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2017

Cosmic abundances of SIMP dark matter

Choi, Soo-Min, Lee, Hyun Min, Seo, Min-Seok

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Thermal production of light dark matter with sub-GeV scale mass can be attributed to $3\rightarrow 2$ self-annihilation processes.

We consider the thermal average for annihilation cross sections of dark matter at $3\rightarrow 2$ and general higher-order interactions.
A correct thermal average for initial dark matter particles is important, in particular, for annihilation cross sections with overall velocity dependence and/or resonance poles.
We apply our general results to benchmark models for SIMP dark matter and discuss the effects of the resonance pole in determining the relic density.

Cosmic abundances of SIMP dark matter · Around

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Cited in the paper.
S. M. Choi, Y. Hochberg, E. Kuflik, H. M. Lee, Y. Mambrini, H. Murayama and M. Pierre, To appear
Cited in the paper.
U. K. Dey, T. N. Maity and T. S. Ray, arXiv:1612.09074 [hep-ph]; J. Cline, H. Liu, T. Slatyer and W. Xue, arXiv:1702.07716 [hep-ph]
Original
Cited in the paper.

Then

S. M. Choi and H. M. Lee, Phys. Lett. B 758
Original
2016
Later among the works it cites.
S. M. Choi, Y. J. Kang and H. M. Lee, JHEP 1612
Original
2016
Later among the works it cites.
Y. Hochberg, E. Kuflik and H. Murayama, JHEP 1605
Original
2016
Later among the works it cites.
N. Bernal and X. Chu, JCAP 1601
Original
2016
Later among the works it cites.

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