Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.222..127p&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 222, no. 1-2, p. 127-145
Astronomy and Astrophysics
Astrophysics
2
Astronomical Models, Background Radiation, Cosmology, Gravitation, Gravitation Theory, Relativity, Cosmic Background Explorer Satellite, Cosmic Dust, Entropy, Lagrangian Function, Red Shift, Tensors
Scientific paper
A previously studied theory of gravitation in flat space-time is applied to homogeneous, isotropic cosmological models. In addition to radiation a two-component fluid model consisting of dust and of a background field is studied. This universe starts from a nonsingular state and expands forever. The energy of radiation, of dust and of the background are emerged from the gravitational energy. Entropy is produced. The age of the universe is infinite measured in units of absolute time whereas the proper-time of the universe is finite. The sum of the density parameters of dust, of radiation and of the background field is about one. There is no flatness and no monopole problem.
No associations
LandOfFree
Nonsingular cosmological model with background field in flat space-time theory of gravitation 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 Nonsingular cosmological model with background field in flat space-time theory of gravitation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nonsingular cosmological model with background field in flat space-time theory of gravitation will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1325787