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Black hole formation in the context of dissipative dark matter
Black holes with masses of |$\rm 10^6\text{-}10^9\,M_{\odot }$| dwell in the centres of most galaxies, but their formation mechanisms are not well known. A subdominant dissipative component of dark matter with similar properties to the ordinary baryons, known as mirror dark matter, may collapse to f...
| Autores principales: | , , , , , |
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| Lenguaje: | eng |
| Publicado: |
2018
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1093/mnras/stz608 http://cds.cern.ch/record/2652728 |