http://arxiv.org/abs/1706.08595
We investigate warm dark matter (WDM) features in a model independent approach through the very simple approximation of the Reduced Relativistic Gas (RRG). Our only and generic supposition is a non-negligible velocity $v$ for dark matter particles which is parameterized by a free parameter $b$. We show that high values for WDM velocities would erase radiation dominated epoch. This would cause an early warm matter domination after inflation, unless $b^2\lesssim 10^{-6}$ (or $v\lesssim 300 km/s$). Also it is shown that RRG approach allows to quantify the lack of power in linear matter spectrum at small scales and in particular, reproduces the relative transfer function commonly used in context of WDM with accuracy of $\lesssim 1\%$. This result with such accuracy does not alter significantly the CMB power spectrum agreeing also with the background observational tests. This suggests that the RRG approximation can be used as a complementary approach to investigate consequences of warmness of dark matter and especially for deriving the main observational exponents for the WDM in a model-independent way in linear and non-linear regime.
W. Hipolito-Ricaldi, R. Marttens, J. Fabris, et. al.
Wed, 28 Jun 17
-28/62
Comments: 13 pages, 8 figures
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