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Degenerate Sub-keV Fermion Dark Matter from a Solution to the Hubble Tension

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arxiv 2002.00036 v2 pith:SPZZWZU7 submitted 2020-01-31 hep-ph astro-ph.COastro-ph.GA

classification hep-phastro-ph.COastro-ph.GA
keywords darkhubblemattertensioncandidatecore-cuspfermionmodel
verification ladder T0 review T1 audit T2 compute T3 formal

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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 $\Lambda$CDM cosmology.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

    astro-ph.CO 2019-08 conditional novelty 5.0 of 10

    An interacting dark energy model with coupling proportional to the dark energy density alleviates the H0 and S8 tensions in Planck 2018 data but is not preferred once BAO and supernova data are included.

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