Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.162..171s&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 162, no. 1, Dec. 1989, p. 171-173.
Astronomy and Astrophysics
Astrophysics
4
Astronomical Models, Universe, Evolution (Development), Gravitational Effects, Quantum Mechanics, Relativistic Effects, Space-Time Functions
Scientific paper
Three versions of the expanding universe models are analyzed. The accelerative variant is represented by the model of a steady-state universe according to which there is a permanent acceleration of hierarchical gravitational-rotating systems (HGRS). The decelerative version is represented by different variants of the standard model of the universe according to which, after the initial explosion, a deceleration of the HGRS arose due to gravitational interaction. The constant version is represented by the nondecelerative variant of the standard model of the universe according to which the HGRS expands at approximately constant velocities during the whole evolution phase of the universe. From the analysis of relativistic quantum-mechanical expanding processes of the universe, it follows that the universe can expand only by the limit velocity of signal propagation c.
No associations
LandOfFree
A note on the problem of choosing a model of the universe. III 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 A note on the problem of choosing a model of the universe. III, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A note on the problem of choosing a model of the universe. III will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1566844