Published May 1981
| Version v1
Journal article
Rotating black holes as dissipative spin-thermodynamical systems
Description
A black hole is interpreted as an ''open system'' in the Prigogine sense. From the point of view of spin transformations, the existence of a phase transition corresponding to an extreme Kerr hole is recognized. The role played by the spin entropy into superradiance of a rotating black hole is investigated. (author)
Additional details
Publishing Information
- Journal Title
- Gen. Relativ. Gravitation
- Journal Volume
- 13
- Journal Issue
- 5
- Series
- Gen. Relativ. Gravitation.
- Journal Page Range
- 417-423
- ISSN
- 0001-7701
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United Kingdom
- INIS RN
- 13652083
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BLACK HOLES; ENERGY LOSSES; ENTROPY; KERR FIELD; PHASE TRANSFORMATIONS; PRIGOGINE THEOREM; ROTATION; SPIN; THERMODYNAMICS
- Descriptors DEC
- ANGULAR MOMENTUM; GRAVITATIONAL FIELDS; PARTICLE PROPERTIES; PHYSICAL PROPERTIES; THERMODYNAMIC PROPERTIES