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| Journal Article | PUBDB-2026-01004 |
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2025
IOP
London
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Please use a persistent id in citations: doi:10.1088/1475-7516/2025/11/072 doi:10.3204/PUBDB-2026-01004
Report No.: DESY-25-056; ULB-TH/25-03; arXiv:2505.01492
Abstract: We perform a detailed study of the cosmological constraints on the decay of a relic particle ϕ into neutrinos, ϕ → νν̅, in particular those arising from the observed light-element abundances in the early Universe. Several processes are relevant, including final-state radiation associated with the decay, as well as subsequent interactions of the injected neutrinos with the thermal background neutrinos or between themselves. All processes generically contribute to the production of electromagnetic and often also hadronic material and may therefore induce late-time photodisintegration and hadrodisintegration reactions, i.e. the destruction of light elements that have previously been formed during BBN. Here, we examine this scenario with a Monte-Carlo inspired probabilistic approach rather than Boltzmann techniques, taking into account all of these different reactions as well as their interplay. We find the resulting constraints to be very significant, covering a broad range of previously unexplored masses and lifetimes of the relic source particle.
Keyword(s): big bang nucleosynthesis ; cosmological neutrinos ; physics of the early universe
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Photo- and Hadrodisintegration constraints on massive relics decaying into neutrinos
[10.3204/PUBDB-2025-01239]
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