From (p)reheating to nucleosynthesis

Details From (p)reheating to nucleosynthesis From (p)reheating to nucleosynthesis

2001-12-10

arxiv.org/abs/astro-ph/0112226v1

Class.Quant.Grav. 19 (2002) 3417-3434

Astronomy and Astrophysics

Astrophysics

18 pages, 6 figures, to be published in "Classical and Quantum Gravity", article based on a talk presented at ``The Early Univ

Scientific paper

10.1088/0264-9381/19/13/303

This article gives a brief qualitative description of the possible evolution of the early Universe between the end of an inflationary epoch and the end of Big Bang nucleosynthesis. After a general introduction, establishing the minimum requirements cosmologists impose on this cosmic evolutionary phase, namely, successful baryogenesis, the production of cosmic dark matter, and successful light-element nucleosynthesis, a more detailed discussion on some recent developments follows. This latter includes the physics of preheating, the putative production of (alternative) dark matter, and the current status of Big Bang nucleosynthesis.

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