Decays of heavy relic particles into neutrinos are far more constrained by Big Bang nucleosynthesis than previously thought, once neutrino-neutrino scattering and hadrodisintegration are included.
Neutrino lines from DM decay induced by high-scale seesaw interactions
1 Pith paper cite this work. Polarity classification is still indexing.
abstract
If the stability of the dark matter (DM) particle is due to an accidental symmetry, nothing prevents UV physics from destabilising it by inducing DM decays suppressed by powers of the UV scale. The seesaw physics, presumably at the origin of neutrino mass, could induce such a decay. We show that if the seesaw scale lies around the usual Weinberg operator scale, the induced DM decay could generically lead to neutrino lines whose intensity is of the order of the present sensitivity of neutrino telescopes. We illustrate this possibility with models in which the DM is made of the gauge boson(s) of an abelian or non-abelian gauge symmetry.
fields
hep-ph 1years
2025 1verdicts
ACCEPT 1representative citing papers
citing papers explorer
-
Photo- and Hadrodisintegration constraints on massive relics decaying into neutrinos
Decays of heavy relic particles into neutrinos are far more constrained by Big Bang nucleosynthesis than previously thought, once neutrino-neutrino scattering and hadrodisintegration are included.