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• W3100411109 abstract "We study in detail how neutrino perturbations can be followed in linear theory by using only terms up to l=2 in the Boltzmann hierarchy. We provide a new approximation to the third moment and demonstrate that the neutrino power spectrum can be calculated to a precision of better than ∼ 5% for masses up to ∼ 1 eV and k ≲ 10 h/Mpc. The matter power spectrum can be calculated far more precisely and typically at least a factor of a few better than with existing approximations. We then proceed to study how the neutrino power spectrum can be reliably calculated even in the non-linear regime by using the non-linear gravitational potential, sourced by dark matter overdensities, as it is derived from semi-analytic methods based on N-body simulations in the Boltzmann evolution hierarchy. Our results agree extremely well with results derived from N-body simulations that include cold dark matter and neutrinos as independent particles with different properties." @default.
• W3100411109 created "2020-11-23" @default.
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• W3100411109 date "2016-06-08" @default.
• W3100411109 modified "2023-09-23" @default.
• W3100411109 title "Efficient calculation of cosmological neutrino clustering in the non-linear regime" @default.
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• W3100411109 doi "https://doi.org/10.1088/1475-7516/2016/06/018" @default.
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