Dark matter spikes in the vicinity of Kerr black holes

Ferrer, Francesc; Medeiros da Rosa, Augusto; Will, Clifford M.

doi:10.1103/physrevd.96.083014

Title: Dark matter spikes in the vicinity of Kerr black holes

Journal Article · Fri Oct 20 00:00:00 EDT 2017 · Physical Review D

DOI:https://doi.org/10.1103/physrevd.96.083014· OSTI ID:1541089

Ferrer, Francesc ^[1]; Medeiros da Rosa, Augusto ^[1]; Will, Clifford M. ^[2]

Washington Univ., St. Louis, MO (United States). Dept. of Physics. McDonnell Center for the Space Sciences
Univ. of Florida, Gainesville, FL (United States). Dept. of Physics; Univ. Pierre et Marie Curie, Paris (France). GReCO. Institut d’Astrophysique de Paris

The growth of a massive black hole will steepen the cold dark matter density at the center of a galaxy into a dense spike, enhancing the prospects for indirect detection. We study the impact of black hole spin on the density profile using the exact Kerr geometry of the black whole in a fully relativistic adiabatic growth framework. We find that, despite the transfer of angular momentum from the hole to the halo, rotation increases significantly the dark matter density close to the black hole. The gravitational effects are still dominated by the black hole within its influence radius, but the larger dark matter annihilation fluxes might be relevant for indirect detection estimates.

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Research Organization:: Washington Univ., St. Louis, MO (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP)

Grant/Contract Number:: FG02-91ER40628

OSTI ID:: 1541089

Alternate ID(s):: OSTI ID: 1400439

Journal Information:: Physical Review D, Vol. 96, Issue 8; ISSN 2470-0010

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 39 works

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