A New General Relativistic Cosmology
| dc.creator | Wagh, Sanjay M. | |
| dc.date | 2002-10-14 | |
| dc.date.accessioned | 2026-07-07T02:05:41Z | |
| dc.date.available | 2026-07-07T02:05:41Z | |
| dc.description | In this work, we outline a new general relativistic cosmology. In this cosmology, the universe originates in the infinite past from sparsely distributed neutral matter and ends in the infinite future as a hot, relativistic plasma. The spatial distribution of matter on the "initial" hyper-surface is {\em arbitrary}. Hence, observed structures can arise in this cosmology from suitable "initial" density contrast. The red-shifts of different objects in this cosmology are indicative of their different states of collapse and need not possess any correlation to their distance from the observer. Further, the microwave background radiation arises in this cosmology as thermalized radiation from all the radiating matter in the universe. This cosmology predicts that the temperature of the microwave background increases with time. Thus, any conclusive evidence that the temperature of the Microwave Background Radiation was more in the past can falsify this cosmology. | |
| dc.description | Revtex4, No Figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0210284 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0210284 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/5175 | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | A New General Relativistic Cosmology | |
| dc.type | text |