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      Constraints on Light Dark Matter from Big Bang Nucleosynthesis

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          Abstract

          We examine the effects of relic dark matter annihilations on big bang nucleosynthesis (BBN). The magnitude of these effects have scale simply with the dark matter mass and annihilation cross-section, which we derive. Estimates based on these scaling behaviors indicate that BBN severely constrains hadronic and radiative dark matter annihilation channels in the previously unconsidered dark matter mass region MeV \(\lesssim m_{\chi} \lesssim 10\) GeV. Interestingly, we find that BBN constraints on hadronic annihilation channels are competitive with similar bounds derived from the cosmic microwave background.

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          Unitarity limits on the mass and radius of dark-matter particles

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            Cold and Fuzzy Dark Matter

            Cold dark matter (CDM) models predict small-scale structure in excess of observations of the cores and abundance of dwarf galaxies. These problems might be solved, and the virtues of CDM models retained, even without postulating {\it ad hoc} dark matter particle or field interactions, if the dark matter is composed of ultra-light scalar particles (m ~ 10^{-22}eV), initially in a (cold) Bose-Einstein condensate, similar to axion dark matter models. The wave properties of the dark matter stabilize gravitational collapse providing halo cores and sharply suppressing small-scale linear power.
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              Primordial nucleosynthesis: The effects of injecting hadrons

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                Author and article information

                Journal
                29 May 2012
                Article
                1205.6479
                ed6a75c7-c782-40cd-899b-155baca6a649

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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                13 pages, 1 figure
                hep-ph

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