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Dark matter particles interacting via the exchange of very light spin-0 mediators can have large self-interaction rates and obtain their relic abundance from thermal freeze-out.
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J. L. Feng, M. Kaplinghat, and H.-B. Yu, Sommerfeld Enhancements for Thermal Relic Dark Matter
2010
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2010
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J. Fan, M. Reece, and L.-T. Wang, Non-relativistic effective theory of dark matter direct detection
2010
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A. Loeb and N. Weiner, Cores in Dwarf Galaxies from Dark Matter with a Yukawa Potential
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2015
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2015
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2015
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2015
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2011
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2011
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B. Batell, M. Pospelov, and A. Ritz, Multi-lepton Signatures of a Hidden Sector in Rare B Decays
2011
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2011
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M. Vogelsberger, J. Zavala, and A. Loeb, Subhaloes in Self-Interacting Galactic Dark Matter Haloes
2012
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2012
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2012
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2012
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2015
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2015
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J. M. Cline, K. Kainulainen, P. Scott, and C. Weniger, Update on scalar singlet dark matter
2015
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S. Oshima, T. Fujita, N. Kanda, and A. Yoshimi, Two Pion versus σ \sigma -Meson Exchange Potentials
2015
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2016
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2016
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2016
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2016
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2016
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2016
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2016
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2016
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2016
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2016
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2016
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G. Krnjaic, Probing Light Thermal Dark-Matter With a Higgs Portal Mediator
2016
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2016
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2016
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2016
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2016
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2016
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E. Ma, Self-Interacting Dark Matter with Naturally Light Mediator
2017
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2017
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