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Dark matter produced from neutrinos

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arxiv 2110.09883 v1 pith:6WG74NQH submitted 2021-10-19 hep-ph astro-ph.CO

classification hep-phastro-ph.CO
keywords neutrinoneutrinosdarkmatterproducedannihilationcosmicdetection
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In the presence of interactions between neutrinos and dark matter (DM), DM can potentially be produced via freeze-in from the neutrino sector. We investigate the implications of such a scenario for the evolution of both DM and neutrinos in the early Universe, and show that the future cosmic neutrino detection experiment PTOLEMY might be sensitive to neutrino signals that originate from DM annihilation in this model.

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Forward citations

Cited by 2 Pith papers

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

  1. New Constraints on Neutrino-Dark Matter Interactions: A Comprehensive Analysis

    hep-ph 2025-07 conditional novelty 6.0 of 10

    Most benchmark neutrino-dark matter couplings adopted in previous studies are excluded when laboratory meson and Z decay bounds are combined with cosmological and astrophysical constraints, leaving only special galact...

  2. Heating the dark matter halo with dark radiation from supernovae

    hep-ph 2024-11 conditional novelty 6.0 of 10

    Even a few parts per million of supernova energy emitted as dark radiation could transform cuspy dwarf dark matter halos into cored ones, and observed core sizes bound how much energy can go to new particles.

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