Black hole evaporation and compact extra dimensions

Physical Review D

Volumn 64, Issue 2, 2001, Pages

  Casadio, Roberto ^a   Harms, Benjamin ^b  

^a UNIVERSITY OF BOLOGNA   (Italy)

^b UNIVERSITY OF ALABAMA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; COSMOS; ENERGY; EVAPORATION; GRAVITY; LUMINANCE; THEORY;

EID: 85037898705     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.64.024016     Document Type: Article

References (39)

1. N. Arkani-Hamed, S. Dimopoulos, and G. Dvali, Phys. Lett. B 429, 263 (1998);
2. Phys. Rev. D 59, 086004 (1999);
3. I. Antoniadis, N. Arkani-Hamed, S. Dimopoulos, and G. Dvali, Phys. Lett. B 436, 257 (1998).
4. L. Randall and R. Sundrum, Phys. Rev. Lett. 83, 4690 (1999).
5. B. Harms and Y. Leblanc, Phys. Rev. D 46, 2334 (1992); 47, 2438 (1993); Ann. Phys. (N.Y.) 244, 262 (1995); 244, 272 (1995); Europhys. Lett. 27, 557 (1994); Ann. Phys. (N.Y.) 242, 265 (1995);
6. P.H. Cox, B. Harms, and Y. Leblanc, Europhys. Leu. 26, 321 (1994).
7. R. Casadio, B. Harms, and Y. Leblanc, Phys. Rev. D 57, 1309 (1998);
8. R. Casadio and B. Harms, ibid. 58, 044014 (1998);
9. -Mod. Phys. Lett. A 17, 1089 (1999);
10. J.M. Bardeen, B. Carter, and S.W. Hawking, Commun. Math. Phys. 31, 161 (1973);
11. G.W. Gibbons and S.W. Hawking, Phys. Rev. D 15, 2752 (1977).
12. J. Polchinski, "TASI Lectures on D-branes," hep-th/9611050.
13. A. Strominger and C. Vafa, Phys. Lett. B 379, 99 (1996).
14. J. Maldacena, Nucl. Phys. B (Proc. Suppl.) 61A, 111 (1998).
15. J.D. Bekenstein, Phys. Rev. D 7, 2333 (1973); 9, 3292 (1974).
16. P.C. Argyres, S. Dimopoulos, and J. March-Russell, Phys. Lett. B 441, 96 (1998).
17. A. Chamblin, S. Hawking, and H.S. Reall, Phys. Rev. D 61, 065007 (2000).
18. R. Emparan, G.T. Horowitz, and R.C. Myers, Phys. Rev. Lett. 85, 499 (2000).
19. R. Casadio and B. Harms, Phys. Lett. B 487, 209 (2000).
20. J.C. Long, H.W. Chan, and J.C. Price, Nucl. Phys. B539, 23 (1999).
21. S. Cullen and M. Perelstein, Phys. Rev. Lett. 83, 268 (1999);
22. V. Barger, T. Han, C. Kao, and R.J. Zhang, Phys. Lett. B 461, 34 (1999);
23. M. Fairbairn, "Cosmological constraints on large extra dimensions," hep-ph/0101131.
24. G.T. Horowitz and A. Strominger, Nucl. Phys. 15360, 197 (1991).
25. R. Gregory and R. Laflamme, Phys. Rev. Lett. 70, 2837 (1993);
26. G. T. Horowitz and K. Maeda, "Fate of Black String Instability," hep-th/0105111.
27. R.C. Myers and M.J. Perry, Ann. Phys. (N.Y.) 172, 304 (1986).
28. S.W. Hawking, Nature (London) 248, 30 (1974); Commun. Math. Phys. 43, 199 (1975).
29. D. Page, Phys. Rev. D 13, 198 (1976); 16, 2402 (1977).
30. S.L. Dubovsky, V.A. Rubakov, and P.G. Tinyakov, Phys. Rev. D 62, 105011 (2000);
31. R. Casadio, A. Gruppuso, and G. Venturi, Phys. Lett. B 495, 378 (2000).
32. A. Celotti, S.C. Miller, and D.W. Sciama, Class. Quantum Grav. 16, A3 (1999).
33. K. Kohri and J. Yokoyama, Phys. Rev. D 61, 023501 (2000);
34. B.J. Carr and J.H. MacGibbon, Phys. Rep. 307, 141 (1998);
35. F. Halzen, E. Zas, J.H. MacGibbon, and T.C. Weeks, Nature (London) 353, 807 (1991).
36. This is the initial mass of a PBH with r(6) of the order of the age of the Universe.
37. C. Alcock et al., Astrophys. J. 542, 281 (2000);
38. E. Roulet and S. Mollerach, Phys. Rep. 279, 67 (1997).
39. There are further contributions to m from the "strips" r-bL and raL, which can be controlled by keeping ci3=b and appropriately "smoothing" the O's.