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Black Hole in a Radiation-Dominated Universe

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Abstract

We study a black hole in an expanding Universe during the radiation-dominated stage. In particular, such a black hole may be of the primordial origin. In the case when the black hole radius is much smaller than the cosmological horizon, we found a self-consistent solution for the metric and the matter distribution and its velocity far from the black hole. At distances much smaller than the cosmological horizon our solution coincides with the previously obtained solution for quasi-stationary accretion. Our results can be applied, in particular, for the formation of dark matter density spikes around primordial black holes, and for the evolution of dark matter clumps during the radiation-dominated stage.

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Authors and Affiliations

  1. Laboratoire de Physique Theorique, Universite Paris-Saclay, Paris, France

    E. O. Babichev

  2. Institute for Nuclear Research, Russian Academy of Sciences, pr. 60-Letiya Oktyabrya 7a, Moscow, 117312, Russia

    V. I. Dokuchaev & Yu. N. Eroshenko

  3. MEPhI National Research Nuclear University, Kashirskoe sh. 31, Moscow, 115409, Russia

    V. I. Dokuchaev

Authors
  1. E. O. Babichev
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  2. V. I. Dokuchaev
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  3. Yu. N. Eroshenko
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Corresponding author

Correspondence to Yu. N. Eroshenko.

Additional information

Original Russian Text © E.O. Babichev, V.I. Dokuchaev, Yu.N. Eroshenko, 2018, published in Pis’ma v Astronomicheskii Zhurnal, 2018, Vol. 44, Nos. 8–9, pp. 537–545.

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Babichev, E.O., Dokuchaev, V.I. & Eroshenko, Y.N. Black Hole in a Radiation-Dominated Universe. Astron. Lett. 44, 491–499 (2018). https://doi.org/10.1134/S1063773718090013

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  • DOI: https://doi.org/10.1134/S1063773718090013

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