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Multi-messenger Astronomy with Quenched Superradiance

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arxiv 2406.13756 v2 pith:MCB4W4Z5 submitted 2024-06-19 hep-ph astro-ph.HEgr-qc

classification hep-phastro-ph.HEgr-qc
keywords neutrinofluxbosonssignalsactiveconsidergenerationgravitational
verification ladder T0 review T1 audit T2 compute T3 formal
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We propose a novel method to study the ultra-light bosons, where compact rotating objects undergo the phenomenon of quenched superradiance to create gravitational waves and neutrino flux signals. The neutrino flux results from appropriate coupling between the ultra-light bosons and the neutrinos. We consider a heavy sterile neutrino generation from ultralight scalar, which later results in active neutrino flux through neutrino oscillations, whereas we consider active neutrino generation directly from the vector bosons. We study the intertwining of gravitational waves and neutrino flux signals produced from a single source and elaborate if and when the signals can be detected in existing and upcoming experiments in a direct manner.

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Cited by 1 Pith paper

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

  1. Enlightening dark moments of neutrino with superradiance

    hep-ph 2026-08 conditional novelty 5.0 of 10

    Quenched superradiance of dark photon clouds around spinning primordial black holes could turn neutrino electromagnetic moment bounds into observable neutrino fluxes and limits on PBH abundance.

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