Chin. Phys. Lett.  2007, Vol. 24 Issue (9): 2497-2500    DOI:
Original Articles |
Generalized Uncertainty Principle and the Quantum Entropy of Rotating Black Hole
SHU Fu-Wen1,3,4;SHEN You-Gen 1,2,3
1Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 2000302National Astronomical Observatories, Chinese Academy of Sciences,Beijing 1000123Joint Institute for Galaxy and Cosmology of SHAO and USTC, Shanghai 2000304Graduate School of the Chinese Academy of Sciences, Beijing 100049
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SHU Fu-Wen, SHEN You-Gen 2007 Chin. Phys. Lett. 24 2497-2500
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Abstract The entropy of rotating Kerr--Newman--Kasuya black hole due to massive
charged fields (bosons and fermions) is calculated by using the new equation of state density motivated by the generalized uncertainty relation. The result shows the entropy does not depend on the mass and the charge but the parameter λ, the area A and the spin of the fields. Moreover, an improved approximation is provided to calculate the scalar entropy.
Keywords: 04.70.Dy      98.80.Cq     
Received: 09 April 2007      Published: 16 August 2007
PACS:  04.70.Dy (Quantum aspects of black holes, evaporation, thermodynamics)  
  98.80.Cq (Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.))  
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SHU Fu-Wen
SHEN You-Gen
[1]Christodolou D 1970 Phys. Rev. Lett. 25 1596 Christodolou D and Ruffini R 1971 Phys. Rev. D 4 3552
[2] Carter B 1972 Nature 238 71
[3]Bekenstein J D 1973 Phys. Rev. D 7 2333
[4]Hawking S W 1975 Commun. Math. Phys. 43 199
[5]'t Hooft G 1985 Nucl. Phys. B 256 727
[6]Susskind L and Uglum L 1995 Phys. Rev. D 50 2700
[7]Xiang L 2002 Phys. Lett. B 540 9
[8]Medved A J M and Vagenas E C2004 Phys. Rev. D 70 124021
[9]Nozari K and Sefidgar A S 2006 Preprint gr-qc/0606046
[10]Li C, Xiang L and Shen Y G2004 Int. J. Mod. Phys. D 13 1847
[11]Kasuya M 1982 Phys. Rev. D 25 995
[12]Shen Y G 1987 Math. Phys. Acta 7 89
[13]Gao C J and Shen Y G2002 Class. Quantum Grav. 194933
[14]Chang L N, Minic D, Okaruma N and Takeuchi T2002 Phys.Rev. D 65 125028
[15]Thorne K S, Zurek W H and Price R H 1986 Blackholes: The Membrane Paradigm ed Thorne K S, Price R H and Macdonald D A (New Haven, CT: Yale University Press)
[16]Chandrasekhar S 1983 The mathematical Theory of BlackHoles (New York: Oxford University Press)
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