Thermodynamics of Expansive Nondecelerative Universe
| dc.creator | Sukenik, Miroslav | |
| dc.creator | Sima, Jozef | |
| dc.date | 2001-06-25 | |
| dc.date.accessioned | 2026-07-07T03:26:02Z | |
| dc.date.available | 2026-07-07T03:26:02Z | |
| dc.description | The present contribution deals with thermodynamic aspects of the model of Expansive Nondecelerative Universe. In this model, in the matter era a dependence T^CBR ~ E^CBR ~ a(exp -3/4) holds for the energy of cosmic background radiation, E^CBR and its temperature T^CBR, while the proportionality of the energy density epsilon^CBR to the gauge factor a can be expressed as epsilon^CBR ~ a(exp -3). The given relationships comply with experimental observations of the cosmic background radiation as well as with a surprising finding that the Universe expansion is not decelerated by gravitational forces. It is rationalized that the specific entropy is proportional to a(exp -1/4), i.e. it is gradually decreasing in time. | |
| dc.description | 8 pages, LaTeX | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0106078 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0106078 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/33941 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Thermodynamics of Expansive Nondecelerative Universe | |
| dc.type | text |