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arxiv: 1006.4172 · v2 · pith:MVVHWETVnew · submitted 2010-06-21 · ✦ hep-ph · astro-ph.CO

Metastable GeV-scale particles as a solution to the cosmological lithium problem

classification ✦ hep-ph astro-ph.CO
keywords cosmologicalgev-scalemetastableparticlesdecaylithiumobservationsproblem
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The persistent discrepancy between observations of 7Li with putative primordial origin and its abundance prediction in Big Bang Nucleosynthesis (BBN) has become a challenge for the standard cosmological and astrophysical picture. We point out that the decay of GeV-scale metastable particles X may significantly reduce the BBN value down to a level at which it is reconciled with observations. The most efficient reduction occurs when the decay happens to charged pions and kaons, followed by their charge exchange reactions with protons. Similarly, if X decays to muons, secondary electron antineutrinos produce a similar effect. We consider the viability of these mechanisms in different classes of new GeV-scale sectors, and find that several minimal extensions of the Standard Model with metastable vector and/or scalar particles are capable of solving the cosmological lithium problem. Such light states can be a key to the explanation of recent cosmic ray anomalies and can be searched for in a variety of high-intensity medium-energy experiments.

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Cited by 4 Pith papers

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  1. Consistent $N_{\rm eff}$ fitting in big bang nucleosynthesis analysis

    hep-ph 2025-07 unverdicted novelty 6.0

    Conventional BBN fitting for negative Delta N_eff is unphysical; a consistent treatment via entropy dilution after neutrino decoupling yields significantly different bounds.

  2. Bipartite Solution to the Lithium Problem

    hep-ph 2026-04 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.

  3. Nucleosynthesis and CMB bounds on photophilic ALPs: a fresh look

    hep-ph 2025-10 unverdicted novelty 5.0

    Updated model-independent BBN and CMB bounds on photophilic ALPs that incorporate rare decays to light hadrons, show extended constraints for multiple reheating temperatures, and flag parameter space that may alleviat...

  4. Primordial Black Holes Evaporating before Big Bang Nucleosynthesis

    astro-ph.CO 2025-09 unverdicted novelty 4.0

    PBHs must exceed 10^9 g to affect BBN observables, yielding beta upper limits from 10^{-17} to 10^{-19} for masses 10^9-10^10 g, with public code provided.