Primordial structure of massive black hole clusters

By Maxim Yu. Khlopov, S. Rubin, Alexander S. Sakharov. 2004

196 citations recorded by the source corpus.

Abstract We describe a mechanism of the primordial black holes formation that can explain the existence of a population of supermassive black holes in galactic bulges. The mechanism is based on the formation of black holes from closed domain walls. The origin of such domain walls could be a result of the evolution of an effectively massless scalar field during inflation. The initial non-equilibrium distribution of the scalar field imposed by background de Sitter fluctuations gives rise to the spectrum of black holes, which covers a wide range of masses—from superheavy ones down to deeply subsolar. The primordial black holes of smaller masses are concentrated around the most massive ones within a fractal-like cluster.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/5af6505a086cd081c8c06765b5f097219f5a94b3

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In Astronomy and Astrophysics

  1. B. Carr
  2. Jeremiah P. Ostriker
  3. M. Volonteri
  4. J. Silk
  5. Florian Kuhnel
  6. K. Mack
  7. M. Ricotti
  8. Heling Deng

In Nuclear and High Energy Physics

  1. B. Carr
  2. Florian Kuhnel
  3. Jeremiah P. Ostriker
  4. K. Mack
  5. M. Ricotti
  6. M. Volonteri
  7. Heling Deng
  8. J. Silk

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