| Article | |
| Report number | arXiv:1905.05769 ; CERN-TH-2019-070 ; CP3-Origins-2019-20 ; DNRF90 |
| Title | The Photon Spectrum of Asymmetric Dark Stars |
| Author(s) | Maselli, Andrea (INFN, Rome ; Rome U.) ; Kouvaris, Chris (Southern Denmark U., CP3-Origins ; CERN) ; Kokkotas, Kostas D. (Tubingen U., IAAT) |
| Publication | 2020-12-05 |
| Imprint | 2019-05-14 |
| Number of pages | 17 |
| Note | Minor changes to match the version published on IJMPD |
| In: | Int. J. Mod. Phys. D 30 (2021) 2150003 |
| DOI | 10.1142/S0218271821500036 (publication) |
| Subject category | hep-ph ; Particle Physics - Phenomenology ; astro-ph.CO ; Astrophysics and Astronomy |
| 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. |
| Copyright/License | preprint: (License: arXiv nonexclusive-distrib 1.0) publication: © 2021-2024 World Scientific Publishing Company |
Corresponding record in: Inspire
レコード 生成： 2019-05-31, 最終変更： 2023-10-04