Clustering properties of a sterile neutrino dark matter candidate
arXiv:0807.0646 · doi:10.1103/PhysRevD.78.103505
Abstract
The clustering properties of sterile neutrinos are studied within an extension of the minimal standard model, where these are produced via the decay of a gauge singlet scalar. The distribution function after decoupling is strongly out of equilibrium. (DM) abundance and phase space density constraints from (dSphs) constrain the mass in the range consistent with a gauge singlet with mass and vacuum expectation value decoupling at this temperature. The (DM) transfer function and power spectrum are obtained from the solution of the non-relativistic Boltzmann-Vlasov equation in the matter dominated era. The small momentum enhancement of the distribution function leads to long range memory of gravitational clustering and a \emph{substantial enhancement of the power spectrum at small scales compared to a thermal relic or sterile neutrino produced via non-resonant mixing with active neutrinos}. The scale of suppression of the power spectrum for such sterile neutrino with is . At large scales with . At small scales corrections to the fluid description and memory of gravitational clustering become important, and we find , where is the free streaming wavevector at matter-radiation equality. The enhancement of power at small scales may provide a possible relief to the tension between the constraints from X-ray and Lyman- forest data.
arXiv commentmatches version to appear in PRD
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