Plane symmetric gravitational fields in (D+1)-dimensional general relativity

We consider plane symmetric gravitational fields within the framework of General Relativity in (D+1)-dimensional spacetime. Two classes of vacuum solutions correspond to higher-dimensional generalizations of the Rindler and Taub spacetimes. The general solutions are presented for a positive and negative cosmological constant as the only source of the gravity. Matching conditions on a planar boundary between two regions with distinct plane symmetric metric tensors are discussed. An example is considered with Rindler and Taub geometries in neighboring half-spaces. As another example, we discuss a finite thickness cosmological constant slab embedded into the Minkowski, Rindler and Taub spacetimes. The corresponding surface energy-momentum tensor is found required for matching the exterior and interior geometries.

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Publication Details

Journal
Astrophysics
Published
2024-09-26
DOI
https://doi.org/10.54503/0571-7132-2024.67.3-409
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
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article

Plane symmetric gravitational fields in (D+1)-dimensional general relativity

R. M. Avagyan, G. H. Harutyunyan, A. A. Saharian, T. A. Petrosyan
Astrophysics
Cosmology and Gravitation Theories
article

Plane symmetric gravitational fields in (D+1)-dimensional general relativity

R. M. Avagyan, G. H. Harutyunyan, A. A. Saharian, T. A. Petrosyan
article en

Abstract

We consider plane symmetric gravitational fields within the framework of General Relativity in (D+1)-dimensional spacetime. Two classes of vacuum solutions correspond to higher-dimensional generalizations of the Rindler and Taub spacetimes. The general solutions are presented for a positive and negative cosmological constant as the only source of the gravity. Matching conditions on a planar boundary between two regions with distinct plane symmetric metric tensors are discussed. An example is considered with Rindler and Taub geometries in neighboring half-spaces. As another example, we discuss a finite thickness cosmological constant slab embedded into the Minkowski, Rindler and Taub spacetimes. The corresponding surface energy-momentum tensor is found required for matching the exterior and interior geometries.

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