Light Particle Solution to the Cosmic Lithium Problem

Andreas Goudelis, Maxim Pospelov, Josef Pradler

Research output: Contribution to journalArticlepeer-review

20 Scopus citations

Abstract

We point out that the cosmological abundance of Li7 can be reduced down to observed values if during its formation, big bang nucleosynthesis is modified by the presence of light electrically neutral particles X that have substantial interactions with nucleons. We find that the lithium problem can be solved without affecting the precisely measured abundances of deuterium and helium if the following conditions are satisfied: the mass (energy) and lifetimes of such particles are bounded by 1.6 MeV≤mX(EX)≤20 MeV and few100s τX 104 s, and the abundance times the absorption cross section by either deuterium or Be7 are comparable to the Hubble rate, nXσabsv∼H, at the time of Be7 formation. We include X-initiated reactions into the primordial nucleosynthesis framework, observe that it leads to a substantial reduction of the freeze-out abundances of Li7+Be7, and find specific model realizations of this scenario. Concentrating on the axionlike-particle case, X=a, we show that all these conditions can be satisfied if the coupling to d quarks is in the range of fd-1∼TeV-1, which can be probed at intensity frontier experiments.

Original languageEnglish (US)
Article number211303
JournalPhysical review letters
Volume116
Issue number21
DOIs
StatePublished - May 25 2016
Externally publishedYes

Bibliographical note

Funding Information:
The work of M. P. is supported in part by NSERC, Canada, and research at the Perimeter Institute is supported in part by the Government of Canada through NSERC and by the Province of Ontario through MEDT.

Publisher Copyright:
© 2016 American Physical Society.

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