Published July 1982
| Version v1
Journal article
The structure of the inhomogeneity field and the formation of primordial black holes
Description
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
Additional details
Publishing Information
- Journal Title
- Sov. Astron. (Engl. Transl.)
- Journal Volume
- 26
- Journal Issue
- 4
- Series
- Sov. Astron. (Engl. Transl.).
- Journal Page Range
- 395-401
- ISSN
- 0038-5301
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 14781631
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BACKGROUND RADIATION; BLACK HOLES; COSMOLOGICAL MODELS; COSMOLOGY; DISTURBANCES; FLUCTUATIONS; MASS; STAR ACCRETION; VARIATIONS
- Descriptors DEC
- MATHEMATICAL MODELS; RADIATIONS; STAR EVOLUTION
Optional Information
- Notes
- Cover-to-cover translation of Astronomicheskij Zhurnal (USSR).