Constraints on the Self-Gravity of Radiation Pressure via Big Bang Nucleosynthesis
| dc.creator | Rappaport, Saul | |
| dc.creator | Schwab, Josiah | |
| dc.creator | Burles, Scott | |
| dc.date | 2007-07-24 | |
| dc.date.accessioned | 2026-07-07T08:19:57Z | |
| dc.date.available | 2026-07-07T08:19:57Z | |
| dc.description | Using standard big-bang nucleosynthesis and present, high-precision measurements of light element abundances, we place constraints on the self-gravity of radiation pressure in the early universe. The self-gravity of pressure is strictly non-Newtonian, and thus the constraints we set are a direct test of this aspect of general relativity. | |
| dc.description | 4 pages, 1 figure | |
| dc.identifier | https://arxiv.org/abs/0707.3589 | |
| dc.identifier | http://arxiv.org/abs/0707.3589 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/134946 | |
| dc.subject | Astrophysics | |
| dc.title | Constraints on the Self-Gravity of Radiation Pressure via Big Bang Nucleosynthesis | |
| dc.type | text |