By using the Euclidean action and the semi-classical approach, the statistical mechanics of a three dimensional (3D) gas of non-spinning Banados, Teitelboim and Zaneli black holes is discussed. We have found that, unlike the 4D and 2D black hole gases, both the microcanonical ensemble and the canonical ensemble can be used to describe the thermodynamical properties of a 3D gas at any temperature. No critical temperature can exist.
机构:
Cent China Normal Univ, Inst Particle Phys, Wuhan 430079, Hubei, Peoples R ChinaCent China Normal Univ, Inst Particle Phys, Wuhan 430079, Hubei, Peoples R China
Jiang, Qing-Quan
Wu, Shuang-Qing
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机构:Cent China Normal Univ, Inst Particle Phys, Wuhan 430079, Hubei, Peoples R China
Wu, Shuang-Qing
Cai, Xu
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机构:Cent China Normal Univ, Inst Particle Phys, Wuhan 430079, Hubei, Peoples R China
机构:
Natl Univ La Plata, CEFIMAS, CC 67, RA-1900 La Plata, Argentina
Natl Univ La Plata, Dept Fis, RA-1900 La Plata, ArgentinaNatl Univ La Plata, CEFIMAS, CC 67, RA-1900 La Plata, Argentina
机构:
Korea Adv Inst Sci & Technol, Dept Phys, Taejon 305701, South KoreaKorea Adv Inst Sci & Technol, Dept Phys, Taejon 305701, South Korea
Hwang, Dong-il
Kim, Hongbin
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Yonsei Univ, Dept Phys, Coll Sci, Seoul 120749, South KoreaKorea Adv Inst Sci & Technol, Dept Phys, Taejon 305701, South Korea
Kim, Hongbin
Yeom, Dong-han
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Korea Adv Inst Sci & Technol, Dept Phys, Taejon 305701, South Korea
Sogang Univ, Ctr Quantum Spacetime, Seoul 121742, South Korea
Sogang Univ, Res Inst Basic Sci, Seoul 121742, South KoreaKorea Adv Inst Sci & Technol, Dept Phys, Taejon 305701, South Korea