Gravitino or Axino Dark Matter with Reheat Temperature as high as GeV
arXiv:1611.05028 · doi:10.1007/JHEP03(2017)005
Abstract
A new scheme for lightest supersymmetric particle (LSP) dark matter is introduced and studied in theories of TeV supersymmetry with a QCD axion, , and a high reheat temperature after inflation, . A large overproduction of axinos () and gravitinos () from scattering at , and from freeze-in at the TeV scale, is diluted by the late decay of a saxion condensate that arises from inflation. The two lightest superpartners are , with mass of order the TeV scale, and with mass anywhere between the keV and TeV scales, depending on the mediation scale of supersymmetry breaking. Dark matter contains both warm and cold components: for LSP the warm component arises from , while for LSP the warm component arises from . The free-streaming scale for the warm component is predicted to be of order 1 Mpc (and independent of in the case of LSP). can be as high as GeV, for any value of , solving the gravitino problem. The PQ symmetry breaking scale depends on and and can be anywhere in the range GeV. Detailed predictions are made for the lifetime of the neutralino LOSP decaying to and , which is in the range of m over much of parameter space. For an axion misalignment angle of order unity, the axion contribution to dark matter is sub-dominant, except when approaches GeV.
arXiv comment43 pages, 16 figures
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