Strong gravitational waves in semiclosed electromagnetic universes. Statement and analysis of the problem in terms of the method of spin coefficients
Journal Article
·
· Sov. Phys. J. (Engl. Transl.); (United States)
OSTI ID:5962076
The problem of integration is discussed for a complete system of Newman-Penrose equations for electrovacuum spaces of the general theory of relativity with nonzero cosmological constant. In terms of the method of spin coefficients, we formulate conditions on the electormagnetic and gravitational field variables, which distinguish a special class of Riemann spaces corresponding to strong gravitational waves in semiclosed Universes of Bertotti-Robinson type.
- OSTI ID:
- 5962076
- Journal Information:
- Sov. Phys. J. (Engl. Transl.); (United States), Journal Name: Sov. Phys. J. (Engl. Transl.); (United States) Vol. 30:11; ISSN SOPJA
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
640106* -- Astrophysics & Cosmology-- Cosmology
657003 -- Theoretical & Mathematical Physics-- Relativity & Gravitation
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ANGULAR MOMENTUM
COSMOLOGICAL MODELS
EINSTEIN-MAXWELL EQUATIONS
ELECTROMAGNETIC FIELDS
EQUATIONS
FIELD EQUATIONS
FIELD THEORIES
GENERAL RELATIVITY THEORY
GEODESICS
GRAVITATIONAL FIELDS
GRAVITATIONAL WAVES
MATHEMATICAL MODELS
MATHEMATICAL SPACE
PARTICLE PROPERTIES
RIEMANN SPACE
SPACE
SPACE-TIME
SPIN
TRANSFORMATIONS
UNIVERSE
657003 -- Theoretical & Mathematical Physics-- Relativity & Gravitation
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ANGULAR MOMENTUM
COSMOLOGICAL MODELS
EINSTEIN-MAXWELL EQUATIONS
ELECTROMAGNETIC FIELDS
EQUATIONS
FIELD EQUATIONS
FIELD THEORIES
GENERAL RELATIVITY THEORY
GEODESICS
GRAVITATIONAL FIELDS
GRAVITATIONAL WAVES
MATHEMATICAL MODELS
MATHEMATICAL SPACE
PARTICLE PROPERTIES
RIEMANN SPACE
SPACE
SPACE-TIME
SPIN
TRANSFORMATIONS
UNIVERSE