Abstract
The description of a point mass in general relativity (GR) is given in the framework of the field formulation of GR, where all the dynamical fields, including the gravitational field, are considered in a fixed background spacetime. With the use of stationary (not static) coordinates, non-singular at the horizon, the Schwarzschild solution is presented as a point-like field configuration in a whole background Minkowski space. The requirement of a stable η-causality stated recently by J. B. Pitts and W. C. Schieve (Found. Phys. 34, 211 (2004)) is used essentially as a criterion for testing configurations.
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References
1. S. W. Hawking, Plenary Lecture at GR17, Dublin, July 2004.
2. L. D. Landau and E. M. Lifshitz, The Classical Theory of Fields (Pergamon, Oxford, 1975).
3. J. V. Narlikar, “Some conceptual problems in general relativity and cosmology,” in A Random Walk in Relativity and Cosmology, N. Dadhich, J. Krishna Rao, J. V. Narlikar, and C. V. Vishevara, eds. (Wiley Eastern, New Delhi, 1985) pp. 171–183.
4. A. N. Petrov and J. V. Narlikar, Found. Phys. 26, 1201 (1996); Erratum; Found. Phys. 28, 1023 (1998).
5. L. P. Grishchuk, A. N. Petrov, and A. D. Popova, Commun. Math. Phys. 94 379 (1984).
6. A. D. Popova and A. N. Petrov, Int. J. Mod. Phys. A 3, 2651 (1988).
7. A. N. Petrov, Class. Quantum Grav. 10, 2663 (1993).
8. S. Deser, Gen. Relat. Grav. 1, 9 (1970); arXiv: gr-qc/0411023.
9. R. H. Kraichnan, Phys. Rev. D 98, 1118 (1955).
10. C. W. Misner, K. S. Thorne, and J. A. Wheeler, Gravitation (Freeman, San Francisco, 1973).
11. J. B. Pitts and W. C. Schieve, Found. Phys. 34, 211 (2004).
12. L. P. Grishchuk, Usp. Fiz. Nauk 160, 147 (1990); Sov. Phys. Usp. 33, 669 (1990).
13. A. N. Petrov, Vestnik Moskov. Univer. Ser. 3. Fiz. Astron. 31 (5), 88 (1990).
14. A. N. Petrov, Astronom. Astrophys. Trans. 1, 195 (1992).
15. A. A. Vlasov, Soviet J. Nucl. Phys. 51, 1148 (1990).
16. Y. M. Loskutov, Soviet J. Nucl. Phys. 54, 903 (1991).
17. T. Damour, P. Jaranowski, and G. Schäfer, Phys. Lett. B 513, 147 (2001).
18. L. Blanchet, T. Damour, and G. Esposito-Farése, Phys. Rev. D 69, 124007 (2004).
19. G. Schaefer, “Binary black holes and gravitational wave production: Post-Newtonian analytic treatment,” in Current Trends in Relativistic Astrophysics, L. Fernendez-Jambrina, and L. M. Gonzolez-Romero, eds. (Lecture Notes in Physics, Vol. 617) (Springer, New York, 2003), p. 195.
20. J. Hartle, K. S. Thorne, and R. H. Price, Chap. V in: Black Holes: The Membrane Paradigm, K. S. Thorne, R. H. Price, and D. A. Macdonald, eds. (Yale University Press, New Haven, 1986).
21. A. J. S. Hamilton and J. P. Lisle, “The river model of black holes,” arXiv:gr-qc/0411060.
22. I. M. Gelfand and G. E. Shilov, Generalized functions. Vol. 1. Properties and Operations (Academic, New York, 1964).
23. S. M. Kopeikin, Astronom. Zh. 62, 889 (1985); Soviet Astron. 29, 516 (1985).
24. G. A. Korn and T. A. Korn, Mathematical Handbook for Scientists and Engineers (McGraw-Hill, New York, 1968).
25. A. N. Petrov, Int. J. Mod. Phys. D 4, 451 (1995).
26. R. Penrose, Proc. R. Soc. Lond. A 381, 53 (1982).
27. K. T. Tod, Proc. R. Soc. Lond. A 388, 457 (1983).
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Petrov, A. The Schwarzschild Black Hole as a Point Particle. Found Phys Lett 18, 477–489 (2005). https://doi.org/10.1007/s10702-005-7538-2
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DOI: https://doi.org/10.1007/s10702-005-7538-2