Cosmic Temperature Decline in the Course of the Evolution of the Universe

Details Cosmic Temperature Decline in the Course of the Evolution of the Universe Cosmic Temperature Decline in the Course of the Evolution of the Universe

2001-11-08

arxiv.org/abs/astro-ph/0111163v1

Appendix C, pages 185 - 188, in: M. Carmeli, "Cosmological Special Relativity: The Large-Scale Structure of Space, Time and Ve

Astronomy and Astrophysics

Astrophysics

5 pages in LaTeX, to be published

Scientific paper

At the early stage of the Universe-evolution there were no stars and no galaxies, but only a uniform hot plasma consisting of free electrons and free nuclei. The Universe temperature was determined by the Stefan-Boltzmann law of thermodynamics and the general relativistic cosmological theory. At the present time one has the background cosmic radiation with the temperature of 2.73K. We calculate how much of the early Universe energy has gone to matter and other forms of energy, so as to leave us with a background radiation of only 2.73K.

Affiliated with

Also associated with

No associations

Rating

Cosmic Temperature Decline in the Course of the Evolution of the Universe does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Cosmic Temperature Decline in the Course of the Evolution of the Universe, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmic Temperature Decline in the Course of the Evolution of the Universe will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-421142