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Primordial Structure of Massive Black Hole Clusters

Maxim. Yu. Khlopov·Sergei. G. Rubin·Alexander. S. Sakharov
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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.

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Maxim. Yu. Khlopov, Sergei. G. Rubin, Alexander. S. Sakharov. 2004-12-13. Primordial Structure of Massive Black Hole Clusters. https://doi.org/10.1016/j.astropartphys.2004.12.002

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