Production of dark-matter bound states in the early universe by three-body recombination

Braaten, Eric; Kang, Daekyoung; Laha, Ranjan

doi:10.1007/JHEP11(2018)084

Title: Production of dark-matter bound states in the early universe by three-body recombination

Journal Article · Tue Nov 13 00:00:00 EST 2018 · Journal of High Energy Physics (Online)

DOI:https://doi.org/10.1007/JHEP11(2018)084· OSTI ID:1602477

Braaten, Eric ^[1]; Kang, Daekyoung ^[2]; Laha, Ranjan ^[3]

The Ohio State Univ., Columbus, OH (United States)
Fudan Univ., Shanghai (China)
Johannes Gutenberg Univ., Mainz (Germany)

The small-scale structure problems of the universe can be solved by self-interacting dark matter that becomes strongly interacting at low energy. A particularly predictive model for the self-interactions is resonant short-range interactions with an S-wave scattering length that is much larger than the range. The velocity dependence of the cross section in such a model provides an excellent fit to self-interaction cross sections inferred from dark-matter halos of galaxies and clusters of galaxies if the dark-matter mass is about 19 GeV and the scattering length is about 17 fm. Such a model makes definite predictions for the few-body physics of weakly bound clusters of the dark-matter particles. The formation of the two-body bound cluster is a bottleneck for the formation of larger bound clusters. We calculate the production of two-body bound clusters by three-body recombination in the early universe under the assumption that the dark matter particles are identical bosons, which is the most favorable case. If the dark-matter mass is 19 GeV and the scattering length is 17 fm, the fraction of dark matter in the form of two-body bound clusters can increase by as much as 4 orders of magnitude when the dark-matter temperature falls below the binding energy, but its present value remains less than 10^-6. The present fraction can be increased to as large as 10^-3 by relaxing the constraints from small-scale structure and decreasing the mass of the dark matter particle.

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Research Organization:: The Ohio State Univ., Columbus, OH (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF); NSFC; German Research Foundation (DFG); European Research Council (ERC)

Grant/Contract Number:: SC0011726; PHY-1607190; 11875112; EXC-1098; KO 4820/1-1; FOR 2239; 637506

OSTI ID:: 1602477

Journal Information:: Journal of High Energy Physics (Online), Vol. 2018, Issue 11; ISSN 1029-8479

Publisher:: Springer BerlinCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 24 works

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Velocity Dependence from Resonant Self-Interacting Dark Matter Chu, Xiaoyong; Garcia-Cely, Camilo; Murayama, Hitoshi Deutsches Elektronen-Synchrotron, DESY, Hamburg https://doi.org/10.3204/pubdb-2019-01981	text	January 2019
Displaced Lepton Jet Signatures from Self-Interacting Dark Matter Bound States Tsai, Yuhsin; Xu, Tao; Yu, Hai-Bo arXiv https://doi.org/10.48550/arxiv.1811.05999	text	January 2018
Baryon-Dark Matter Coincidence in Mirrored Unification Ibe, Masahiro; Kamada, Ayuki; Kobayashi, Shin arXiv https://doi.org/10.48550/arxiv.1907.03404	text	January 2019
Astrophysical probes of inelastic dark matter with a light mediator Alvarez, Gerardo; Yu, Hai-Bo arXiv https://doi.org/10.48550/arxiv.1911.11114	text	January 2019

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