Cosmic no-hair conjecture and black-hole formation: An exact model with gravitational radiation

Article

Cosmic no-hair conjecture and black-hole formation: An exact model with gravitational radiation

Bičák, J.; Podolský, J.

Phys. Rev. D 52(0), 887-895 (1995)

Abstract

Robinson-Trautman radiative space-times with a positive cosmological constant are studied by analytical methods. They are shown to approach the Schwarzschild–de Sitter solution at large retarded times. Their global structure is analyzed, and it is demonstrated that they represent explicit models exhibiting the cosmic no-hair conjecture and black-hole formation under the presence of gravitational waves.

Institute authors

Supported by

GACR 202/93/0503 — Relativistic physics and astrophysics
GAUK 318/1993 — Relativistická teorie gravitace

BibTeX

@article{UTF276,
  author        = {Bičák, J. and Podolský, J.},
  title         = {{Cosmic no-hair conjecture and black-hole formation: An exact model with gravitational radiation}},
  journal       = {Phys. Rev. D},
  volume        = {52},
  number        = {0},
  pages         = {887-895},
  year          = {1995},
  doi           = {10.1103/PhysRevD.52.887},
  eprint        = {ads: 1995PhRvD..52..887B},
  archivePrefix = {arXiv},
  url           = {http://link.aps.org/abstract/PRD/v52/p887},
}