Degenerate Sub-keV Fermion Dark Matter from a Solution to the Hubble Tension
arXiv:2002.00036 · doi:10.1103/PhysRevD.101.075031
Abstract
We present a dark sector model addressing both the Hubble tension and the core-cusp problem. The model is based on a hidden Abelian gauge symmetry group with some chiral fermions required by the anomaly cancellation conditions, producing a candidate for the decaying fermion dark matter as a solution to the Hubble tension. Moreover, the sub-keV mass regime and the thermal history of the dark sector help the dark matter candidate resolve the core-cusp problem occurring in the standard CDM cosmology.
7 pages, 2 figures, version published in PRD
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