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Indirect Signals from Solar Dark Matter Annihilation to Long-lived Right-handed Neutrinos

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arxiv 1612.03110 v1 pith:ZHLBXD6K submitted 2016-12-09 hep-ph astro-ph.HE

classification hep-phastro-ph.HE
keywords solardarkdetectionneutrinoneutrinossignalsannihilationbounds
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

We study indirect detection signals from solar annihilation of dark matter (DM) particles into light right-handed (RH) neutrinos with a mass in a $1-5$ GeV range. These RH neutrinos can have a sufficiently long lifetime to allow them to decay outside the Sun and their delayed decays can result in a signal in gamma rays from the otherwise `dark' solar direction, and also a neutrino signal that is not suppressed by the interactions with solar medium. We find that the latest Fermi-LAT and IceCube results place limits on the gamma ray and neutrino signals, respectively. Combined photon and neutrino bounds can constrain the spin-independent DM-nucleon elastic scattering cross section better than direct detection experiments for DM masses from 200 GeV up to several TeV. The bounds on spin-dependent scattering are also much tighter than the strongest limits from direct detection experiments.

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Cited by 2 Pith papers

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  1. Complementary Planetary Spectroscopy Probes of Dark Matter

    hep-ph 2025-08 conditional novelty 6.0 of 10

    Dark matter annihilation energy deposited in planetary atmospheres and interiors, compared against existing UV airglow and heat flow measurements, yields new sub-GeV scattering constraints and long-lived mediator reach.

  2. Structures of the Massive Vector Boson Propagators at Finite Temperature Illuminated by the Goldstone Equivalence Gauge

    hep-ph 2019-08 conditional novelty 6.0 of 10

    At finite temperature, a massive vector boson's longitudinal mode sheds part of its Goldstone component, which reappears as a branch cut that can be approximated as a massless quasi-Goldstone with a computed wave-func...

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