The exact linear retarded spherically symmetrical solutions to the Einstein equations linearized around the Friedmann background are derived and examined for an ultrarelativistic equation of state. The uniqueness of the solutions in class C1 is proved.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Yu. G. Ignat'ev and N. Elmakhi, Russ. Phys. J., No. 1, 74 (2008).
Yu. G. Ignat'ev and A. A. Popov, The Problems of Gravitation Theory, Relativistic Kinetics, and Evolution of the Universe [in Russian], Izd. KSPI, Kazan', 1988.
Yu. G. Ignat'ev and A. A. Popov, Russ. Phys. J., No. 5, 391 (1989).
Yu. G. Ignat'ev and A. A. Popov, Astrophys. Space Sci., 163, 153 (1990).
Yu. G. Ignat'ev and A. A. Popov, Phys. Lett. A, 220, 22 (1996).
Author information
Authors and Affiliations
Corresponding author
Additional information
Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 7, pp. 69–76, July, 2008.
Rights and permissions
About this article
Cite this article
Ignat’ev, Y.G., Elmakhi, N. A dynamic model of spherical perturbations in the Friedmann Universe. II. Retarded solutions to an ultrarelativistic equation of state. Russ Phys J 51, 735–745 (2008). https://doi.org/10.1007/s11182-008-9103-5
Received:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s11182-008-9103-5