Gravitational waves in vacuum spacetimes with cosmological constant. I. Classification and geometrical properties of nontwisting type N solutions

Article

Gravitational waves in vacuum spacetimes with cosmological constant. I. Classification and geometrical properties of nontwisting type N solutions

Bičák, J; Podolský, J.

J. Math. Phys. 40(0), 4495-4505 (1999)

Abstract

All nontwisting Petrov-type N solutions of vacuum Einstein field equations with cosmological constant Lambda are summarized. They are shown to belong either to the nonexpanding Kundt class or to the expanding Robinson-Trautman class. Invariant subclasses of each class are defined and the corresponding metrics are given explicitly in suitable canonical coordinates. Relations between the subclasses and their geometrical properties are analyzed. In the subsequent paper these solutions are interpreted as exact gravitational waves propagating in de Sitter or anti-de Sitter spacetimes.

Keywords

gravitational waves, Einstein field equations, space-time configurations, differential geometry, cosmology

Institute authors

Supported by

GACR 202/99/0261 — Relativistic physics and astrophysics

BibTeX

@article{UTF150,
  author        = {Bičák, J and Podolský, J.},
  title         = {{Gravitational waves in vacuum spacetimes with cosmological constant. I. Classification and geometrical properties of nontwisting type N solutions}},
  journal       = {J. Math. Phys.},
  volume        = {40},
  number        = {0},
  pages         = {4495-4505},
  year          = {1999},
  doi           = {10.1063/1.532981},
  eprint        = {gr-qc/9907048},
  archivePrefix = {arXiv},
  url           = {http://jmp.aip.org/resource/1/jmapaq/v40/i9/p4495\_s1},
}