Geodesic
Tunneling radiation of a Gibbons–Maeda dilaton black hole
Teoretičeskaâ i matematičeskaâ fizika, Tome 151 (2007) no. 1, pp. 172-175 Cet article a éte moissonné depuis la source Math-Net.Ru

Voir la notice de l'article

We use the Parikh–Wilczek method to treat Hawking radiation as a tunneling process across the event horizon and calculate the emission rate of a Gibbons–Maeda dilaton black hole. We show that if self-gravitation is taken into account, then the radiation deviates from the purely thermal spectrum, and the corrected spectrum is consistent with an underlying unitary theory.
Keywords: tunneling radiation, energy conservation, self-gravitation, black hole. 
@article{TMF_2007_151_1_a11,
     author = {Li Gu Qiang},
     title = {Tunneling radiation of {a~Gibbons{\textendash}Maeda} dilaton black hole},
     journal = {Teoreti\v{c}eska\^a i matemati\v{c}eska\^a fizika},
     pages = {172--175},
     year = {2007},
     volume = {151},
     number = {1},
     language = {ru},
     url = {http://geodesic.mathdoc.fr/item/TMF_2007_151_1_a11/}
}
TY  - JOUR
AU  - Li Gu Qiang
TI  - Tunneling radiation of a Gibbons–Maeda dilaton black hole
JO  - Teoretičeskaâ i matematičeskaâ fizika
PY  - 2007
SP  - 172
EP  - 175
VL  - 151
IS  - 1
UR  - http://geodesic.mathdoc.fr/item/TMF_2007_151_1_a11/
LA  - ru
ID  - TMF_2007_151_1_a11
ER  - 
%0 Journal Article
%A Li Gu Qiang
%T Tunneling radiation of a Gibbons–Maeda dilaton black hole
%J Teoretičeskaâ i matematičeskaâ fizika
%D 2007
%P 172-175
%V 151
%N 1
%U http://geodesic.mathdoc.fr/item/TMF_2007_151_1_a11/
%G ru
%F TMF_2007_151_1_a11
Li Gu Qiang. Tunneling radiation of a Gibbons–Maeda dilaton black hole. Teoretičeskaâ i matematičeskaâ fizika, Tome 151 (2007) no. 1, pp. 172-175. http://geodesic.mathdoc.fr/item/TMF_2007_151_1_a11/

[1] S. W. Hawking, Commun. Math. Phys., 43 (1975), 199 | DOI | MR | Zbl

[2] G. W. Gibbons, S. W. Hawking, Phys. Rev. D, 15 (1977), 2752 ; W. B. Liu, Z. Zhao, Chin. Phys. Lett., 18 (2001), 310 ; S. Z. Yang, L. B. Lin, Chin. Phys., 11 (2002), 619 ; J. L. Jing, Chin. Phys. Lett., 20 (2003), 459 ; Q. Q. Jiang, S. Z. Yang, H. L. Li, Chin. Phys., 14 (2005), 1736 | DOI | MR | DOI | Zbl | DOI | DOI | DOI

[3] P. Kraus, F. Wilczek, Nucl. Phys. B, 433 (1995), 403 | DOI

[4] M. K. Parikh, F. Wilczek, Phys. Rev. Lett., 85 (2000), 5042 | DOI | MR

[5] J. Y. Zhang, Z. Zhao, JHEP, 0510 (2005), 055 ; Mod. Phys. Lett. A, 20 (2005), 1673 ; Nucl. Phys. B, 725 (2005), 173 ; Y. W. Han, S. Z. Yang, Chin. Phys. Lett., 22 (2005), 2769 ; A. J. Medved, Phys. Rev. D, 66 (2002), 124009 ; S. Hemming, E. Keski-Vakkuri, Phys. Rev. D, 64 (2001), 044006 | DOI | DOI | Zbl | DOI | MR | Zbl | DOI | DOI | MR | DOI | MR

[6] Y. G. Shen, Phys. Lett. A, 266 (2000), 234 | DOI | MR | Zbl

[7] E. Keski-Vakkuri, P. Kraus, Nucl. Phys. B, 491 (1997), 249 | DOI | MR | Zbl

[8] J. Y. Zhang, Z. Zhao, Phys. Lett. B, 618 (2005), 14 | DOI | MR | Zbl