Analytical solutions for superdense stars in the Bimetric Theory of Gravitation
Proceedings of the Yerevan State University. Physical and mathematical sciences, no. 2 (1988), pp. 42-48
Citer cet article
Voir la notice de l'article provenant de la source Math-Net.Ru
Analytical solutions for spheric-symmetrical case, inside mass distribution in the Bimetric Theory of Gravitation are obtained by the method of inversion problem. These solutions correspond to physical reality. Models of super dense star configurations are obtained.
[1] N. Rosen, “Bimetric theory and singularities in relativity”, Ann. Phys., 84 (1974), 455–473 | DOI | MR
[2] G. S. Saakyan, A. V. Sarkisyan, B. V. Khachatryan, E. V. Chubaryan, “Konfiguratsii vyrozhdennykh mass po bimetricheskoi teorii gravitatsii”, Astrofizika, 14 (1978), 489–500
[3] O. A. Grigoryan, E. V. Chubaryan, “Statsionarnye aksialno-simmetrichnye gravitatsionnye polya v bimetricheskoi teorii”, Astrofizika, 23 (1985), 177–190 | MR
[4] A. V. Sarkisyan, B. V. Khachatryan, E. V. Chubaryan, “Konfiguratsii vyrozhdennykh mass po bimetricheskoi teorii gravitatsii Rozena”, Astrofizika, 23 (1985), 506–511