Published April 15, 1987
| Version v1
Journal article
Gravitational radiation from realistic relativistic stars: Odd-parity fluid perturbations
Creators
- 1. Department of Astronomy, Yale University, New Haven, Connecticut 06511
Description
Odd-parity gravitational perturbations of a spherically symmetric background are studied in the linearized Einstein theory. A variety of collapse models, based on a May-White hydrodynamic code, are investigated, simulating dust collapse and stellar core collapse typical of type-II supernova models. Numerical results are presented, showing that in this linearized problem a typical core collapse may radiate up to 10/sup -7/ Mc2 in gravitational-wave energy
Additional details
Publishing Information
- Journal Title
- Phys. Rev., D
- Journal Volume
- 35
- Journal Issue
- 8
- Series
- Phys. Rev., D.
- Journal Page Range
- 2287-2296
- ISSN
- 0556-2821
- CODEN
- PRVDA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 19024329
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- DISTURBANCES; EINSTEIN FIELD EQUATIONS; ENTROPY; GAUGE INVARIANCE; GRAVITATIONAL COLLAPSE; GRAVITATIONAL RADIATION; HYDRODYNAMIC MODEL; NUMERICAL SOLUTION; PARITY; PERTURBATION THEORY; RELATIVITY THEORY; SCHWARZSCHILD METRIC; STARS; SUPERNOVAE
- Descriptors DEC
- BINARY STARS; EQUATIONS; ERUPTIVE VARIABLE STARS; FIELD EQUATIONS; FIELD THEORIES; INVARIANCE PRINCIPLES; MATHEMATICAL MODELS; METRICS; PARTICLE MODELS; PARTICLE PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS; STATISTICAL MODELS; THERMODYNAMIC MODEL; THERMODYNAMIC PROPERTIES; VARIABLE STARS