Hostname: page-component-cb9f654ff-qc88w Total loading time: 0 Render date: 2025-08-15T19:58:57.624Z Has data issue: false hasContentIssue false
  • English
  • Français

Gravitational radiation in homogeneous cosmological models with space-sections of constant negative curvature

Published online by Cambridge University Press:  24 October 2008

J. Krishna Rao  and
P. C. Vaidya
J. Krishna Rao
Affiliation:
Department of Mathematics, Gujarat University, Ahmedabad 9, India
P. C. Vaidya
Affiliation:
Department of Mathematics, Gujarat University, Ahmedabad 9, India
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The propagation of type N gravitational radiation in homogeneous cosmological models with space-sections of constant negative curvature is considered. It is found that the propagation of radiation distorts the isotropy of the fluid pressure in the models permanently.

Information

Type
Research Article
Information
Mathematical Proceedings of the Cambridge Philosophical Society , Volume 61 , Issue 3 , July 1965 , pp. 763 - 765
Copyright
Copyright © Cambridge Philosophical Society 1965

References

(1)Einstein, A. and Rosen, N.J. Franklin Inst. 223 (1937), 43.CrossRefGoogle Scholar
(2)Infeld, L. and Schild, A.Phys. Rev. 68 (1945), 250.CrossRefGoogle Scholar
(3)Krishna Rao, J. and Vaidya, P. C. To be published in Indian J. Phys.Google Scholar
(4)Krishna Rao, J.Curr. Sci. 32 (1963), 350.Google Scholar
(5)Lichnerowicz, A.Ann. Mat. Pura. Appl. (iv) 50 (1960), 450.CrossRefGoogle Scholar
(6)Lichnerowicz, A.Théories rélativistes de la gravitation et l' électromagnétisme (Masson, 1955), p. 14.Google Scholar
(7)O'brien, S. and Synge, J. L.Comm. Dublin Inst. Adv. Studies Ser. A 9 (1952), 1.Google Scholar
(8)Petrov, A. Z.Sci. Not. Kazan State Univ. 114 (1954), 55.Google Scholar
(9)Pirani, F. A. E.Recent developments in general relativity (Pergamon, 1962), p. 103.Google Scholar