Published March 2003
| Version v1
Journal article
Baryon asymmetry of the universe from evaporation of primordial black holes
- 1. Institute for Nuclear Research, Russian Academy of Sciences, pr. Shestidesyatiletiya Oktyabrya 7a, Moscow, 117312 (Russian Federation)
Description
The process of baryogenesis through evaporation of black holes formed at the end of the inflation phase is considered. The increase in black hole mass due to accretion from the surrounding radiation after reheating is taken into account. It is shown that the influence of the accretion on the baryogenesis is important only in the case where the initial values of black hole mass are larger than ∼104 g. The behavior of the calculated baryon asymmetry as a function of model parameters is studied
Additional details
Identifiers
- DOI
- 10.1134/1.1563709;
Publishing Information
- Journal Title
- Physics of Atomic Nuclei
- Journal Volume
- 66
- Journal Issue
- 3
- Journal Page Range
- p. 476-480
- ISSN
- 1063-7788
- CODEN
- PANUEO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 35079324
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Translation
- Descriptors DEI
- ASYMMETRY; BARYONS; BLACK HOLES; EVAPORATION MODEL; INFLATIONARY UNIVERSE; MASS
- Descriptors DEC
- COSMOLOGICAL MODELS; ELEMENTARY PARTICLES; FERMIONS; HADRONS; MATHEMATICAL MODELS; NUCLEAR MODELS
Optional Information
- Notes
- Translated from Yadernaya Fizika, ISSN 0044-0027, 66, 504-508 (No. 3, 2003); (c) 2003 MAIK ''Nauka / Interperiodica''.