Abstract
It is shown that, similarly to general relativity, the bimetric theory of gravitation predicts the formation of primordial minicompact objects. Contrary to general relativity, however, it predicts that such objects are stable. Observational consequences are discussed.
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References
Hawking, S. W. (1971).mon. Not. R. Astron. Soc.,152, 75.
Hawking, S. W. (1974).Nature,248, 30.
Rosen, N. (1973).Gen. Rel Grav.,4, 435; (1914).Ann. Phys. (N. Y.),84, 455.
Rosen, J., and Rosen, N. (1977).Astrophys. J.,212, 605.
Hawking, S. W. (1975).Commun. Math. Phys.,43, 199.
Lindhard, J., and Scharf, M. (1961).Phys. Rev. 124, 128.
Hillas, A. M. (1915).Phys. Rep.,20C, 61.
Jacobs, K. C., and Seitzer, P. O. (1977).Gen. Rel. Grav.,8, 7.
Price, P. B., Shirk, E. K., Osborne, W. Z., and Pinsky, L. S. (1978).Phys. Rev. D,18, 1382.
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In partial fulfillment of the requirements for the D.Sc. degree.
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Falik, D., Opher, R. Minicompact objects according to the bimetric theory of gravitation. Gen Relat Gravit 10, 227–230 (1979). https://doi.org/10.1007/BF00759857
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DOI: https://doi.org/10.1007/BF00759857