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Radiative Decay of a Long-Lived Particle and Big-Bang Nucleosynthesis

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abstract

The effects of radiatively decaying, long-lived particles on big-bang nucleosynthesis (BBN) are discussed. If high-energy photons are emitted after BBN, they may change the abundances of the light elements through photodissociation processes, which may result in a significant discrepancy between the BBN theory and observation. We calculate the abundances of the light elements, including the effects of photodissociation induced by a radiatively decaying particle, but neglecting the hadronic branching ratio. Using these calculated abundances, we derive a constraint on such particles by comparing our theoretical results with observations. Taking into account the recent controversies regarding the observations of the light-element abundances, we derive constraints for various combinations of the measurements. We also discuss several models which predict such radiatively decaying particles, and we derive constraints on such models.

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hep-ph 1

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2026 1

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representative citing papers

Bipartite Solution to the Lithium Problem

hep-ph · 2026-04-01 · conditional · novelty 5.0

A sequential majoron-to-neutrinos decay followed by axion-like particle-to-photons decay can lower primordial lithium without exceeding deuterium limits.

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  • Bipartite Solution to the Lithium Problem hep-ph · 2026-04-01 · conditional · none · ref 75 · internal anchor

    A sequential majoron-to-neutrinos decay followed by axion-like particle-to-photons decay can lower primordial lithium without exceeding deuterium limits.