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26 April 2024
 
  » arxiv » astro-ph/9712199

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Cosmological Neutrino Background Revisited
Nickolay Y. Gnedin ; Oleg Y. Gnedin ;
Date 16 Dec 1997
Journal Astrophys.J. 509 (1998) 11-15
Subject astro-ph
AbstractWe solve the Boltzmann equation for cosmological neutrinos around the epoch of the electron-positron annihilation in order to verify the freeze-out approximation and to compute accurately the cosmological neutrino distribution function. We find the radiation energy density to be about 0.3% higher than the one predicted by the freeze-out approximation. As a result, the spectrum of the Cosmic Microwave Background anisotropies changes by 0.3-05%, depending on the angular scale, and the amplitude of the mass fluctuations on scales below about 100 h^{-1} Mpc decreases by about 0.2-0.3%.
Source arXiv, astro-ph/9712199
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