Post-Inflation Reheating in an Expanding Universe

Details Post-Inflation Reheating in an Expanding Universe Post-Inflation Reheating in an Expanding Universe

1995-07-26

arxiv.org/abs/astro-ph/9507108v3

Phys.Rev. D53 (1996) 1776-1783

Astronomy and Astrophysics

Astrophysics

18pp. Plain LaTeX; no figures. Final revised version. To appear in Physical Review D, 15 February 1996

Scientific paper

10.1103/PhysRevD.53.1776

An analytic means of studying the resonant decay of the inflaton field is
developed for the case of background expansion, $H \neq 0$. It is shown that
the parametric resonance in the inflaton's decay need not disappear when the
expansion of the universe is taken into account, although the total number of
particles produced is fewer than in the $H \simeq 0$ case.

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