MeV-mass dark matter and primordial nucleosynthesis

Abstract

The annihilation of new dark matter candidates with masses $m_X$ in the MeV range may account for the galactic positrons that are required to explain the 511 keV $\gamma$-ray flux from the galactic bulge. We study the impact of MeV-mass thermal relic particles on the primordial synthesis of ${}^2$H, ${}^4$He, and ${}^7$Li. If the new particles are in thermal equilibrium with neutrinos during the nucleosynthesis epoch they increase the helium mass fraction for $m_X\alt 10$ MeV and are thus disfavored. If they couple primarily to the electromagnetic plasma they can have the opposite effect of lowering both helium and deuterium. For $m_X=4$--10 MeV they can even improve the overall agreement between the predicted and observed ${}^2$H and ${}^4$He abundances.

11 pages, 10 figures, references and two appendices added, conclusions unchanged; accepted for publication in Phys.Rev.D

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