\begin{document}$ T-S $\end{document} and isothermal \begin{document}$ \Phi-Q_e $\end{document} behaviors, the absence of the Hawking-Page transition is another notable feature. However, in the high temperature limit, the thermodynamic behavior of the present model becomes exactly the same as that of the Einstein gravity and black hole scan models, which adds further evidence for the universality of the recently reported correspondence between high temperature AdS black holes and low temperature quantum phonon gases in nonmetallic crystals."> Restricted phase space thermodynamics of charged AdS black holes in conformal gravity -
  • [1]

    J. Maldacena,Einstein Gravity from Conformal Gravity, arXiv:10.1105.5632

  • [2]

    P. D. Mannheim and J. G. O'Brien, J. Phys.: Conf. Ser.437, 012002 (2013), arXiv:1211.0188

  • [3]

    R. K. Nesbet, Entropy15, 162-176 (2013), arXiv:1208.4972

  • [4]

    H. Lu and C. N. Pope, Phys. Rev. Lett.106, 181302 (2011), arXiv:1101.1971

  • [5]

    J. Li, H. -S. Liu, H. Luet al., JHEP02, 109 (2013), arXiv:1210.5000

  • [6]

    H. Lu, Y. Pang, C. N. Popeet al., Phys. Rev. D86, 044011 (2012), arXiv:1204.1062

  • [7]

    J. D. Bekenstein, Lett. Nuovo Cim.4(15), 737 (1972)

  • [8]

    J. D. Bekenstein, Phys. Rev. D7(8), 2333-2346 (1973)

  • [9]

    J. M. Bardeen, B. Carter, and S. W. Hawking, Comm. Math. Phys.31(2), 161-170 (1973)

  • [10]

    S. W. Hawking, Comm. Math. Phys.43, 199-220 (1975)

  • [11]

    J. D. Bekenstein, Phys. Rev. D12(10), 3077 (1975)

  • [12]

    D. Kastor, S. Ray, and J. Traschen, Class. Quant. Grav.26(19), 195011 (2009), arXiv:0904.2765

  • [13]

    B. P. Dolan, Class. Quant. Grav.28(12), 125020 (2010), arXiv:1008.5023

  • [14]

    Dolan, B. P, Class. Quant. Grav.28(23), 235017 (2011), arXiv:1106.6260

  • [15]

    B. P. Dolan, Phys. Rev. D84(12), 127503 (2011), arXiv:1109.0198

  • [16]

    D. Kubizňák and R. B. Mann, JHEP7, 33 (2012), arXiv:1205.0559

  • [17]

    S. Gunasekaran, R. B. Mann, and D. Kubizňák, JHEP11, 110 (2012), arXiv:1208.6251

  • [18]

    A. Belhaj, M. Chabab, H. El Moumniet al., Chin. Phys. Lett.29, 100401 (2012), arXiv:1210.4617

  • [19]

    S. H. Hendi and M. H. Vahidinia, Phys. Rev. D88, 084045 (2013), arXiv:1212.6128

  • [20]

    S. Chen, X. Liu, C. Liuet al., Chin. Phys. Lett.30, 060401 (2013), arXiv:1301.3234

  • [21]

    R. Zhao, H. H. Zhao, M. S. Maet al., Eur. Phys. J. C73, 2645 (2013), arXiv:1305.3725

  • [22]

    M. B. J. Poshteh, B. Mirza, and Z. Sherkatghanad, Phys. Rev. D88(2), 024005 (2013), arXiv:1306.4516

  • [23]

    N. Altamirano, D. Kubizňák, and R. B. Mann, Phys. Rev. D88, 101502 (2013), arXiv:1306.5756

  • [24]

    R. G. Cai, L. M. Cao, L. Liet al., JHEP9, 5 (2013), arXiv:1306.6233

  • [25]

    A. Belhaj, M. Chabab, H. El. Moumniet al., Chin. Phys. Lett.30, 090402 (2013), arXiv:1307.7421

  • [26]

    N. Altamirano, D. Kubizňák, R. B. Mannet al., Class. Quant. Grav.31, 042001 (2014), arXiv:1308.2672

  • [27]

    W. Xu, H. Xu, and L. Zhao, Euro. Phys. J. C74(7), 2970 (2014), arXiv:1311.3053

  • [28]

    D. -C. Zou, S. -J. Zhang, and B. Wang, Phys. Rev. D89, 044002 (2014), arXiv:1311.7299

  • [29]

    N. Altamirano, D. Kubizňák, R. B. Mannet al., Galaxies2, 89 (2014), arXiv:1401.2586

  • [30]

    S. -W. Wei and Y. -X. Liu, Phys. Rev. D90, 044057 (2014), arXiv:1402.2837

  • [31]

    D. Kubizňák and R. B. Mann,Black Hole Chemistry, arXiv:10.1404.2126

  • [32]

    D. -C. Zou, Y. Liu, and B. Wang, Phys. Rev. D90, 044063 (2014), arXiv:1404.5194

  • [33]

    H. Xu, W. Xu, and L. Zhao, Euro. Phys.J. C74, 3074 (2014), arXiv:1405.4143

  • [34]

    J. L. Zhang, R. G. Cai, and H. Yu, Phys. Rev. D91(4), 044028 (2015), arXiv:1502.01428

  • [35]

    D. Kubizňák, R. B. Mann, and M. Teo, Class. Quant. Grav.34(6), 063001 (2017), arXiv:1608.06147

  • [36]

    J. P. S. Lemos and O. B. Zaslavskii, Phys. Lett. B786, 296-299 (2018), arXiv:1806.07910

  • [37]

    W. Xu and L. Zhao, Phys. Lett. B736, 214-220 (2014), arXiv:1405.7665

  • [38]

    S. -W. Wei and Y. -X. Liu, Phys. Rev. Lett.115(11), 111302 (2015), arXiv:1502.00386

  • [39]

    A. Dehyadegari, A. Sheykhi, and S. -W. Wei, Phys. Rev. D102(10), 104013 (2020), arXiv:2006.12265

  • [40]

    S. -W. Wei and Y. -X. Liu, Phys. Rev. D101(10), 104018 (2020), arXiv:2003.14275

  • [41]

    M. R. Visser, Phys. Rev. D105, 106014 (2022), arXiv:2101.04145

  • [42]

    W. Cong, D. Kubizňák, and R. B. Mann, Phys. Rev. Lett.127, 091301 (2021), arXiv:2105.02223

  • [43]

    R. B. Alfaia, I. P. Lobo, and L. C. T. Brito, Eur. Phys. J. Plus137, 402 (2022), arXiv:2109.06599

  • [44]

    Z. Gao and L. Zhao, Class. Quant. Grav.39, 075019 (2021), arXiv:2112.02386

  • [45]

    Z. Gao, X. Kong, and L. Zhao, Euro. Phys. J. C82(2), 112 (2022), arXiv:2112.08672

  • [46]

    T. Wang and L. Zhao, Phys. Lett. B827, 136935 (2022), arXiv:2112.11236

  • [47]

    L. Zhao, Chin. Phys. C46(5), 055105 (2022), arXiv:2201.00521

  • [48]

    X. Kong, T. Wang, Z. Gaoet al., Entropy24(8), 1131 (2022), arXiv:2208.07748

  • [49]

    X. Kong, T. Wang, and L. Zhao,High temperature AdS black holes are low temperature quantum phonon gases, arXiv:10.2209.12230

  • [50]

    J. Sadeghi, M. Shokri, S. N. Gashtiet al., Gen. Rel. Grav.54, 129 (2022), arXiv:2205.03648

  • [51]

    Y. Y. Bai, X. R. Chen, Z. M. Xuet al. Revisit on thermodynamics of BTZ black hole with variable Newton constant, arXiv:10.2208.11859

  • [52]

    Y.-Z. Du, H.-F. Li, Y. Zhanget al. Restricted phase space thermodynamics of Einstein-power-Yang-Mills AdS black hole, arXiv:10.2210.02006

  • [53]

    C. Wang, S. P. Yin, Z. M. Xuet al. Ruppeiner geometry and the fluctuation of the RN-AdS black hole in framework of the extensive thermodynamics, arXiv:10.2210.08822

  • [54]

    S. W. Hawking and D. N. Page, Commun. Math. Phys.98, 577 (1983)

Baidu
map