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Journal Article | PUBDB-2022-00387 |
; ;
2021
IOP
London
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Please use a persistent id in citations: doi:10.1088/1475-7516/2021/04/011 doi:10.3204/PUBDB-2022-00387
Report No.: DESY-20-160; ULB-TH/20-15; arXiv:2011.06519
Abstract: In this work, we revise and update model-independent constraints from Big Bang Nucleosynthesis on MeV-scale particles ϕ which decay into photons and/or electron-positron pairs. We use the latest determinations of primordial abundances and extend the analysis in [1] by including all spin-statistical factors as well as inverse decays, significantly strengthening the resulting bounds in particular for small masses. For a very suppressed initial abundance of ϕ, these effects become ever more important and we find that even a pure `freeze-in' abundance can be significantly constrained. In parallel to this article, we release the public code which numerically solves the reaction network necessary to evaluate the effect of photodisintegration on the final light element abundances. As an interesting application, we re-evaluate a possible solution of the lithium problem due to the photodisintegration of beryllium and find that e.g. an ALP produced via freeze-in can lead to a viable solution.
Keyword(s): nucleosynthesis: big bang ; electromagnetic decay ; electron positron ; suppression ; beryllium ; network ; lithium ; photon: energy ; energy dependence ; elements: production
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