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Spherical Gravitational Collapse of Annihilating Dark Matter and the Minimum Mass of CDM Black Holes

arXiv:astro-ph/0505497 · doi:10.1088/1475-7516/2005/11/004

Abstract

Spherical gravitational collapse of a cold gas of annihilating particles involves a competition between the free-fall rate and the (s-wave) annihilation rate . Thus, there is a critical density $\rhoann$ above which annihilation proceeds faster than free fall. Gravitational collapse of a cloud of (initial) mass to a black hole is only possible if $3/32πG^3M^2\lesssim\rhoann$, or $M\gtrsim\Mann\equiv (3/32πG^3\rhoann)^{1/2}$. For a particle mass and freeze-out temperature , the minimum black hole mass is $\Mann\approx 10^{10}\msun \times(x_f\sqrt{g_\star}/100\omcdm g_{\star S}m({\rm Gev}))$, where and are degeneracy factors. The formation of a black hole of initial mass is accompanied by the annihilation of about released in a burst lasting a time that could reach a total annihilation luminosity . The absence of astronomical observations of such spectacular events suggests either: (i) the branching ratio for CDM annihilation to pairs or quarks , while the branching ratio to is ; or (ii) CDM is not made of annihilating particles, but may be in some non-annihilating form, such as axions; or (iii) CDM black holes never form.

Spherical Gravitational Collapse of Annihilating Dark Matter and the Minimum Mass of CDM Black Holes · wovepaper