Published February 1986
| Version v1
Journal article
Emission of massive particles from a rotating black hole
Description
The author obtains and analyzes spectral characteristics for Hawking emission of massive spinless and Dirac particles from a Kerr mini black hole in the limit of long waves (uM<wM<<1). The stability of the emission was shown with reference to the formation of a naked singularity. However, in the process of evaporating, the black hole cannot fully lose its angular momentum by the emission of spinless particles
Additional details
Publishing Information
- Journal Title
- Sov. Phys. J. (Engl. Transl.)
- Journal Volume
- 28
- Journal Issue
- 8
- Series
- Sov. Phys. J. (Engl. Transl.).
- Journal Page Range
- 682-684
- ISSN
- 0038-5697
- CODEN
- SOPJA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 18059217
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANGULAR MOMENTUM; BLACK HOLES; COSMIC RADIATION; DIRAC FORM FACTORS; EMISSION SPECTRA; EVAPORATION; FREQUENCY RANGE; KERR METRIC; SINGULARITY; SPIN
- Descriptors DEC
- FORM FACTORS; IONIZING RADIATIONS; METRICS; PARTICLE PROPERTIES; PHASE TRANSFORMATIONS; RADIATIONS; SPECTRA
Optional Information
- Notes
- Cover-to-cover translation of Izvestiya Vysshikh Uchebnykh Zavedenij, Fizika (USSR).