Abstract
It is shown that from the point of view of a distant observer the gravitational field of a moving Schwarzschild black hole is the same as produced by an extended, non-rotating, spherical body of the same mass. According to him, a black hole follows the Newtonian equations of motion, though some quantities, for example the distance, lose their Newtonian meaning.
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References
Giacconi, R.Proceedings of the I.A.U. Symposium No. 64, (to be published).
Einstein, A., Infeld, L. and Huffman, B. (1938).Ann. Math.,39, 65.
Einstein, A. and Infeld, L. (1940).Ann. Math.,41, 455.
Einstein, A. and Infeld, L. (1949).Can. J. Phys.,1, 209.
Fock, V. (1964).The Theory of Space, Time and Gravitation, (Pergamon Press, Oxford).
Infeldj L. and Plebanski, J. (1960).Motion and Relativity, (P.W.N., Warsaw).
Plebanski, J. and Bazanski, S. (1959).Acta Phys. Polon.,18, 307.
Kerr, R.P. (1960).Nuovo Cim.,16, 26.
Trautman, A. (1958).Lectures on General Relativity, (Kings College, London).
Regge, T. and Wheeler, J.A. (1957).Phys. Rev.,108, 1063.
Zerilli, F.J. (Ph.D. Thesis), (Princeton University), (unpublished).
Patashinskii, A.Z. and Kharkov, A.A. (1970).Zh. Eksper. Teor. Fiz.,59, 574.
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Demiański, M., Grishchuk, L.P. Note on the motion of black holes. Gen Relat Gravit 5, 673–679 (1974). https://doi.org/10.1007/BF00761925
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DOI: https://doi.org/10.1007/BF00761925