Primordial Nucleosynthesis and Dark Matter
| dc.creator | Sarkar, Subir | |
| dc.date | 1996-11-27 | |
| dc.date.accessioned | 2026-07-07T02:22:24Z | |
| dc.date.available | 2026-07-07T02:22:24Z | |
| dc.description | The cosmological abundance of nucleons determined from considerations of Big Bang nucleosynthesis allegedly provides compelling evidence for non-nucleonic dark matter. Recent developments in measurements of primordial light element abundances, in particular deuterium and helium, require reexamination of this important issue. The present situation is uncertain but exciting. | |
| dc.description | 15 pages LaTeX (needs sprocl.sty) including 3 figures (epsf); Invited review to appear in proceedings of the workshop on `Aspects of Dark Matter in Astro- and Particle Physics', Heidelberg, Sept 16-20 1996, eds H.V. Klapdor-Kleingrothaus and Y. Ramachers (World Scientific Press); PostScript available at ftp://ftp.physics.ox.ac.uk/pub/local/users/sarkar/dark96.ps.gz | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9611232 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9611232 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10864 | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Primordial Nucleosynthesis and Dark Matter | |
| dc.type | text |