General limit on the relation between abundances of D and Li in big bang nucleosynthesis with nucleon injections
arXiv:1404.3090 · doi:10.1103/PhysRevD.90.045009
Abstract
The injections of energetic hadrons could have occurred in the early universe by decays of hypothetical long-lived exotic particles. The injections induce the showers of nonthermal hadrons via nuclear scattering. Neutrons generated at these events can react with Be nuclei and reduce Be abundance solving a problem of the primordial Li abundance. We suggest that thermal neutron injection is a way to derive a model independent conservative limit on the relation between abundances of D and Li in a hadronic energy injection model. We emphasize that an uncertainty in cross sections of inelastic scattering affects the total number of induced neutrons, which determines final abundances of D and Li. In addition, the annihilations of antinucleons with He result in higher D abundance and trigger nonthermal Li production. It is concluded that a reduction of Li abundance from a value in the standard big bang nucleosynthesis (BBN) model down to an observational two upper limit is necessarily accompanied by an undesirable increase of D abundance up to at least an observational 12 upper limit from observations of quasi-stellar object absorption line systems. The effects of antinucleons and secondary particles produced in the hadronic showers always lead to a severer constraint. The BBN models involving any injections of extra neutrons are thus unlikely to reproduce a small Li abundance consistent with observations.
14 pages, 6 figures
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