Abstract
The recently proposed criteria for naked blackholes are conveniently rephrased. It is shown that twosolutions of dilaton-Maxwell gravity, satisfying weakenergy conditions, represent naked blackholes.
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REFERENCES
Horowitz, G. T., and Ross, S. F. (1997). Phys. Rev. D 56, 2180; (1998). Phys. Rev. D 57, 1098.
Kar, S. (1997). Phys. Rev. D 55, 4872.
Visser, M. (1995). Lorentzian Wormholes-From Einstein to Hawking (A.I.P. New York).
Morris, M. S., and Thorne, K. S. (1988). Amer. J. Phys. 56, 395.
Chan, K. C. K., Mann, R. B., and Horne, J. (1995). Nucl. Phys. B 447, 441.
Nandi, K. K., Islam, A., and Evans, J. (1997). Phys. Rev. D 55, 2497.
Nandi, K. K., Bhattacharjee, B., Alam, S. M. K., and Evans, J. (1998). Phys. Rev. D 57, 823.
Nandi, K. K. (1999). Phys. Rev. D 59, to appear.
Magnano, G., and Sokolowski, L. M. (1994). Phys. Rev. D 50, 5039.
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Nandi, K.K., Alam, S.M.K. On Naked Black Holes. General Relativity and Gravitation 31, 1263–1270 (1999). https://doi.org/10.1023/A:1026772707627
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DOI: https://doi.org/10.1023/A:1026772707627