Electromagnetic Fields in a Homogeneous, Nonisotropic Universe

Electromagnetic Fields in a Homogeneous, Nonisotropic Universe

A solution of the Einstein-Maxwell equations is derived that represents a closed universe of topology S/sup 3 / x R, filled with gravitational and electromagnetic radiation. The lowest of the large number of possible modes of radiation in such a universe is considered. This mode has maximum symmetry...

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Veröffentlicht in:Physical Review (U.S.) Superseded in part by Phys. Rev. A, Phys. Rev. B: Solid State, Phys. Rev. C, and Phys. Rev. D Phys. Rev. B: Solid State, Phys. Rev. C, and Phys. Rev. D, 1964-01, Vol.133 (3B), p.B845-B848
1. Verfasser: Brill, Dieter R.
Format: Artikel
Sprache:eng
Schlagworte:
ANISOTROPY
ASTROPHYSICS
DIFFERENTIAL EQUATIONS
ELECTROMAGNETIC FIELDS
GRAVITATION
PHYSICS
RADIATIONS
SPACE
VECTORS
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container_issue 3B
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container_title Physical Review (U.S.) Superseded in part by Phys. Rev. A, Phys. Rev. B: Solid State, Phys. Rev. C, and Phys. Rev. D
container_volume 133
creator Brill, Dieter R.
description A solution of the Einstein-Maxwell equations is derived that represents a closed universe of topology S/sup 3 / x R, filled with gravitational and electromagnetic radiation. The lowest of the large number of possible modes of radiation in such a universe is considered. This mode has maximum symmetry consistent with the existence of a vector field; the universe is homogeneous but not isotropic, and is therefore a generalization of one of the solutions discussed by Taub. It is possible to solve explicitly for the metric coefficients. Some of the physical properties of the solution are discussed. (auth)
doi_str_mv 10.1103/PhysRev.133.B845
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D</title><description>A solution of the Einstein-Maxwell equations is derived that represents a closed universe of topology S/sup 3 / x R, filled with gravitational and electromagnetic radiation. The lowest of the large number of possible modes of radiation in such a universe is considered. This mode has maximum symmetry consistent with the existence of a vector field; the universe is homogeneous but not isotropic, and is therefore a generalization of one of the solutions discussed by Taub. It is possible to solve explicitly for the metric coefficients. Some of the physical properties of the solution are discussed. 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source American Physical Society Journals
subjects ANISOTROPY
ASTROPHYSICS
DIFFERENTIAL EQUATIONS
ELECTROMAGNETIC FIELDS
GRAVITATION
PHYSICS
RADIATIONS
SPACE
VECTORS
title Electromagnetic Fields in a Homogeneous, Nonisotropic Universe
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