A Simple Way of Calculating Cosmological Relic Density

Abstract

A simple procedure is presented which leads to a dramatic simplification in the calculation of the relic density of stable particles in the Universe.

arXiv comment7 pages in LaTex, no figures; University of Michigan preprint UM-TH-94-02 (February 1994). Changes: a coefficient in $b^0$ (Eq. 16) corrected; added Acknowledgements and revised Note Added; plain LaTex only (no need to use RevTex)

References in corpus (1)

• The Neutralino Relic Density in Minimal N=1 Supergravity

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• Towards An Accurate Calculation of the Neutralino Relic Density
• SUSY spectrum constraints on direct dark matter detection
• About direct Dark Matter detection in Next-to-Minimal Supersymmetric Standard Model
• Extra-Dimensions and Dark Matter
• Electroweak fragmentation functions for dark matter annihilation
• Flavor structure, Higgs boson mass and dark matter in supersymmetric model with vector-like generations