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Black holes remnants in extra dimensions and dark matter. (English) Zbl 1133.83361

Summary: Bekenstein–Hawking formalism of black hole thermodynamics should be modified to incorporate quantum gravitational effects. Generalized Uncertainty Principle (GUP) provides a suitable framework to perform such modifications. In this paper, we consider a general form of GUP to find black hole thermodynamics in a model universe with large extra dimensions. We will show that black holes radiate mainly in the four-dimensional brane. Existence of black holes remnants as a possible candidate for dark matter is discussed.

MSC:

83C57 Black holes
83E15 Kaluza-Klein and other higher-dimensional theories
80A10 Classical and relativistic thermodynamics
83C45 Quantization of the gravitational field
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References:

[1] DOI: 10.1016/S0370-2693(98)00466-3 · Zbl 1355.81103
[2] DOI: 10.1016/S0370-2693(98)00860-0
[3] DOI: 10.1103/PhysRevD.59.086004
[4] DOI: 10.1103/PhysRevLett.83.4690 · Zbl 0946.81074
[5] DOI: 10.1103/PhysRevLett.83.3370 · Zbl 0946.81063
[6] DOI: 10.1103/PhysRevLett.88.021303
[7] DOI: 10.1016/S0370-2693(01)01421-6 · Zbl 01686885
[8] Ringwald A., Phys. Lett. B 529 pp 1–
[9] Ave M., Phys. Rev. D 68 pp 043004–
[10] DOI: 10.1103/PhysRevD.66.033002
[11] DOI: 10.1103/PhysRevD.65.064023
[12] DOI: 10.1142/S0218271803004316
[13] DOI: 10.1142/S0217751X03013569 · Zbl 1035.83023
[14] DOI: 10.1016/j.physletb.2003.06.065 · Zbl 01969754
[15] DOI: 10.1103/PhysRevLett.85.499 · Zbl 1369.83039
[16] DOI: 10.1103/PhysRevD.67.064025
[17] Harris C. M., J. High Energy Phys. 0310 pp 014–
[18] DOI: 10.1103/PhysRevD.66.024023
[19] DOI: 10.1103/PhysRevD.67.104019
[20] DOI: 10.1016/0370-2693(89)91366-X
[21] DOI: 10.1016/0550-3213(90)90375-N
[22] DOI: 10.1016/0550-3213(93)90367-X
[23] DOI: 10.1016/0370-2693(90)91927-4
[24] DOI: 10.1103/PhysRevD.49.5182
[25] DOI: 10.1016/0370-2693(93)90785-G
[26] DOI: 10.1103/PhysRevD.52.1108
[27] DOI: 10.1016/0370-2693(93)91401-8
[28] DOI: 10.1016/S0370-2693(99)00167-7
[29] DOI: 10.1088/0264-9381/20/18/305 · Zbl 1048.83009
[30] DOI: 10.1023/A:1015281430411 · Zbl 1003.83020
[31] Medved A. J. M., Phys. Rev. D 70 pp 1240–
[32] DOI: 10.1088/0264-9381/22/1/009 · Zbl 1060.83522
[33] DOI: 10.1088/0264-9381/20/15/303 · Zbl 1108.83304
[34] DOI: 10.1016/S0370-2693(98)01184-8
[35] Chamblin A., Phys. Rev. D 61 pp 0605007–
[36] DOI: 10.1103/PhysRevLett.85.499 · Zbl 1369.83039
[37] DOI: 10.1103/PhysRevD.54.5174
[38] DOI: 10.1142/S0217732399001462
[39] DOI: 10.1103/PhysRevD.52.1108
[40] DOI: 10.1016/j.physletb.2003.09.040 · Zbl 1029.83501
[41] H. Ohanian and R. Ruffini, Gravitation and Spacetime, 2nd edn. (W. W. Norton, 1994) p. 481.
[42] Adler R. J., Phys. Rev. D 14 pp 2472–
[43] Hanni R. S., Black Holes (1973)
[44] Christodoulou D., Phys. Rev. D 4 pp 3352–
[45] DOI: 10.1088/0264-9381/20/15/101 · Zbl 1044.83502
[46] Zeldovich Ya. B., Sov. Astron. 10 pp 602–
[47] DOI: 10.1093/mnras/152.1.75
[48] DOI: 10.1103/PhysRevD.49.6410
[49] DOI: 10.1016/S0370-1573(98)00128-8
[50] DOI: 10.1016/S0370-1573(00)00038-7
[51] DOI: 10.1016/j.newar.2005.01.015
[52] DOI: 10.1142/S0217751X03013569 · Zbl 1035.83023
[53] DOI: 10.1103/PhysRevD.64.093010
[54] DOI: 10.1103/PhysRevLett.16.748
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