publication . Article . Preprint . Other literature type . 2018

Black hole formation in the context of dissipative dark matter

Muhammad A. Latif; G. D'Amico; G. D'Amico; Paolo Panci; Alessandro Lupi; Dominik R. G. Schleicher; S. Bovino;
Open Access
  • Published: 07 Dec 2018 Journal: Monthly Notices of the Royal Astronomical Society, volume 485, pages 3,352-3,359 (issn: 0035-8711, eissn: 1365-2966, Copyright policy)
  • Publisher: Oxford University Press (OUP)
Black holes with masses of $\rm 10^6-10^9~M_{\odot}$ dwell in the centers 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 form massive black holes during the epoch of first galaxies formation. In this study, we explore the possibility of massive black hole formation via this alternative scenario. We perform three-dimensional cosmological simulations for four distinct halos and compare their thermal, chemical and dynamical evolution in both the ordinary and the mirror sectors. We find that the collap...
arXiv: Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics::Galaxy AstrophysicsAstrophysics::High Energy Astrophysical PhenomenaGeneral Relativity and Quantum Cosmology
free text keywords: Space and Planetary Science, Astronomy and Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies, High Energy Physics - Phenomenology, hep-ph, Particle Physics - Phenomenology, astro-ph.GA, Astrophysics and Astronomy, astro-ph.CO, Astrophysics, Baryon, Dissipative system, Black hole, Physics, Thermal, Galaxy, Fragmentation (computing), Dark matter, Halo
Funded by
The Interstellar Medium of High Redshift Galaxies
  • Funder: European Commission (EC)
  • Project Code: 740120
  • Funding stream: H2020 | ERC | ERC-ADG
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