b b T = -g p (a,b, = 1,2,3) (1) a a |
1 2 3 4 4 T = T + T + T + T = T -3p (2) 1 2 3 4 4 |
4. Numerical computations |
Page 18 |
4.1 Purpose of these Computationsd |
Page 18 |
4.2 Methods and results of the computations. |
Page 19 |
5. Interpretaion of the resultds |
Page 23 |
Note on a special kind of Singularity in differential Equations |
Page 49 |
Certain comments:
For a concept of density a similar issue exists, assuming density of mass throughout the whole universe. It makes sense to consider only one reference frame.
Het Universum is niet te groot voor de mensheid, het overstijgt noch de mogelijkheden van de wetenschap noch de capaciteiten van de menselijke geest
|
The Universe is not too big for humanity, it neither transcends nor exceeds possibilities of science nor the capabilities of the human mind |
Tijdsafhankelijke evolutie van de schaalfactor van het Heelal in functie van de kosmologische constante voor een ruimte met positieve kromming, door Georges Lemaître, 1927 |
Time-dependent evolution of the scale factor of the Universe as a function of the cosmological constant for a space with positive curvature, by Georges Lemaître, 1927 |
The current physical state of the universe is supposed to be expanding. That means that the outer shell is expanding.
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