The structure of the inhomogeneity field and the formation of primordial black holes

Details The structure of the inhomogeneity field and the formation of primordial black holes The structure of the inhomogeneity field and the formation of primordial black holes

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982azh....59..647z&link_type=abstract

(Astronomicheskii Zhurnal, vol. 59, July-Aug. 1982, p. 647-656) Soviet Astronomy (ISSN 0038-5301), vol. 26, July-Aug. 1982, p. 3

Astronomy and Astrophysics

Astronomy

3

Black Holes (Astronomy), Cosmology, Universe, Mass Spectra, Mathematical Models

Scientific paper

The most probable profile of a large-amplitude perturbation in the early universe will depend on the parameters describing the spatial spectrum of the stochastic field of inhomogeneities. Criteria are obtained such that the accretion of matter and the decay of strong fluctuations will significantly influence the development of the primordial black hole mass spectrum.

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