Published August 25, 1975
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Numerical study of rotating relativistic stars
Description
The equations of structure for rotating stars in general relativity are presented and put in a form suitable for computer calculations. The results of equilibrium calculations for supermassive stars, neutron stars, and magnetically supported stars are reported, as are calculations of collapsing, rotating, and magnetized stars in the slowly changing gravitational field approximation. (auth)
Availability note (English)
MF available from INIS under the Report Number.Files
7232029.pdf
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Additional details
Publishing Information
- Imprint Pagination
- 54 p.
- Report number
- UCRL--76967
Conference
- Title
- Meeting of physics and astrophysics of neutron stars and black holes.
- Dates
- 14 Jul 1975.
- Place
- Varenna, Italy.
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 7232029
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- BLACK HOLES; EQUATIONS; EQUILIBRIUM; GENERAL RELATIVITY THEORY; GRAVITATIONAL COLLAPSE; GRAVITATIONAL FIELDS; MAGNETIC STARS; MATHEMATICAL MODELS; NEUTRON STARS; RELATIVISTIC RANGE; ROTATION; STARS
- Descriptors DEC
- ENERGY RANGE; FIELD THEORIES
Optional Information
- Secondary number(s)
- CONF-750744--1.