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Boosted Neutrinos and Relativistic Dark Particles as Messengers from Reheating

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arxiv 2007.15006 v1 pith:LTJBPWOW submitted 2020-07-29 hep-ph astro-ph.CO

Boosted Neutrinos and Relativistic Dark Particles as Messengers from Reheating

classification hep-ph astro-ph.CO
keywords reheatinginformationarguedarkeventsinflatonmassmessengers
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Usually information from early eras such as reheating is hard to come by. In this paper we argue that, given the right circumstances, right-handed sterile neutrinos decaying to left-handed active ones at relatively late times can carry information from reheating by propagating freely over the thermal history. For not too small mixing angles, suitable right-handed neutrino masses are around ${\cal O}$(MeV-GeV). We identify the typical spectra and argue that they provide information on the ratio of the inflaton mass to the reheating temperature. This primordial neutrino signal can be strong enough that it can be detected in IceCube. More speculatively, for a reheating temperature and inflaton mass satisfying $T_R={\cal O}(1-100)\, {\rm MeV}$, and $m_\phi={\cal O}(10^{16-19})\,$GeV they may even explain the observed PeV events. Also more general relativistic dark particles can play the role of such messengers, potentially not only allowing for the PeV events but also alleviating the $H_0$-tension .

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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.

  1. Seesaw Cosmology

    hep-ph 2026-07 accept novelty 6.0

    In seesaw reheating, the post-inflation universe can pass through four alternating matter/radiation eras, with the Standard Model temperature falling as a^{-1/4} and then a^{-3/8}, which changes dark-matter production.

  2. The KM3NeT event: a primordial high energy neutrino?

    astro-ph.HE 2026-04 unverdicted novelty 5.0

    The KM3NeT neutrino event may be a primordial neutrino from relic particle decay or annihilation near recombination, yielding a narrow spectral peak that evades broad power-law constraints from other telescopes.