• [1]

    S. W. Hawking, Phys. Rev. D, 14: 2460-2473 (1976)

  • [2]

    S. Chakraborty and K. Lochan, Universe, 3(3): 55 (2017)

  • [3]

    D. Marolf, Rept. Prog. Phys., 80(9): 092001 (2017)

  • [4]

    S. W. Hawking, M. J. Perry, and A. Strominger, Phys. Rev. Lett., 116(23): 231301 (2016)

  • [5]

    A. Strominger (Lectures on the Infrared Structure of Gravity and Gauge Theory), (2017), arXiv:1703.05448

  • [6]

    M. Stafford. A Review of Soft Black Hole Hair and Its Potential as a Solution to the Information Paradox. Master’s thesis, (Imperial Coll., London, 2017)

  • [7]

    H. Afshar, D. Grumiller, and M. M. Sheikh-Jabbari, Phys. Rev. D, 96(8): 084032 (2017)

  • [8]

    M. M. Sheikh-Jabbari and H. Yavartanoo, Phys. Rev. D, 95(4): 044007 (2017)

  • [9]

    H. Afshar, D. Grumiller, M. M. Sheikh-Jabbari et al, JHEP, 08: 087 (2017)

  • [10]

    H. Afshar, S. Detournay, D. Grumiller et al, Phys. Rev. D, 93(10): 101503 (2016)

  • [11]

    H. Afshar, D. Grumiller, W. Merbis et al, Phys. Rev. D, 95(10): 106005 (2017)

  • [12]

    J. Wang (Black hole as topological insulator (I): the BTZ black hole case), (2017), arXiv:1703.09365

  • [13]

    J. Wang (Black hole as topological insulator (II): the boundary modes), (2017), arXiv:1706.01630

  • [14]

    J. R. Ellis, N. E. Mavromatos, and D. V. Nanopoulos, Phys. Lett. B, 267: 465-474 (1991)

  • [15]

    J. R. Ellis, N. E. Mavromatos, and D. V. Nanopoulos, Phys. Lett. B, 278: 246-256 (1992)

  • [16]

    J. R. Ellis, N. E. Mavromatos, and D. V. Nanopoulos, Phys. Lett. B, 284: 27-35 (1992)

  • [17]

    J. R. Ellis, N. E. Mavromatos, and D. V. Nanopoulos, Phys. Lett. B, 284: 43-49 (1992)

  • [18]

    J. R. Ellis, N. E. Mavromatos, and D. V. Nanopoulos, Phys. Rev. D, 94(2): 025007 (2016)

  • [19]

    L. Bonora and M. Cvitan, JHEP, 05: 071 (2008)

  • [20]

    L. Bonora, M. Cvitan, S. Pallua et al, JHEP, 12: 021 (2008)

  • [21]

    L. Bonora, M. Cvitan, S. Pallua et al, Phys. Rev. D, 80: 084034 (2009)

  • [22]

    S. Iso, T. Morita, and H. Umetsu, Phys. Rev. D, 75: 124004 (2007)

  • [23]

    S. Iso, T. Morita, and H. Umetsu, Phys. Rev. D, 76: 064015 (2007)

  • [24]

    S. Iso, T. Morita, and H. Umetsu, Nucl. Phys. B, 799: 60-79 (2008)

  • [25]

    X. Shen, Int. J. Mod. Phys. A, 7: 6953-6994 (1992)

  • [26]

    V. Kac and A. Radul, Commun. Math. Phys., 157: 429-457 (1993)

  • [27]

    E. Frenkel, V. Kac, A. Radul et al, Commun. Math. Phys., 170: 337-358 (1995)

  • [28]

    A. Cappelli, C. A. Trugenberger, and G. R. Zemba, Nucl. Phys. B, 396: 465-490 (1993)

  • [29]

    A. Cappelli, C. A. Trugenberger, and G. R. Zemba, Phys. Rev. Lett., 72: 1902-1905 (1994)

  • [30]

    J. Wang and C.-G. Huang, Chin. Phys. C, 42(12): 123110 (2018)

  • [31]

    A. Cappelli, C. A. Trugenberger, and G. R. Zemba, Nucl. Phys. B, 448: 470 (1995)

  • [32]

    L. Donnay, G. Giribet, H. A. Gonzalez et al, Phys. Rev. Lett., 116(9): 091101 (2016)

  • [33]

    F. Philippe, M. Pierre, and S. David. Conformal Field Theory, (Springer, 1999)

  • [34]

    M. Banados, C. Teitelboim, and J. Zanelli, Phys. Rev. Lett., 69: 1849-1851 (1992)

  • [35]

    G. Hardy and S. Ramanujan, Proceedings of the London Mathematical Society, 2(XVII): 75 (1918)

  • [36]

    R. F. Penna, JHEP, 10: 049 (2017)

  • [37]

    B. L. Hu, Int. J. Theor. Phys., 44: 1785-1806 (2005)

  • [38]

    G. E. Volovik, Phil. Trans. Roy. Soc. Lond. A, 366: 2935-2951 (2008)

  • [39]

    S. Liberati, F. Girelli, and L. Sindoni. Analogue Models for Emergent Gravity. In 18th SIGRAV Conference Cosenza, Italy, September 22-25, 2008

  • [40]

    D. Vaid, Adv. High Energy Phys., 2017: 7935185 (2017)