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• W3111450481 abstract "Asymmetric Dark Stars, i.e. compact objects formed from the collapse of asymmetric dark matter could potentially produce a detectable photon flux if dark matter particles self-interact via dark photons that kinetically mix with ordinary photons. The morphology of the emitted spectrum is significantly different and therefore distinguishable from a typical black-body one. Given the above and the fact that asymmetric dark stars can have masses outside the range of neutron stars, the detection of such a spectrum can be considered as a smoking gun signature for the existence of these exotic stars." @default.
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• W3111450481 date "2020-12-05" @default.
• W3111450481 modified "2023-10-16" @default.
• W3111450481 title "Photon spectrum of asymmetric dark stars" @default.
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• W3111450481 doi "https://doi.org/10.1142/s0218271821500036" @default.
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