Stability of superdense stars in the bimetric theory of gravitation |
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| Authors: | V. Bálek E. V. Chubarian |
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| Affiliation: | (1) Dept of Theoretical Physics, Yerevan State University, Armenian, SSR;(2) Present address: Dept. of Theoretical Physics, Comenius University, Czechoslovakia |
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| Abstract: | Calculations of superdense star models in the Rosen bimetric theory of gravitation are presented. There is a family of  quark stars whose members are probably stable even if their masses do not exceed the maximum mass of neutron stars. |
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