The Cosmic Neutrino Background Anisotropy - Linear Theory
arXiv:0910.4578 · doi:10.1088/1475-7516/2010/03/020
Abstract
The cosmic neutrino background anisotropy is calculated for massive neutrino states by solving the full Boltzmann equation. The effect of weak gravitational lensing, including the Limber approximation, is also derived for massive particles, and subsequently applied to the case of massive neutrinos.
16 pages, 8 figures, JCAP format
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- Influence of local structure on relic neutrino abundances and anisotropies
- Geodesic motion and phase-space evolution of massive neutrinos
- How much cosmological information can be measured?
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- Decaying neutrinos: The long way to isotropy
- The connection between cosmology and neutrino physics