Geodesic
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.

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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. 
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E. V. Chubaryan; D. I. Zaslavsky. 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. http://geodesic.mathdoc.fr/item/UZERU_1988_2_a6/

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[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

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[4] A. V. Sarkisyan, B. V. Khachatryan, E. V. Chubaryan, “Konfiguratsii vyrozhdennykh mass po bimetricheskoi teorii gravitatsii Rozena”, Astrofizika, 23 (1985), 506–511