pith. sign in

arxiv: 1203.1822 · v1 · pith:5CGPUEZCnew · submitted 2012-03-08 · ✦ hep-th · astro-ph.HE· math-ph· math.MP

Asymptotic Analysis of the Boltzmann Equation for Dark Matter Relics

classification ✦ hep-th astro-ph.HEmath-phmath.MP
keywords asymptoticequationsanalysisbehaviorboltzmannabundancescalculatedcase
0
0 comments X p. Extension
pith:5CGPUEZC Add to your LaTeX paper What is a Pith Number?
\usepackage{pith}
\pithnumber{5CGPUEZC}

Prints a linked pith:5CGPUEZC badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more

read the original abstract

This paper presents an asymptotic analysis of the Boltzmann equations (Riccati differential equations) that describe the physics of thermal dark-matter-relic abundances. Two different asymptotic techniques are used, boundary-layer theory, which makes use of asymptotic matching, and the delta expansion, which is a powerful technique for solving nonlinear differential equations. Two different Boltzmann equations are considered. The first is derived from general relativistic considerations and the second arises in dilatonic string cosmology. The global asymptotic analysis presented here is used to find the long-time behavior of the solutions to these equations. In the first case the nature of the so-called freeze-out region and the post-freeze-out behavior is explored. In the second case the effect of the dilaton on cold dark-matter abundances is calculated and it is shown that there is a large-time power-law fall off of the dark-matter abundance. Corrections to the power-law behavior are also calculated.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.