[Submitted on 1 Jan 2024] (cross-list from hep-ph)
Constraining MeV to 10 GeV majoron by Big Bang Nucleosynthesis
Sanghyeon Chang🇰🇷 · Sougata Ganguly🇰🇷 · Tae Hyun Jung🇰🇷 · Tae-Sun Park🇰🇷 · Chang Sub Shin🇰🇷
We estimate the Big Bang nucleosynthesis (BBN) constraint on the majoron in the mass range between to which dominantly decays into the standard model neutrinos. When the majoron lifetime is shorter than , the injected neutrinos mainly heat up background plasma, which alters the relation between photon temperature and background neutrino temperature. For a lifetime longer than , most of the injected neutrinos directly contribute to the protons-to-neutrons conversion. In both cases, deuterium and helium abundances are enhanced, while the constraint from the deuterium is stronger than that from the helium. abundance gets decreased as a consequence of additional neutrons, but the parameter range that fits the observed abundance is excluded by the deuterium constraint. We also estimate other cosmological constraints and compare them with the BBN bound.
- Comments:
- 12 pages, 3 figures, v2: major revision made by including correct n/p conversion induced by modified thermal neutrinos, slight changes in the result, references added, version accepted in PRD
- Subjects:
- High Energy Physics — Phenomenology (hep-ph); Nuclear Theory (nucl-th)
- arXiv:
- 2401.00687 [pdf]