is << t - t0).
The spherical shell is expanding, with the speed c. This shell, where
the field the field is changing its configuration from the old one to
the new one, is what propagates. To get an impression how the electric
field looks like in this shell, take this image:
http://www.walter-orlov.wg.am/berkley.JPG
You see some "buckling" in the diretion of the electric field. This
"buckling" forms an electromagnetic wave pulse, which is nothing but the
bremsstrahlung emitted from the charge due to the short acceleration phase.
So, as long as electric charges are resting or uniformly moving, there
isn't anything propagating. Only if charges are accelerated, there are
changes in the field that propagate. The same principle applies for any
other field, including the gravitational field.
Concerning gravitons and photons: I guess you read somewhere that
interactions are mediated by virtual particles, photons in the
electromagnetic case and gravitons in the gravitational case. That is
correct in that sense that in Quantum Field Theory, if one applies the
method of perturbation theory to processes where particles are
scattered, one has to calculate the so-called S-matrix in which
mathematical terms occur that look similar to terms that describe the
propagation of particles that belong to field that carries the
interaction that causes the scattering.
Imagine two electrons scattering under the regime of the electromagnetic
field (Moeller scattering). Then in the S-matrix, the so-called photon
propagator occurs. This photon propagator can also be used to describe
the propagation of photons, i.e. particles (field quanta) that belong to
the electromagnetic field. This motivated the terminology that a virtual
photon is exchanged in the scattering process.
However, one should not try to understand this terminology in that way
that it would make sense to imagine a photon emitted from the one
electron and being absorbed by the other one. Perturbation theory does
not give any foundation for such an understanding. The focus of
perturbation theory is to calculate transition probabilities from
initial states (e.g. two electrons coming close) to final states (e.g.
the two electrons moving apart), is tells little about the details of
the scattering process itself.
And most notably, perturbation theory does not say anything about cases
where no scattering processes are involved, e.g. about the way changes
in field configurations do propagate.
>> |
One could quantize Newtonian gravity, but this wouldn't in any way yield
gravitons: there are no dynamical degrees of freedom for the
gravitational field in Newtonian theory, since gravitational field is
fully determined by matter distribution. To yield field quanta, like
photons, graviton, W and Z bosons or gluons, in quantization procedure,
there are dynamical degrees of freedomg required, which are related to
finite propagation speed.
|
> |
I have simulated the forward movement of Mercury and it works when you
introduce cg based on Newton's Law.
|
Maybe you can achieve results that are quantitatively correct in some
cases in this way. But just adding a limited speed of gravity to
Newton's law does not even make up a consistent theory of the
gravitational field. For a consistent theory, there should be e.g. a
field equation where the limited speed is implemented in.
>>> |
These forces act instantaneous
|
>> |
What exludes the occurence of gravitons.
|
> |
I fully agree with you. The forces in Newton's law act instantaneous.
That means cg is infite. The problem is they are "wrong". That means
in some way or an other you have to modify the laws and make cg finite.
|
There is already a well-known modification of Newtonian Gravity: namely
GR. Unlike an approach where you simply make the speed of gravity finite
within the Newtonian framework, GR is widely studied for being consistent.
> |
That allows for the introduction of gravitons.
|
No, your approach where you just claim that the speed of gravity is
finite does not allow for that. Your approach does not in any way define
a field theory to which the methods of field quantization could be applied.
>>> |
What is also important, and that is true for all models, it does not
matter if the objects involved are stars, neutron stars or blackholes:
the basic laws that describe the behaviour (movement) are the same.
|
>> |
In GR, it makes a difference, due to the central singularities in black
holes. For stars or neutron stars, you can use GR field equations in a
numerical field theory approach, but for black holes, you cannot, since
field equations fail at the central singularities. Therfore, black holes
require a different approach.
|
> |
The issue is, what the difference is in behaviour, between a cluster of 10
stars of 50m0 with the same cluster of 10 BH with the same mass.
Simpler is two stars and two BH's with the same mass. Will they merge?
|
Like two black holes that orbit each other, two stars that orbit each
other emit gravitational waves and loose energy by that, making their
orbits closer and closer, until the stars' surfaces begin to touch each
other. The processes that run as soon as the surfaces are touching each
other are surely different from the processes that run in the case of
black holes.
> |
IMO the two stars will not merge. The two BH's will in general only merge
when there is infalling matter.
|
You're wrong. In both cases, the orbits are becoming closer due to
energy loss caused by emitting gravitational waves.
>> |
See, for example, arXiv:1203.5166
|
> |
In this document mainly the technical details of the simulations are
discussed but not the physical implications.
|
The physical implications are well-known: the physical implications of GR.
> |
(For the neutron stars mergers this is different after page 11)
At page 2 they write:
"(in a clean vacuum environment)," Why? Space around BH's is not empty.
|
However, what is in the space around a black hole has a neglectable
influence on the gravitational field. If it has not, Schwarzschild
solution is wrong and the foundation of the simulation, too.
> |
At page 5 they write:
"Gauge conditions and constraint damping terms contain parameters chosen
by trial and error, and mesh structures are tuned based on user experience."
Seems to me dangerous.
|
In numerical approaches, some problems may occur that can be solved for
special situations only, that is correct.
> |
At page 9 they write:
"there were difficulties for the SpEC code to obtain robust and automatic
mergers". Is that wrong?
|
I don't see a reason why that should be wrong.
>> |
for more information.
-- jt]]
|
> |
This article contains the interesting sentence P35:
"That surgery is justified physically since, by definition, the black hole
interior cannot affect the exterior."
I agree with the physical implications (that means there is no singularity
involved)
|
What makes you think the physical implications would mean that there is
no singularity involved?
> |
but not with the logic: by definition.
|
They refere to the fact that (according to GR) the spacetime region
inside a black hole cannot influence the region outside. Where do you
see a problem? If we assume that, in contradiction to GR, the spacetime
region inside the black hole can influcence the region outside, then GR
is wrong and we can immediately forget about a discussing a simulation
that is based on GR.
> |
In fact what counts
is the mass and the radius.
|
I don't see any contradiction: that the mass and radius of black hole
counts for its gravitational field does not in any way change the fact
that the spacetime region inside the black hole cannot influence the
spacetime region outside. The radius is relevant only in that way that
the bigger the radius, the bigger is the interior.
> |
The article amazes me because it discusses a BH encounter with a neutron
star (P37). IMO these type of mergers do "not" produce gravitational waves
|
According to GR, they do.
>>> |
GR IMO also causes a problem specific when the Lorentz transformations
are considered as part of this (physical) model, because these
transformations are based around photons, the speed of light.
|
>> |
Lorentz transformations are related to the quantity c, but not to
photons. Applying Lorentz transformation does not imply considering
electromagnetic waves, still less photons.
|
> |
The issue is what is meant with the parameter c in the Lorentz
transformations. IMO this is the speed of light and not the speed of gravity.
|
If you restrict the symbol c to be the speed of electromagnetic waves,
and introduce another symbol cg for the speed of gravity, then you have
to introduce additional symbols, at least one, that denotes the
connector quantity of space and time, let's write it cs (s for
spacetime). The parameter in the Lorentz transformation is cs then, not c.
> |
Ofcourse you could claim that the two are identical quantities, but physical
they are completely different. Anyway this places the Lorentz transformations
in a "complete different light".
|
Inserting c in the Lorentz transformation after the restriction you made
would place Lorentz transformation in a fully wrong light.
Except you intend to reject SR and develop a theory in which Lorentz
transformation is a property of Electrodynamics.
>>> |
Gravitational waves do not show the lensing effect, photons do.
|
>> |
What do you mean by that? Do you want to say electromagnetic waves are
deflected by a gravitational field due to the gravitational lense
effect, but gravitational wave would not? Then you would be wrong:
gravitational waves are in the same way deflected as electromagnetic waves.
|
> |
I do not understand why you write that (Or I was not clear?)
When the Moon passes between the earth and the Sun from a gravitational
point of view you cannot detect that here on earth.
|
But you can have a look on what GR tells us. GR tells us that
gravitational waves behave in the same way as electromagnetic waves.
24 The two postulates in Special Relativity - part 2
From: Gregor Scholten
Datum: Sunday 7 augustus 2016
>>> |
This article requires carefull study.
At page 33 we read:
"Black holes contain physical spacetime singularities, regions where
the gravitational tidal field (curvature) becomes infinite. It is
crucial, but hardly easy, to choose a computational technique that
avoids encountering those singularities."
|
>> |
Because we are not in Newtonian Gravity, but in GR. GR permits - or
better say: even forces - the condition of a singularity being reached
physically. Imagine a star collapsing to a black hole. According to GR,
the collaps of the star's matter reaches the state of a singularity,
i.e. of infinite density, within finite proper time.
|
> |
GR (as all laws) should be a description of the physical reality.
When a star collapses, somewhere it stops to contract, meaning that the
density physical does not reach infinity i.e a singularity.
|
We don't know that. So far, there isn't any observation that yields any
information about what exactly happens to a collapsing star after it has
deceeded the Schwarzschild radius. So, the statement of GR that the
collaps reaches a singularity state within finite proper time is not in
contradiction to any current observation. Assumed, we will ever make an
obversation that gives evidence of the collaps stopping at a finite
density (even though it is hard to imagine how such an observation could
look like), this would mean a falsification of GR, but currently, no
such observation has been made yet.
Many physics do not feel pretty happy with singularities occuring in GR,
though, an hope that a theory of quantum gravity will yield a way to
prevent singularities, but as long as one programs a simulation based on
GR and not on quantum gravity, one has to implement what GR tells us.
>>> |
At page 33 we also read:
"Finally, different formulations of Einstein's equations behave very
differently when implemented numerically, and we numerical relativists
had to find suitable formulations that generate stable solutions"
|
>> |
This is not about described situations being unstable, but the
*simulation* of such situations being unstable. I once programmed a
simulation of the time evolution of a wave function, ruled by
Schroedinger equation, based on solving the Schroedinger equation
numerically. Several times, I found the simulated wave function rapidly
diverging to infinity. This happened when I chosed the time steps too
rough, what caused to numerical procedure to become unstable. The
situation which I was describing itself isn't unstable, though.
|
> |
IMO there are different problems: 1. The situation can be unstable,
2. the equations are unstable, 3. the numerical solution can be unstable
|
In the article you are referring to, they talk about the numerical
solution becoming unstable. The situation is assumed to be stable.
Unstabilities in sets of interacting bodies that are unstabilities of
the situation are only know from cases where three of more bodies are
involved. Take e.g. a planet in the gravitational field of two nearby
suns (two suns + one planet = three bodies), the trajectory of the
planet is known to easily become unstable then. In a two-body system,
the situation shouldn't become unstable.
Concerning your distinction between category 1 and 2: that doesn't make
sense. The situation being unstable is equivalent to the equations being
unstable. Equations are part of the theoretical description of the
situation. If it follows from the theory that situation is stable, then
the equations are stable, too. What could happen is that the theory
predicts that the situation (and as well the equations) becomes
unstable, but from obversation, we find out that the situation does not
become unstable. Then, the theory is in contradiction to observation,
and by this, falsified. This does not belong to a category "situation is
stable, but equations are unstable", but to the category "theory is
proven to be wrong".
> |
4. or any combination
Step size problems belong in cathegory 3.
The problems I had with implementing the equations outlined in
chapter 15.3 of the book "Introducing Einstein's relativity" belong
in cathegory 2. In these cases the solution is known.
|
As we have seen, category 2 does not make sense. Maybe you could
describe what your problem has been, and what the solution has been, so
that we can analyze to what category it belongs in fact?
As one can read here:
https://de.scribd.com/doc/133470394/Ray-d-Inverno-Introducing-Einstein-s-Relativity-pdf
on page 195, chapter 15.3 of the book you are referring to is about the
advance of the Mercury perihelion. In GR, the advance of the perihelion
is a stable situation, except the advance itself is not considered as
unstability. So, the equations that describe this situation are stable,
too. If you program a numerical solution of the equations, e.g. (15.18),
(15.19) and (15.20), this solution can be unstable (making the simulated
Mercury move oddly instead of simply performing an advance of its
perihelion), but that is what you called category 3 in your enumeration,
not category 2.
>>> |
In such a system all objects are like blackholes.
|
>> |
You mean because you can handle celestial bodies like mass points? You
can do that in Newtonian Gravity, but not in GR.
To program a simulation based on Newtonian Gravity, you can apply a
numerical mechanics approach where you simulate the movement of
particles that are sufficiently described by positions, but in GR, this
does not work pretty well. You are rather obliged to apply a numerical
field theory approach, where space is discretized and you calculate the
participating fields (gravitational field and at least one matter field
that describes the celestial bodies) at the discrete space points.
|
> |
Each such fields must be a 3D field and grid used must have the same
accuracy (or better) as the step size used with Newton's Law.
|
In practice, this is impossible. In numerical mechanics, time is
dicretized, i.e. you calculate quantities at discrete time points
{t_i} = {t0 + i * Delta_t} = {t0, t0 + Delta_t, t0 + 2*Delta_t, ...}
The quantities you calculate are positions of bodies
{x_j(t_i)} = {x_j(t0), x_j(t0 + Delta_t), x_j(t0 + 2*Delta_t), ...}
where j enumerates the bodies and i the time points. The set of possible
body positions is continuous, i.e. the quantities x_j(t_i) are
continuous. In practice, you will use floating number numbers to compute
these quantities, so that they become discrete, with a step size of 1
ULP (unit in the last place), typically something in the order of 10^-15
for double precistion (64 bit) floating point numbers.
In numerical field theory, on the other hand, you do not calculate
positions, but values of fields, at discrete time points and at discrete
points in space:
{(t_i, x_j)} = {(t0 + i * Delta_t, x0 + j * Delta_x)} = {(t0,x0), {t0 +
Delta_t, x0), ..., {t0, x0 + Delta_x), ...}
Here, the spatial steps Delta_x are not only discreate due to the use of
computational numbers, but by definition. In practice, it is impossible
to make the spatial grid that fine that the step size Delta_x is in the
order of 1 ULP. The step size is rather much bigger. Take e.g. a cubic
grid of size 1 x 1 x 1. A step size of 1 ULP (10^-15) would yield an
amount of grid points of 10^45 -> one could never do calculations on
that many points!
In practive, one choses a step size that yields e.g. 100 x 100 x 100 = 1
million points. So, the accuracy is much worse than in numerical
mechanics. If your statement that the accurary had to be the same or
better were correct, this would mean that numerical field theory is
impossible. However, your statement is not correct.
All you have to do is to replace the description of moving bodies as
moving bodies in terms of numerical mechanis by a matter field
description. Instead of describing a body as having a position that
changes continuously (or with 1 ULP discretness) by time, you introduce
a matter field and consider the body as a sharply limited wave packet of
this field.
> |
Not only that after every calculation (dt) the fields change.
|
The interaction-carrying fields as well as the matter fields change, and
the movement of bodies is described by changes of the matter fields (as
propagation of the wave packets).
> |
A different issue is to what extend you have to take size of the objects
involved into account. Paragraph 15.3 mentioned above does not.
|
Because for the topic of paragraph 15.3, the advance of the Mercury
perihelion, a mechanical approach is sufficient: you need to calculate
the trajectory x(t) of Mercury, not the field configuration g_ij(x,t),
since that is presumed to be known as Schwarzschild solution describing
the Sun's gravitational field. And what is notably, too: you do not take
the gravitational field of Mercury into account, you only consider the
Sun's gravitational field. Therefore, the actual size of Mercury is out
of focus.
For a binary black hole system, things are completely different. For
such a system, it is not sufficient any more to consider the
gravitational field of the one black hole (what would be an analytical
Schwarzschild solution, too) and to calculate the trajectory of the
other black hole. Instead, you need to calculate the gravitational field
itself that is caused by the two black holes. In that case, the size of
the objects has to be taken into account, because a field theory
approach is required instead of a mechanical approach.
>>> |
In such a system the speed of light is not considered.
|
>> |
Little correction: the propagation of electromagnetic signals is not
considered. The speed of light, however, is considered, since it is the
speed with which changes in gravitational field do propagate.
|
> |
In that sense, when studying the gravitational field, always the parameter
cg should be mentioned and not the parameter c. This is important because
their physical behavior can be different.
|
Within the framework of GR, the behaviour cannot be different. Changes
in gravitational field always propagate with the same speed like changes
in EM field.
>>> |
There is no
issue if this speed is constant or not. The most(?) important
parameter is cg the speed of gravity propagation. IMO this speed
can be considered constant.
|
>> |
In GR, cg is equal to c. Measured with respect to a general coordinate
system, c may be variable, and so may be cg.
|
> |
I assume that this coordinate system is the same as the grid discussed.
|
The grid should define a coordinate system. One can use that, yes.
> |
The reason that c varies can be gravity (mass).
For cg I do not think that this applies.
|
Then you think that GR is wrong. In GR, cg and c are always the same.
Variation of c implies variation of cg.
>>> |
At page 34 we read:
"and showed that only about 0.1% of the total mass of the blackholes is
radiated away in the collision as gravitational waves"
|
>> |
See you? If you would simulate a black hole merger based on Newtonian
Gravity, there wouldn't be any gravitational waves at all, since
Newtonian Gravity does not know gravitational waves. So, obviously,
Newtonian Gravity is highly inappropriate here.
|
> |
Gravitational waves only become "visible" around binary systems when
test objects are used. Such a test object (at large distance) in circular
orbit shows a sinus function (or wave). The periodicity is the same as the
revolution of the binary system.
In the case of Newton's law the forces involved act instantaneous.
|
And there are no gravitational waves in the cases of Newton's law that
could become visible.
> |
GR assumes that this is not the case; there is a delay.
|
And this delay is related to what make gravitational waves existing:
namely the gravitational field having dynamical degrees of freedom. In a
parallel post, you described a modification of Newtonian Gravity where
you just introduce a limited speed of gravity. That approach is
incomplete, because it does not consider the question whether there are
dynamical degrees of freedom occuring for the gravitational field.
Therefore, it is undefined in this approach whether gravitational waves
do exist.
> |
If you consider gravitons than in the case of GR the speed is finite.
|
This statement does not make sense. Gravitons are assumed to appear in a
theory of quantum gravity. In GR, there no gravitons. So, if you
consider gravitons, you imply that you do not consider GR, but quantum
gravity, so there is no GR case.
In the case of GR, the speed is finite, but without considering gravitons.
>>> |
At page 35 we read:
"In particular, some formulations satisfy criteria that guarantee
stable or otherwise well-behaved solutions, while others do not."
I find this remark disturbing. See above question 1. Suppose the two
objects (BHs?) do not merge, but move apart. Is that wrong?
|
>> |
It is quite obvious that this would be wrong. If two bodies (no matter
if black holes or other celestial bodies) orbit each other initially due
to some attractive force, and then start to move apart, without influx
of energy from outside, then energy conversation must be violated.
|
> |
That not what I have in mind. It has to do with the physical behaviour.
How do we know that BH's (natural) merge?
|
We don't. We know that GR tells us that they do. Und there are recent
observations of gravitational waves that are in agreement to the
prediction of GR that a black hole merger produces strong gravitational
waves that are strong enough to be detected in billions of light years
distance.
> |
Is it not possible that they (natural) move apart?
|
One could imagine that an alternative theory different from GR might
predict that black holes move apart, yes. Although such an theory would
probably be hard to combine with energy conservation. However, in the
simulation that we are discussing, GR is presumed, so black holes should
not move apart in that simulation.
>>> |
At page 36 we read:
"For symmetric binaries, the emissions (gravitational waves) from the two
companions cancel each other, but for asymmetric binaries they do not."
I do not understand. IMO the emission of gravitational energy
for any body of mass M is the same. When they merge (2M) it doubles.
|
>> |
Gravitational waves can interfer, just like EM waves. Imagine two
sources of EM waves, e.g. two accelerated charges. The emitted EM waves
can interfer destructively, making the emitted energy lower than twice
the energy that would be emitted if only one of the two charges were
present.
|
> |
Electric fields are based around positive and negative charges.
|
That is of little relevance for destructive interference. Destructive
interference can also occur with only positive (or only negative)
charges involved. Imagine a torus of e.g. positive charge. If the torus
rotates around its main axis, it does not emit EM radiation. Now cut off
a small segment from the torus and let it revolve around the centre of
the former torus: it radiates!
One can explain this in the following way: when the full torus rotates,
the EM waves generated by the partial charges in the torus interfer
destructively, so there is no radiation emitted in total. After cutting
away the most parts of the torus except the small segment, the remaining
charges generate EM waves that no longer interfer completely
destructively.
> |
By comparison, gravitational fields do not have this distinction.
They are one of a kind.
|
Take this animation of a gravitational waves passing through a set of
test particles:
http://www.einstein-online.info/images/vertiefung/GW_WellenI/cyl_slice.gif
During the first half-cycle, the set is stretched in vertical direction
and shrinked in horizontal direction, in the second half-cycle, it's the
other way round. Now imagine two passing gravitational waves with a phase
difference of 180 degrees: when the one wave tries to stretch the set of
test particles in vertical direction, the other wave tries to shrink the
set in this direction. As result, the set is not streteched or shrinked
at all.
One half-period later, the inverse happens: the first wave tries to
shrink the set in vertical direction, the second wave tries to stretch
it. In total, he set is neither shrinked nor stretched. So, both waves
interfer destructively.
25 The two postulates in Special Relativity - part 2
From: Gregor Scholten
Datum: Monday 8 augustus 2016
Nicolaas Vroom wrote:
>> |
In the actual simulations, you want to simulate the gravitational field.
Or at least the movement of celestial bodies under the regime of
gravity. So, for the gravitational field, c is relevant, because it is
the propagation velocity of changes in the gravitational field.
|
> |
Please let us call this speed cg.
|
You can, if you want, distinguish in GR between the propagation speed of
electromagnetic signals, let's call it cl (l for light), and the
propagation speed of gravitational signals, cg, although theirs values
are always the same. However, you have to define a third quantity then,
the connector quantity between space and time, let's call it cs (s for
spacetime). So, we have cs, cg and cl.
>> |
Of course, you can neglect that if you restrict yourself to consider
the Newtonian limit.
|
> |
Under Newton's law the speed cg is infinite (instantaneous)
|
Another remark to your approach you described in a parallel post where
you modified Newton's law by making cg finite. Newton's law can be
written as
\vec H(\vec r, t) = - (M G / |\vec r - \vec r0(t)|^2) \vec e_{r,r0} (1)
where \vec H is the strength of the gravitational field at the point
\vec r at time t, M the mass of the gravitational centre, \vec r0 the
position of the gravitational centre, and \vec e_{r,r0} the unit vector
from the position of the gravitational centre to the point \vec r.
Now your approach is that you replace the actual position \vec r0(t) of
the gravitational centre at time t by the retarded position
[\vec r0]_ret = \vec r0(t_ret)
i.e. the position for a earlier time t_ret:
\vec H(\vec r, t) = - [(M G / |\vec r - \vec r0|^2) \vec e_{r,r0}]_ret
= - (M G / |\vec r - \vec r0(t_ret)|^2) [\vec e_{r,r0}]_ret (2)
The trouble with this approach is the the non-retarded version (1) is
the solution of a field equation
\div \vec H(\vec r, t) = - rho(\vec r, t) (3)
where \div is the divergence that can be written in Cartesian coordinates as
\div \vec H = \partial_x H_x + \partial_y H_y + \partial_z H_z
and rho is the mass density. In some sense, equation (3) itself can be
considered as Newton's law. For equation (2) however that is constructed
in your approach, you didn't show that it is a solution of a field
equation. Thefore your approach is incomplete.
To get an impression how a field equation that yields a retarding
effect, i.e. a finite speed of gravity, could look like, let's have a
look on Electrodynamics, i.e. on Maxwell equations:
\div \vec E = \rho_el (4a)
\div \vec B = 0 (4b)
\rot \vec E = - \partial_t \vec B (4c)
\rot \vec B = \vec j + \partial_t \vec E (4d)
(4a) looks very similar to (3), and is nothing but the Coulomb law from
Electrostatics. What makes the retarding are equations (4c) and (4d),
that contain the magnetic field besides the electric field. So, for a
retarded gravitational field, one might assume that is not only the
gravitational field \vec H, but as well some "gravitomagnetic" field.
Second, the solutions of the Maxwell equations for an electric charge
that is moving is not simply a electrostatic Coulomb field with
retarding like
\vec E(\vec r, t) = - [(q / (4 pi eps0 |\vec r - \vec r0|^2))
\vec e_{r,r0}]_ret (5)
that would be comparable to the gravitational field (2) from your
approach. E.g. for a uniformly moving charge, equation (5) would yield
an electric field with a direction towards the retarded position of the
charge. However, in fact, Maxwell equation yield a solution for the
electric field of a moving charge where the direction of the field is
towards the *actual* position of the charge.
So, your approach is probably inconsistent.
>> |
Because the movement of celestial bodies is ruled by gravity. And the
speed of light is relevant for the gravitational field. Once again: as
long as you restict yourself to the Newtonian limit, you do not need the
speed of light.
|
> |
Consider a world in which all objects are darkmatter object.
You could also consider a world with only BH's.
Why do you need the speed of light?
|
We do not need cl. But cs and cg.
>>> |
Ofcourse you need light to make observations, but that does not mean
you need the speed of light in order to describe the trajectories of
the objects.
|
>> |
That is trivial. But as already pointed out: in Relativity, c is not
only the speed with which electromagnetic waves propagate, but rather a
general quantity that concerns all laws of physics, e.g. the laws of
mechanics, i.e. the equations that rule the movement of bodies, etc.
|
> |
"I know what Relativity says", but physical photons and gravitons
are completely different "objects" and IMO you should try to study
them independently.
|
In GR, you should not try to study gravitons at all, since gravitons as
quantum gravity objects are incompatible with GR. Accepting a limited
lack of consistency, you can add photons to GR.
If you didn't really intend to refer to quantum theory, but rather used
"photons" and "gravitons" as other words for electromagnetic field and
gravitational field: both fields can be studied independly. However, in
any case, one has to deal with a quantity that is typically denoted c.
In the upper definition, this quantity is neither cl nor cg, but cs.
> |
At page 170 of th earlier book discussed by Ray d'Inverno we read:
"The non-linearity reveals itself physically in the following way:
the gravitational field produced by some source contains energy and
hence, by SR, mass, and this mass in turn is itself a source of a
gravitational field
|
That argument is incompatible with GR. It is rather a little fruitfull
attempt to combine SR and Newtonian Gravity. Since we are talking about
a simulation based on GR, such approaches are little helpful.
In GR, the source of the gravitational field is NOT mass, but the
stress-energy tensor T^ij, a tensor of rank 2. In many cases, this
tensor can be written as
T^ij = diag(rho, p, p, p)
where rho is energy density and p is pressure.
> |
that is to say that the gravitational field
is coupled to itself. This non-linearity means that the equations
are very difficult to solve in general."
This raises immediate two questions: How do you than know
that the equations are correct
|
The equations that come out when trying to combine SR and Newtonian
Gravity are probably not correct. The equations of GR are checked to be
correct by comparing predictions of GR with observations. Those
predictions come from special cases where the field equations have been
succesfully solved analytically. These cases are, amongst others:
- Schwarzschild solution
- Gravitational waves
- Cosmological solutions (Friedmann-Lemaitre-Robertson-Walker metric)
> |
A different question is what does it mean: that you have solved the
equations. In many cases there are no continuous solutions.
The best you can do is to use a numerical solution and solve
the equation step by step in a timewise manner.
|
And after doing so, you have solved the equations, numerically. In the
cases where you have found an analytical solution, you have solved the
equations analytically.
> |
IMO why celestial problems are so difficult is because of lack of
information about the actual gravitational field.
The actual gravitational field here is some type of "superposition" of
the subset gravitational fields caused by all the objects considered.
The problem is that each of these fields we observe here is caused
by the objects in the past.
|
That problem also occurs e.g. in Electrodynamics. However, there it is
easier to solve because Electrodynamics is linear: the EM field
configuration caused by two electric charges is just a linear
combination of two EM field configurations that are each caused by a
single charge. GR, on the other hand, is non-linear: the gravitational
field configutation caused by two celestial bodies is not a simple
superposition, but much more complicated. Therefore, the non-linearity
of GR makes the problem even harder.
>> |
However, such theories are different from GR. And above, you claimed
that you do not intend you reject GR.
|
> |
Reading all about numerical solutions and how difficult this is,
you start thinking are there no different, more simpler solutions
to do a correct simulation of the evolution of the planets.
|
If you want to program a simulation that is in agreement with GR, your
possibilities to imagine simpler solutions are limited. Solutions where
cl, cg and cs have different values are excluded.
>>> |
For me the most important issue to understand is why do you need
c in order to describe the movement of objects i.e. Einstein equations.
|
>> |
Einstein field equations incorporate that changes in the gravitational
field propagate with c. Not only that, Einstein field equations are
based on a four-formalism that is founded on the concept of spacetime,
where c is the connector quantity between space and time. So, any
simulation based on calculations that incorporate Einstein field
equations incorporates the quantity c.
|
> |
I agree, however the issue when you consider numerical solutions, when
you consider that the initial positions and velocities are known,
to what extend do you need the quantity c and cg.
IMO only cg. The quantity c is only used as part of the observations
or when there are electromagnetic fields involved.
A typical case where you need c is when you want to calculate
the Schwarzschild Radius.
|
You're wrong. The quantity c in the formula
rs = 2 G M / c^2
for the Schwarzschild radius is rather cs than cl. In GR, the meaning of
the Schwarzschild radius is that is some kind of geometrization of mass:
a mass M "is" a length of G M / c^2, so that rs = 2 M. Since this
geometrization does not concern the propagation of EM signals (cl) nor
or gravitational signals (cg), the relevant quantity is cs.
> |
Ofcourse you could claim that they have the same strength
|
I guess you wanted to write the same value instead the same stength? A
speed does not have a strength.
> |
For example it is possible that you can solve gravitational fields
in one coordinate system and without moving clocks.
IMO such a consideration would make the equations simpler.
|
This sounds as if you think that Einstein field equations can be written
either in a way where only one coordinate system is involved or in a way
where several coordinate systems (and moving clocks) are involved. Let's
have a look on the field equations:
R_ij + 1/2 R g_ij = T_ij
The quantities R_ij, g_ij and T_ij with two indices i,j are tensors of
2nd level, the indices i and j run each from 0 to 3. In total, each of
the three tensors has 4 x 4 = 16 components, yielding 16 equations, that
can be reduced to 10 due to symmetries of the tensors. Now write the
equations in a single coordinate system, i.e. express the quantities
occuring in the equation in terms that refer to that coordinate system.
There are still 10 equations then.
Now, let's assume you want to write the field equations in a way that
refers not only to one single coordinate system, but to two different
coordinate systems. The only way to do so is to write the equations in
the first coordinate system, yielding 10 equations, and then again in
the second coordinate system, yielding another 10 equations, so that you
have 10 + 10 = 20 equations in total. And if you want to write the field
equations in a way that refers to three coordinate systems, you have 30
equations in the end. And 40 equations for four coordinate systems, and
so on. Of course, you can do that, but it makes little sense, since all
information is present in the first 10 equations. All additional
equations are redundant.
So, writing the field equations in a way that involves only one
coordinate system instead of N coordinate systems make the equations
indeed simpler, by reducing the number of equations from 10 * N to 10,
but that is trivial. Imagine you want to solve Newtonian equation of
motion, m a = F, for a single body. You can, if you want, write this
equation in one inertial frame S, and then again in a second inertial
frame S', and then solve the equation in S and once again in S'. You
double the number of equations by this from one to two, although they
both express exactly the same, and calculate two solutions that or both
the same. Skipping this and solve only one equation is simpler, so your
statement is correct in some sense, but that's trivial.
And of course, any physicist who tries to solve Einsteins field
equations writes these equations as 10 equations in a single coordinate
system, not as 10 * N equations referring to N coordinate systems. So,
you cannot make anything simpler here than it already is usually.
What is involved in Einstien field equations, however, is the property
that they are generally covariant, i.e. that they do not only apply in
the coordinate system in which they are currently written for being
solved, but as well in any other coordinate system. If this property is
what you are talking about: solving the equations in one coordinate
system does not change anything of this property. So, there isn't any
way to make the equations simpler by removing that property. If that is
what you wanted to say.
Concerning moving clocks: I guess you intend to refer to
special-relativistic time dilation when talking about moving clocks? On
the one hand, time dilation is more complicated in GR than in SR, since
time dilation does not only occurd due to movement, but also du to
gravity. On the other hand, you do not need to consider this when
solving Einstein field equations. You can, if you want, use the found
solution to calculate the proper times of clocks, but you are not
obliged to do so.
>>> |
(Assuming no electric or magnetic fields)
How important are the lorentz transformations?
|
>> |
Except in SR limit, Lorentz transformations are rather unimportant in
GR. However, Lorentz transformations formulas are not the only
relativistic equations where c occurs. Einstein field equations contain
c as well.
|
> |
That means when you want to simulate the movements of the planets
using GR you do not need the Lorentz transformations.
|
Exactly.
Even in a special-relativistic theory, like Electrodynamics, you do not
need Lorentz transformations when considering the movement of bodies
that couple to the particular interaction. Considering e.g. the movement
of electric charges in an EM field does not require Lorentz
transformations (but dealing with Lorentz-covariant equations like
Maxwell equations). It's like Einsteins field equations described above:
you can do all the calculations within one single inertial frame, you
do not need to duplicate the equations by considering several inertial
frames.
>> |
It gets rid of coordinate transformations, but not of Einstein field
equations (which contain c).
|
> |
But does it also get rid of moving clocks?
|
Under assumption that you mean the requirement to consider the proper
time of moving bodies when saying "moving clocks": yes. You can
calculate the proper time of the involved bodies, if you want, but it is
not necessarily needed.
26 The two postulates in Special Relativity - part 2
From: Nicolaas Vroom
Datum: Monday 15 augustus 2016
On Friday, 5 August 2016 09:04:06 UTC+2, Gregor Scholten wrote:
> > |
This does not explain why physicists use the concept of singularity.
Singularities IMO are only mathematical constructs, inside the radius
of the BH.
|
> |
If we follow GR, singularities are not only mathematical constructs, but
exist unavoidably.
|
The whole issue in some sense is that you have to make testable
predictions, and singularities and infinities are not part of
these predictions.
> > |
The physical issue is what is the difference between a gravitational
field of a star with mass m0 and a BH with mass m0.
Both at r=0 have a singularity?
|
> |
No. The black hole has a singularity at r = 0 (according to GR), but the
the ordinary star does not. The ordinary star has a non-zero radius and
a finit mass density.
|
IMO a BH also has a non-zero radius and a finite mass density
> > |
That means they use (it seems) special initial conditions
such that the two BH's will merge.
|
> |
No, that does not mean that. The use initial conditions that result in a
collaps to two black holes, which do not immediately merge. Such initial
conditions can e.g. be two ordinary stars that each undergo a collaps to
a black hole. The merger of the two black holes is something that
happens in the later evolution of the binary black hole system.
|
And what causes this to happen?
IMO when both (normal and BH) collect more mass (Energy) than they radiate
they will never merge
> > |
The book by Ray d'Inverno mentioned above in paragraph 15.3 explains
the "Advance of the perihelion of Mercury"
The impression I get is that it is very difficult to simulate more (all?)
planets using GR.
|
> |
You should note that paragraph 15.3 depicts a mechanical approach: the
equations describe the movement of a body (Mercury), not the evolution
of fields. The configuration of the gravitational field is presumed as
known there (namely as being the Schwarzschild solution), so it needn't
be calculated.
|
The issue is here to calculate the movement of all the planets using GR.
My impression is here that this is very difficult
> |
The first difference that occurs that you can no longer apply a
mechanical approach like in Newtonian theory or for the advance of the
Mercury perihelion. You need to calculate the field configuration
applying a field theory approach.
For the advance of the Mercury perihelion, although it belongs to GR,
the mechanical approach is sufficient because the field configuration is
known (from an analytical field theory approach applies by Karl
Schwarzschild in 1917 that yielded Schwarzschild solution). For the
blach hole merger, the field configuration is not known analytically,
therefore a numerical field theory approach is required.
|
This is in line with my assumption that this is very difficult.
It is also in line with the doubt I have if two binary BH always will merge.
Anyway the behaviour of two objects is a physical phenomena.
How sure are we that a binary star system will merge?
> |
According to the result of the simulation we are talking about: yes.
|
I agree with you. But you have to know the details of what is physical
involved.
Is there preference for binary BH's to merge? compared to stars to merge?
Specific when equal masses are considered.
> |
In fact, according to GR, the planets of our solar system do merge:
during their movement around the sun, they emit gravitational waves and
therefore loose energy, making them fall into the sun spirally. However,
the intensity of the emitted gravitational waves is very low, so the
energy loss per time unit is very low, too, and by this, it takes some
10^24 years until all planets have fallen into the sun.
In a close binary black hole system, the energy loss due to
gravitational wave emissions is much higher, so the merger is very much
quicker.
|
The issue is to compare equal masses.
> >> |
Observations of actual astrophysical BHs and their inspiral/mergers
are a whole separate topic, which I'm not going to get into here.
|
> > |
But this is actual very important.
I mean are we sure that BH's actual merge?
|
> |
No, we aren't. However, we are sure that according to GR, they do. And
we have recent observations of gravitational waves that match the
predictions that GR makes concerning gravitational waves emitted during
a black hole merger.
|
I my simulation I assume that a third object is involved. What is wrong
with that?
> > |
When there is an increase in mass they start to merge.
|
> |
You mean in Newton's theory? Then your statement is not correct. In
Newton's theory, it depends on the way the mass is increased. Imagine
two celestial bodies orbitting each other. Imagine the mass of one body
is increased by infalling comets. If the comets fall in that direction
that is opposite to the orbitting direction, they slow down the body
when hitting it, resulting in the orbit becoming closer, like in a
merger scenarion. If the comets fall in the other direction, however,
the body is accelerated, so that the orbit becomes wider.
|
I fully agree with your objections but that does not mean that my
simulation is wrong. In fact you partly agree with me. (50%?)
Nicolaas Vroom
27 The two postulates in Special Relativity - part 2
From: Jonathan Thornburg
Datum: Thursday 18 augustus 2016
Gregor Scholten wrote:
[[many clear and cogent comments with which I entirely agree]]
> |
And of course, any physicist who tries to solve Einsteins field
equations writes these equations as 10 equations in a single coordinate
system, not as 10 * N equations referring to N coordinate systems.
|
While that's usually true, it's not always true: some physicists, e.g.,
Scheel, Pfeiffer, Lindblom, Kidder, Rinne, and Teukolsky
"Solving Einstein's equations with dual coordinate frames"
Physical Review D 74, 104006 (2006)
open-access preprint arXiv:gr-qc/0607056
do in fact (numerically) solve Einstein's field equations using multiple
coordinate systems.
In this paper Scheel at al are numerically simulating orbiting binary
black holes using very different numerical methods (and, indeed,
formulations of the Einstein equations) than those we've discussed
elsewhere in this thread.
[Scheel et al are using pseudospectral methods, rather
than the finite-difference ones we've discussed elsewhere
in this thread.]
Scheel et al find that in order to obtain stable evolutions in their
scheme, they need to setup and solve their numerical equations in a
different coordinate system (frame) near each black hole than than far
away from the black holes. Their numerical scheme includes explicit
transformation equations between the different coordinate systems.
(In fact, the transformations are time-dependent, and are chosen
dynamically during the numerical simulation.)
Scheel et al's scheme is implemented in their SpEC ("Spectral Einstein
Code") numerical code. Of the various numerical-relativity codes which
simulate binary black hole orbits and coalescences, I'd say SpEC is the
most accurate and efficient code. But it's also the most complicated,
and it took the (*very* talented) authors many years to get it to work
well.
So far as I know, SpEC is the only non-finite-difference code to have
successfully simulated binary black hole orbital inspiral and merger;
all the other binary-black-hole codes are finite-difference codes.
[We've generally been discussing finite-difference
codes in this thread.]
Compared to pseudospectral codes, finite-difference codes are somewhat
less accurate (for the same CPU time) or equivalently somewhat less
efficient (in terms of accuracy obtained per CPU time used), but much
simpler, more forgiving of small inconsistencies in (e.g.) boundary
conditions, and generally require less tweaking/tuning of parameters
to simulate novel physical systems.
ciao,
--
-- "Jonathan Thornburg [remove -animal to reply]"
Dept of Astronomy & IUCSS, Indiana University, Bloomington, Indiana, USA
"There was of course no way of knowing whether you were being watched
at any given moment. How often, or on what system, the Thought Police
plugged in on any individual wire was guesswork. It was even conceivable
that they watched everybody all the time." -- George Orwell, "1984"
28 The two postulates in Special Relativity - part 2
From: Jonathan Thornburg
Datum: Friday 19 augustus 2016
Gregor Scholten wrote:
[[snip many clear and cogent comments with which I fully agree]]
> |
And of course, any physicist who tries to solve Einsteins field
equations writes these equations as 10 equations in a single coordinate
system, not as 10 * N equations referring to N coordinate systems.
|
That's not quite true, i.e., there are some (rare) exceptions to this
statement: some physicists, e.g.,
- show quoted text -
29 The two postulates in Special Relativity - part 2
From: Gregor Scholten
Datum: Sunday 28 augustus 2016
Nicolaas Vroom wrote:
>>> |
This does not explain why physicists use the concept of singularity.
Singularities IMO are only mathematical constructs, inside the radius
of the BH.
|
>> |
If we follow GR, singularities are not only mathematical constructs, but
exist unavoidably.
|
> |
The whole issue in some sense is that you have to make testable
predictions, and singularities and infinities are not part of
these predictions.
|
First, it is not forbidden for a theory to make non-testable predictions
besides testable predictions. Second, the collaps to a singularity
indeed is a testable prediction: if a collapsong star stops collapsing
at a non-zero radius and finite density, it is, in principle, possible
to observe that. By this, the prediction that the collaps does not stop
before reaching infinite density can be falsified.
>>> |
The physical issue is what is the difference between a gravitational
field of a star with mass m0 and a BH with mass m0.
Both at r=0 have a singularity?
|
>> |
No. The black hole has a singularity at r = 0 (according to GR), but the
the ordinary star does not. The ordinary star has a non-zero radius and
a finit mass density.
|
> |
IMO a BH also has a non-zero radius and a finite mass density
|
According to GR, the black hole itself has a non-zero radius, namely its
Schwarzschild radius, but the matter of the preceding star has collapsed
to a singularity in the centre of the black hole.
>>> |
That means they use (it seems) special initial conditions
such that the two BH's will merge.
|
>> |
No, that does not mean that. The use initial conditions that result in a
collaps to two black holes, which do not immediately merge. Such initial
conditions can e.g. be two ordinary stars that each undergo a collaps to
a black hole. The merger of the two black holes is something that
happens in the later evolution of the binary black hole system.
|
> |
And what causes this to happen?
|
While orbitting each other, the two black holes loose kinetic energy due
to emission of gravitational waves. Due to that, the orbits become
closer and closer, until the black holes merge. From the analytical
point of view, there is no doubt that this happens. The reason why they
run numerical simulations of this process is not to verify that a merger
happens, but rather to analyze the details of the process, which are
beyond currently known analytical approaches.
> |
IMO when both (normal and BH) collect more mass (Energy) than they radiate
they will never merge
|
Remember my argument of infalling comets from a parallel post: matter
that falls into one of both black holes out of the environment will
sometimes accelerate the orbit velocity and sometimes slow it down. In
the average, changes in the orbit velocity caused by infalling matter
will compensate each other, so infalling matter has no influence on the
black holes doing or not doing merge. The emission of gravitational
waves, on the other hand, does have an influence: it causes the loss of
kinetic energy and therefore the orbits becoming closer and closer.
>>> |
The book by Ray d'Inverno mentioned above in paragraph 15.3 explains
the "Advance of the perihelion of Mercury"
The impression I get is that it is very difficult to simulate more (all?)
planets using GR.
|
>> |
You should note that paragraph 15.3 depicts a mechanical approach: the
equations describe the movement of a body (Mercury), not the evolution
of fields. The configuration of the gravitational field is presumed as
known there (namely as being the Schwarzschild solution), so it needn't
be calculated.
|
> |
The issue is here to calculate the movement of all the planets using GR.
My impression is here that this is very difficult
|
This issue seperates in two different issues:
1) calculate the movements of planets in a known gravitational field
configuration (like the movement of Mercury in the Sun's gravitational
field described by Schwarzschild solution). For this issue, it is
sufficient to solve the geodesic equations for the trajectory of the planet.
2) calculate the movements of celestial bodies taking the gravitational
fields of the bodies themselves into account (like in a binary black
hole system). Here, the gravitational field configuration is not known
and needs to be calculated, too. So, one has to solve a set of coupled
equations, namely geodesic equations and field equations. For a
numerical approach, one can replace solving the geodesic equations for
the trajectories of the bodies by solving field equations for matter
fields that describe the bodies. The approach is a pure field theory
approach then, not a mixture of field theory and mechanics.
Issue 2) is even more difficult than issue 1).
Another remark concering your approach to introduce a finite speed of
gravity to Newtonian Gravity. You said in some other post that in your
simulation, the advance of the Mercury perihelion occured then. The
interesting question is now: did you neglect the gravitational field of
Mercury itself and take only the Sun's gravitational field into account?
Or did you take the gravitational field of Mercury into account, too,
yielding Sun and Mercury both orbit a common centre of mass (that might
be located inside the Sun, but not in the Sun's centre)?
If you neglected the gravitational field of Mercury, the usual approach
would be to consider the Sun resting at the position r = 0 in a
spherical coordinate system (r,theta,phi). The gravitational field of
the Sun would be static then, and a finite speed of gravity wouldn't
have any influence. So, if this was your approach, your result that the
advance of the Mercury perihelion occurs due to the finite speed of
gravity would probably be wrong.
If you, on the other hand, took the gravitational field of Mercury into
account, so that Sun and Mercury orbit a common centre of mass, then a
finite speed of gravity could indeed have some effect, due to the
non-uniform movement of the Sun. However, those effects should depend on
the mass of Mercury: the lower the mass of Mercury, the closer is the
common centre of mass to the centre of the Sun, and the lower are the
changes in the Sun's position. So, the advance of the Mercury perihelion
yielded by your simulation should depend of the mass of Mercury, in
contradiction to GR, where the advance of the perihelion is independent
from Mercury's mass.
>> |
The first difference that occurs that you can no longer apply a
mechanical approach like in Newtonian theory or for the advance of the
Mercury perihelion. You need to calculate the field configuration
applying a field theory approach.
For the advance of the Mercury perihelion, although it belongs to GR,
the mechanical approach is sufficient because the field configuration is
known (from an analytical field theory approach applies by Karl
Schwarzschild in 1917 that yielded Schwarzschild solution). For the
blach hole merger, the field configuration is not known analytically,
therefore a numerical field theory approach is required.
|
> |
This is in line with my assumption that this is very difficult.
It is also in line with the doubt I have if two binary BH always will merge.
|
What makes you think in would be in line with that doubt? That a binary
black hole systemv will merge is out of doubt from the analytical point
of view in GR. The numerical simulations are just run to evaluate the
details of the merger process, not to verify that it happens at all,
since that is already clear analytically.
For comparison, take numerical simulations of Ising model that describes
ferromagnetism. It is well known that a ferromagnatic solid body prefers
to be magnetized under its Curie temperature and de-magnetizes above its
Curie temperature, so, there is a phase transition occuring at Curie
temperature.
In the framework of Ising model, this phase transition can be derived
from an analytical consideration. However, there is a high number of
numerical simulations based on Ising model, using Metropolis algorithm.
The aim of those simulations is not to verify the occurence of a phase
transition (this is already verified analytically), but to examine the
details of the phase transition process.
> |
Anyway the behaviour of two objects is a physical phenomena.
How sure are we that a binary star system will merge?
|
Within the framework of GR, we are very sure, from the analytical point
of view, that a binary star system emits gravitational waves, causing
loss of kinetic energy, and by this, making the orbits closer and
closer. What results in a merger, sooner or later.
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According to the result of the simulation we are talking about: yes.
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And from the analytical point of view, too.
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I agree with you. But you have to know the details of what is physical
involved.
Is there preference for binary BH's to merge? compared to stars to merge?
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Both tend to merge due to emission of gravitational waves that causes
loss of kinetic energy.
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Specific when equal masses are considered.
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Let's consider two extreme cases:
1) Two celestial bodies with very different masses, like the Sun and
Mercury. The centre of mass is located in the Sun, and the Sun does only
little orbitting movement. So, the emission of gravitational waves from
the Sun does not have a very high intensity. Mercury, on the other hand,
does very much more orbitting movement, but its mass is very low. So,
Mercury does not emit gravitational waves with high intensity, too. In
total, the sytem Sun-Mercury does not emit gravitational waves very
strongly.
2) Two celestial bodies of similar (or equal) mass, e.g. a binary star
system. The centre of mass is located in the middle between both stars,
and both perform much orbitting movement. Since their masses are high,
too, they should emit gravitational waves of quite high intensity.
So, roughly estimated, a system of two bodies of similar or equal mass
should yield a higher intensity of gravitational waves emission than a
system of bodies where the one body has much more mass than the other.
So, for equal masses, the loss of kinetic energy is higher, and the
merger is faster.
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Observations of actual astrophysical BHs and their inspiral/mergers
are a whole separate topic, which I'm not going to get into here.
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But this is actual very important.
I mean are we sure that BH's actual merge?
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No, we aren't. However, we are sure that according to GR, they do. And
we have recent observations of gravitational waves that match the
predictions that GR makes concerning gravitational waves emitted during
a black hole merger.
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I my simulation I assume that a third object is involved. What is wrong
with that?
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If we do not restrict ourselves to consider GR, we cannot exclude from
the recent observations of gravitational waves that those waves
originated from a process that involved a third object (or a 4th, 5th,
... object). One could imagine that there might be some theory that
predicts that a system of three bodies produces waves with the observed
characteristics.
If we took Newtonian Gravity, we would immediately know that there were
no gravitational waves, since gravitational waves do not exist in
Newtonian Gravity. So, Newtonian Gravity is in contradiction to the
observation of gravitational waves. If we, one the other hand, take the
approach you described, where you modify Newtonian Gravity by
introducing a finite speed of gravity, we have the problem, that this
approach has a lack of consistency (e.g. because you do not indicate a
field equation), so it is not decidable whether it yields gravitational
waves or not.
If we, on the other hand, restrict ourselves to consider GR, we can be
quite sure the characteristics of the observed gravitational waves are
in good compliance with the characterics GR predicts for a merger of two
black holes. It isn't likely that a system where a third object (of
non-neglectable mass) was involved would produce a similar characteristic.
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