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Neutron stars contain a significant number of stable muons due to the large chemical potential and degenerate electrons.
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N. F. Bell, G. Busoni, and S. Robles, “Capture of Leptophilic Dark Matter in Neutron Stars,” JCAP
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D. Page, J. M. Lattimer, M. Prakash, and A. W. Steiner, “Minimal cooling of neutron stars: A New paradigm,” Astrophys. J. Suppl
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G. Belanger, F. Boudjema, A. Pukhov, and A. Semenov, “MicrOMEGAs 2.0: A Program to calculate the relic density of dark matter in a generic model,” Comput. Phys. Commun
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2009
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2009
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2010
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C. Kouvaris and P. Tinyakov, “Can Neutron stars constrain Dark Matter?,” Phys. Rev
2010
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2011
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C. Kouvaris and P. Tinyakov, “Excluding Light Asymmetric Bosonic Dark Matter,” Phys. Rev. Lett
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2012
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2016
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G. Bertone and T. M. P. Tait, “A new era in the search for dark matter,” Nature
2018
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2018
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N. F. Bell, G. Busoni, and S. Robles, “Heating up Neutron Stars with Inelastic Dark Matter,” JCAP
2018
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Y. Kahn, G. Krnjaic, N. Tran, and A. Whitbeck, “M 3
2018
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S. Tulin and H.-B. Yu, “Dark Matter Self-interactions and Small Scale Structure,” Phys. Rept
2018
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2019
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