On the spectrum of the radiation from a naked singularity

Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

Volumn 442, Issue 1-4, 1998, Pages 90-96

  Vaz, Cenalo ^a   Witten, Louis ^b  

^a UNIVERSITY OF ALGARVE   (Portugal)

^b UNIVERSITY OF CINCINNATI   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0345919006     PISSN: 03702693     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0370-2693(98)01221-0     Document Type: Article

References (21)

1. R. Penrose, Riv. Nuovo Cimento 1 (1969) 252; in: S.W. Hawking, W. Israel (Eds.), General Relativity, An Einstein Centenary Survey, Cambridge Univ. Press, Cambridge, London, 1979, p. 581. In its original form, the Cosmic Censorship Hypothesis (CCH) essentially states that no physically realistic collapse, evolving from a well posed initial data set and satisfying the dominant energy condition, results in a singularity in the causal past of null infinity. There is also a strong version of the CCH which states that no physically realistic collapse leads to a locally timelike singularity.
2. R. Penrose, Riv. Nuovo Cimento 1 (1969) 252; in: S.W. Hawking, W. Israel (Eds.), General Relativity, An Einstein Centenary Survey, Cambridge Univ. Press, Cambridge, London, 1979, p. 581. In its original form, the Cosmic Censorship Hypothesis (CCH) essentially states that no physically realistic collapse, evolving from a well posed initial data set and satisfying the dominant energy condition, results in a singularity in the causal past of null infinity. There is also a strong version of the CCH which states that no physically realistic collapse leads to a locally timelike singularity.
3. P.S. Joshi, Global Aspects in Gravitation and Cosmology, Clarendon Press, Oxford, 1993.
4. C. Vaz, L. Witten, Phys. Lett. B 325 (1994) 27; Class. Quant. Grav. 12 (1995) 1; 13 (1996) L59; Nucl. Phys. B 487 (1997) 409.
5. C. Vaz, L. Witten, Phys. Lett. B 325 (1994) 27; Class. Quant. Grav. 12 (1995) 1; 13 (1996) L59; Nucl. Phys. B 487 (1997) 409.
6. C. Vaz, L. Witten, Phys. Lett. B 325 (1994) 27; Class. Quant. Grav. 12 (1995) 1; 13 (1996) L59; Nucl. Phys. B 487 (1997) 409.
7. C. Vaz, L. Witten, Phys. Lett. B 325 (1994) 27; Class. Quant. Grav. 12 (1995) 1; 13 (1996) L59; Nucl. Phys. B 487 (1997) 409.
8. S. Barve, T.P. Singh, C. Vaz, L. Witten, Particle Creation in the Marginally Bound Self-Similar Collapse of Dust, grqc/9802035, Nucl. Phys. B, in press.
9. S. Barve, T.P. Singh, C. Vaz, L. Witten, The Quantum Stress Tensor in Self-Similar Spherical Dust Collapse, gr-qc/9805095, Phys. Rev. D, in press.
10. W.A. Hiscock, L.G. Williams, D.M. Eardley, Phys. Rev. D 26 (1982) 751.
11. L.H. Ford, L. Parker, Phys. Rev. D 17 (1978) 1485.
12. R.C. Tolman, Proc. Nat. Acad. Sci. USA 20 (1934) 169; H. Bondi, Mon. Not. Astron. Soc. 107 (1947) 410.
13. R.C. Tolman, Proc. Nat. Acad. Sci. USA 20 (1934) 169; H. Bondi, Mon. Not. Astron. Soc. 107 (1947) 410.
14. See, for example, N.D. Birrel, P.C.W. Davies, Quantum Fields in Curved Space, Cambridge Monographs in Math. Phys., Cambridge University Press, London, 1982.
15. C. Callan, S.B. Giddings, J. Harvey, A. Strominger, Phys. Rev. D 45 (1992) 1005; S. de Alwis, Phys. Lett. B 289 (1992) 282; A. Bilal, C. Callan, Nucl. Phys. B 394 (1993) 73; Sukanta Bose, L. Parker, Y. Peleg, Phys. Rev. D 52 (1995) 3512; D 53 (1996) 5708, 7089; Phys. Rev. Lett. 76 (1996) 861; A. Fabri, J.G. Russo, Phys. Rev. D 53 (1996) 6995.
16. C. Callan, S.B. Giddings, J. Harvey, A. Strominger, Phys. Rev. D 45 (1992) 1005; S. de Alwis, Phys. Lett. B 289 (1992) 282; A. Bilal, C. Callan, Nucl. Phys. B 394 (1993) 73; Sukanta Bose, L. Parker, Y. Peleg, Phys. Rev. D 52 (1995) 3512; D 53 (1996) 5708, 7089; Phys. Rev. Lett. 76 (1996) 861; A. Fabri, J.G. Russo, Phys. Rev. D 53 (1996) 6995.
17. C. Callan, S.B. Giddings, J. Harvey, A. Strominger, Phys. Rev. D 45 (1992) 1005; S. de Alwis, Phys. Lett. B 289 (1992) 282; A. Bilal, C. Callan, Nucl. Phys. B 394 (1993) 73; Sukanta Bose, L. Parker, Y. Peleg, Phys. Rev. D 52 (1995) 3512; D 53 (1996) 5708, 7089; Phys. Rev. Lett. 76 (1996) 861; A. Fabri, J.G. Russo, Phys. Rev. D 53 (1996) 6995.
18. C. Callan, S.B. Giddings, J. Harvey, A. Strominger, Phys. Rev. D 45 (1992) 1005; S. de Alwis, Phys. Lett. B 289 (1992) 282; A. Bilal, C. Callan, Nucl. Phys. B 394 (1993) 73; Sukanta Bose, L. Parker, Y. Peleg, Phys. Rev. D 52 (1995) 3512; D 53 (1996) 5708, 7089; Phys. Rev. Lett. 76 (1996) 861; A. Fabri, J.G. Russo, Phys. Rev. D 53 (1996) 6995.
19. C. Callan, S.B. Giddings, J. Harvey, A. Strominger, Phys. Rev. D 45 (1992) 1005; S. de Alwis, Phys. Lett. B 289 (1992) 282; A. Bilal, C. Callan, Nucl. Phys. B 394 (1993) 73; Sukanta Bose, L. Parker, Y. Peleg, Phys. Rev. D 52 (1995) 3512; D 53 (1996) 5708, 7089; Phys. Rev. Lett. 76 (1996) 861; A. Fabri, J.G. Russo, Phys. Rev. D 53 (1996) 6995.
20. C. Callan, S.B. Giddings, J. Harvey, A. Strominger, Phys. Rev. D 45 (1992) 1005; S. de Alwis, Phys. Lett. B 289 (1992) 282; A. Bilal, C. Callan, Nucl. Phys. B 394 (1993) 73; Sukanta Bose, L. Parker, Y. Peleg, Phys. Rev. D 52 (1995) 3512; D 53 (1996) 5708, 7089; Phys. Rev. Lett. 76 (1996) 861; A. Fabri, J.G. Russo, Phys. Rev. D 53 (1996) 6995.
21. C. Callan, S.B. Giddings, J. Harvey, A. Strominger, Phys. Rev. D 45 (1992) 1005; S. de Alwis, Phys. Lett. B 289 (1992) 282; A. Bilal, C. Callan, Nucl. Phys. B 394 (1993) 73; Sukanta Bose, L. Parker, Y. Peleg, Phys. Rev. D 52 (1995) 3512; D 53 (1996) 5708, 7089; Phys. Rev. Lett. 76 (1996) 861; A. Fabri, J.G. Russo, Phys. Rev. D 53 (1996) 6995.