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Hawking radiation from a five-dimensional Lovelock black hole |
Mahamat Saleh1,2( ),Bouetou Thomas Bouetou1,3,*( ),Timoleon Crepin Kofane4,*( ) |
1. Department of Physics, Faculty of Science, University of Yaoundé I, P.O. Box 812, Yaoundé, Cameroon 2. Department of Physics, Higher Teachers’ Training College, University of Maroua, P.O. Box 55, Maroua, Cameroon 3. National Advanced School of Engineering, University of Yaoundé I, P.O. Box 8390, Yaoundé, Cameroon 4. The Max Planck Institute for the Physics of Complex Systems, Nöthnitzer Strasse 38, 01187 Dresden, Germany |
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Abstract We investigate Hawking radiation from a five-dimensional Lovelock black hole using the Hamilton–Jacobi method. The behavior of the rate of radiation is plotted for various values of the ultraviolet correction parameter and the cosmological constant. The results show that, owing to the ultraviolet correction and the presence of dark energy represented by the cosmological constant, the black hole radiates at a slower rate in comparison to the case without ultraviolet correction or cosmological constant. Moreover, the presence of the cosmological constant makes the effect of the ultraviolet correction on the black hole radiation negligible.
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Keywords
Hawking radiation
Lovelock black hole
Hamilton–Jacobi method
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Corresponding Author(s):
Bouetou Thomas Bouetou,Timoleon Crepin Kofane
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Issue Date: 26 October 2015
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