A bi-metric theory of gravitation
A bi-metric theory of gravitation is proposed, satisfying the covariance and equivalence principles. It is based on a simple form of Lagrangian and has a simpler mathematical structure than that of the general theory of relativity. The theory agrees with general relativity up to the accuracy of the observations made up to now. The static spherically symmetric solution of the present field equations does not involve any 'black hole'.
KeywordsBlack Hole Covariance General Relativity General Theory Simple Form
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- 1.Rosen, N. (1940).Phys. Rev.,57, 147, 150.Google Scholar
- 2.Papapetrou, A. (1948).Proc. Roy. Irish Acad.,A52, 11.Google Scholar
- 3.Rosen, N. (1963).Ann. Phys.,22, 1.Google Scholar
- 4.Rosen, N. (1966).Perspectives in Geometry and Relativity, (Indiana University Press, Bloomington, Indiana), p. 325.Google Scholar
- 5.de Donder, T. (1921).La Gravifique Einsteinienne, (Paris).Google Scholar
- 6.Yilmaz, H. (1958).Phys. Rev.,111, 1417. The considerations there are quite different from those of the present paper.Google Scholar
- 7.Weber, J. (1961).General Relativity and Gravitational Waves, (Interscience Publishers, New York).Google Scholar
- 8.Clapp, R. E. (1973).Phys. Rev.,D7, 345.Google Scholar