Published November 15, 1987
| Version v1
Journal article
Thermal conduction and gravitational collapse
Creators
- 1. Departamento de Fsica, Facultad de Ciencias, Universidad Central de Venezuela, Caracas, Venezuela
Description
A method used to study the evolution of radiating spheres, reported some years ago by Herrera, Jimenez, and Ruggeri, is extended to the case in which thermal conduction within the sphere is taken into account. By means of an explicit example it is shown that heat flow, if present, may play an important role, affecting the final outcome of collapse
Additional details
Publishing Information
- Journal Title
- Phys. Rev., D
- Journal Volume
- 36
- Journal Issue
- 10
- Series
- Phys. Rev., D.
- Journal Page Range
- 2986-2993
- ISSN
- 0556-2821
- CODEN
- PRVDA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 19033725
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- EINSTEIN FIELD EQUATIONS; ENERGY-MOMENTUM TENSOR; GENERAL RELATIVITY THEORY; GRAVITATIONAL COLLAPSE; HEAT TRANSFER; METRICS; NEUTRON STARS; STARS; SUPERNOVAE; THERMAL CONDUCTION
- Descriptors DEC
- BINARY STARS; ENERGY TRANSFER; EQUATIONS; ERUPTIVE VARIABLE STARS; FIELD EQUATIONS; FIELD THEORIES; TENSORS; VARIABLE STARS