• [1]

    R. Penrose, Riv. Nuovo Cim., 1: 252 (1969) [Gen. Rel. Grav., 34: 1141 (2002)]. doi: 10.1023/A:1016578408204

  • [2]

    D. Christodoulou, Phys. Rev. Lett., 25: 1596 (1970)

  • [3]

    J. M. Bardeen, Nature, 226: 64 (1970)

  • [4]

    D. Christodoulou and R. Ruffini, Phys. Rev. D, 4: 3552 (1971)

  • [5]

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

  • [6]

    J. D. Bekenstein, Phys. Rev. D, 7: 2333 (1973)

  • [7]

    J. M. Bardeen, B. Carter, and S. W. Hawking, Commun. Math. Phys., 31: 161 (1973)

  • [8]

    S. W. Hawking, Commun. Math. Phys., 43: 199 (1975) Erratum: [Commun. Math. Phys., 46: 206 (1976)] doi: 10.1007/ BF02345020, 10.1007/BF01608497

  • [9]

    J. M. Maldacena, Int. J. Theor. Phys., 38: 1113 (1999) [Adv. Theor. Math. Phys., 2: 231 (1998)] doi: 10.1023/ A:1026654312961,10.4310/ATMP.1998.v2.n2.a1[hep-th/9711200].

  • [10]

    S. W. Hawking and D. N. Page, Commun. Math. Phys., 87: 577 (1983)

  • [11]

    E. Witten, Adv. Theor. Math. Phys., 2: 505 (1998), arXiv:hep-th/9803131

  • [12]

    A. Chamblin, R. Emparan, C. V. Johnson et al., Phys. Rev. D, 60: 064018 (1999), arXiv:hep-th/9902170

  • [13]

    A. Chamblin, R. Emparan, C. V. Johnson et al., Phys. Rev. D, 60: 104026 (1999), arXiv:hep-th/9904197

  • [14]

    M. M. Caldarelli, G. Cognola, and D. Klemm, Class. Quant. Grav., 17: 399 (2000), arXiv:hepth/9908022

  • [15]

    R. G. Cai, Phys. Rev. D, 65: 084014 (2002), arXiv:hep-th/0109133

  • [16]

    D. Kubiznak and R. B. Mann, JHEP, 1207: 033 (2012), arXiv:1205.0559[hep-th

  • [17]

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

  • [18]

    B. P. Dolan, Class. Quant. Grav., 28: 235017 (2011), arXiv:1106.6260[gr-qc

  • [19]

    S. Gunasekaran, R. B. Mann, and D. Kubiznak, JHEP, 1211: 110 (2012), arXiv:1208.6251[hep-th

  • [20]

    S. W. Wei and Y. X. Liu, Phys. Rev. D, 87(4): 044014 (2013), arXiv:1209.1707[gr-qc

  • [21]

    R. G. Cai, L. M. Cao, L. Li et al., JHEP, 1309: 005 (2013), arXiv:1306.6233[gr-qc

  • [22]

    W. Xu and L. Zhao, Phys. Lett. B, 736: 214 (2014), arXiv:1405.7665[gr-qc

  • [23]

    A. M. Frassino, D. Kubiznak, R. B. Mann et al., JHEP, 1409: 080 (2014), arXiv:1406.7015[hep-th

  • [24]

    R. A. Hennigar, W. G. Brenna, and R. B. Mann, JHEP, 1507: 077 (2015), arXiv:1505.05517[hep-th

  • [25]

    P. Wang, H. Wu, and H. Yang, JCAP, 1904: 052 (2019), arXiv:1808.04506[gr-qc

  • [26]

    R. Wald, Ann. Phys., 82: 548 (1974)

  • [27]

    V. E. Hubeny, Phys. Rev. D, 59: 064013 (1999), arXiv:gr-qc/9808043

  • [28]

    T. Jacobson and T. P. Sotiriou, Phys. Rev. Lett., 103: 141101 (2009), arXiv:0907.4146[gr-qc

  • [29]

    A. Saa and R. Santarelli, Phys. Rev. D, 84: 027501 (2011), arXiv:1105.3950[gr-qc

  • [30]

    S. Hod, Phys. Rev. Lett., 100: 121101 (2008), arXiv:0805.3873[gr-qc

  • [31]

    E. Barausse, V. Cardoso, and G. Khanna, Phys. Rev. Lett., 105: 261102 (2010), arXiv:1008.5159[grqc

  • [32]

    E. Barausse, V. Cardoso, and G. Khanna, Phys. Rev. D, 84: 104006 (2011), arXiv:1106.1692[gr-qc

  • [33]

    P. Zimmerman, I. Vega, E. Poisson et al., Phys. Rev. D, 87(4): 041501 (2013), arXiv:1211.3889[gr-qc

  • [34]

    M. Colleoni and L. Barack, Phys. Rev. D, 91: 104024 (2015), arXiv:1501.07330[gr-qc

  • [35]

    M. Colleoni, L. Barack, A. G. Shah et al., Phys. Rev. D, 92(8): 084044 (2015), arXiv:1508.04031[gr-qc

  • [36]

    G. E. A. Matsas and A. R. R. da Silva, Phys. Rev. Lett., 99: 181301 (2007), arXiv:0706.3198[gr-qc

  • [37]

    M. Richartz and A. Saa, Phys. Rev. D, 78: 081503 (2008), arXiv:0804.3921[gr-qc

  • [38]

    S. Isoyama, N. Sago, and T. Tanaka, Phys. Rev. D, 84: 124024 (2011), arXiv:1108.6207[gr-qc

  • [39]

    S. Gao and Y. Zhang, Phys. Rev. D, 87(4): 044028 (2013), arXiv:1211.2631[gr-qc

  • [40]

    S. Hod, Phys. Rev. D, 87(2): 024037 (2013), arXiv:1302.6658[gr-qc

  • [41]

    K. Düzta and. Semiz, Phys. Rev. D, 88(6): 064043 (2013), arXiv:1307.1481[gr-qc

  • [42]

    H. M. Siahaan, Phys. Rev. D, 93(6): 064028 (2016), arXiv:1512.01654[gr-qc

  • [43]

    J. Natario, L. Queimada, and R. Vicente, Class. Quant. Grav., 33(17): 175002 (2016), arXiv:1601.06809[gr-qc

  • [44]

    K. Düzta, Phys. Rev. D, 94(12): 124031 (2016), arXiv:1701.07241[gr-qc

  • [45]

    K. S. Revelar and I. Vega, Phys. Rev. D, 96(6): 064010 (2017), arXiv:1706.07190[gr-qc

  • [46]

    J. Sorce and R. M. Wald, Phys. Rev. D, 96(10): 104014 (2017), arXiv:1707.05862[gr-qc

  • [47]

    V. Husain and S. Singh, Phys. Rev. D, 96(10): 104055 (2017), arXiv:1709.02395[gr-qc

  • [48]

    T. Crisford, G. T. Horowitz, and J. E. Santos, Phys. Rev. D, 97(6): 066005 (2018), arXiv:1709.07880[hep-th

  • [49]

    B. Gwak, JHEP, 1711: 129 (2017), arXiv:1709.08665[gr-qc

  • [50]

    J. An, J. Shan, H. Zhang et al., Phys. Rev. D, 97(10): 104007 (2018), arXiv:1711.04310[hep-th

  • [51]

    B. Ge, Y. Mo, S. Zhao et al., Phys. Lett. B, 783: 440 (2018), arXiv:1712.07342[hep-th

  • [52]

    T. Y. Yu and W. Y. Wen, Phys. Lett. B, 781: 713 (2018), arXiv:1803.07916[gr-qc

  • [53]

    B. Gwak, JHEP, 1809: 081 (2018), arXiv:1807.10630[gr-qc

  • [54]

    Y. Gim and B. Gwak, Phys. Lett. B, 794: 122 (2019), arXiv:1808.05943[gr-qc

  • [55]

    D. Chen, Chin. Phys. C, 44(1): 015101 (2020), arXiv:1812.03459[gr-qc

  • [56]

    X. X. Zeng and H. Q. Zhang, Thermodynamics and weak cosmic censorship conjecture in Born-Infeldanti-de Sitter black holes, arXiv: 1901.04247[hep-th]

  • [57]

    D. Chen, W. Yang, and X. Zeng, Nucl. Phys. B, 946: 114722 (2019), arXiv:1901.05140[hep-th

  • [58]

    B. Gwak, JCAP, 1908: 016 (2019), arXiv:1901.05589[grqc

  • [59]

    X. X. Zeng, Y. W. Han, and D. Y. Chen, Chin. Phys. C, 43(10): 105104 (2019), arXiv:1901.08915[gr-qc

  • [60]

    D. Chen, Eur. Phys. J. C, 79(4): 353 (2019), arXiv:1902.06489[hep-th

  • [61]

    P. Wang, H. Wu, and H. Yang, Eur. Phys. J. C, 79(7): 572 (2019)

  • [62]

    X. X. Zeng, X. Y. Hu, and K. J. He, Nucl. Phys. B, 949: 114823 (2019), arXiv:1905.07750[hep-th

  • [63]

    W. Hong, B. Mu, and J. Tao, Nucl. Phys. B, 949: 114826 (2019), arXiv:1905.07747[gr-qc

  • [64]

    T. T. Hu, Y. Song, S. Sun et al., Eur. Phys. J. C, 80(2): 147 (2020), arXiv:1906.00235[hep-th

  • [65]

    S. Q. Hu, Y. C. Ong, and D. N. Page, Phys. Rev. D, 100(10): 104022 (2019), arXiv:1906.05870[gr-qc

  • [66]

    B. Mu and J. Tao, Minimal Length Effect on Thermodynamics and Weak Cosmic Censorship Conjecture in anti-de Sitter Black Holes via Charged Particle Absorption, arXiv: 1906.10544[gr-qc]

  • [67]

    K. J. He, X. Y. Hu, and X. X. Zeng, Chin. Phys. C, 43(12): 125101 (2019), arXiv:1906.10531[gr-qc

  • [68]

    Q. Gan, G. Guo, P. Wang et al., Phys. Rev. D, 100(12): 124009 (2019), arXiv:1907.04466[hep-th

  • [69]

    X. X. Zeng and X. Y. Hu, Thermodynamics and weak cosmic censorship conjecture with pressure in the rotating BTZ black holes, arXiv: 1908.03845[gr-qc]

  • [70]

    K. J. He, G. P. Li, and X. Y. Hu, Eur. Phys. J. C, 80(3): 209 (2020), arXiv:1909.09956[hep-th

  • [71]

    S. Q. Hu, B. Liu, X. M. Kuang et al., Revisiting Black Hole Thermodynamics in Massive Gravity: Charged Particle Absorption and Shell of Dust Falling, arXiv: 1910.04437 [gr-qc]

  • [72]

    B. Gwak, JCAP, 2003(03): 058 (2020), arXiv:1910.13329[gr-qc

  • [73]

    Q. Gan, P. Wang, H. Wu et al., Strong Cosmic Censorship for a Scalar Field in an EinsteinMaxwell-Gauss-Bonnet-de Sitter Black Hole, arXiv: 1911.10996[gr-qc]

  • [74]

    W. Hong, B. Mu, and J. Tao, Test the Weak Cosmic Censorship Conjecture in Torus-Like Black Hole under Charged Scalar Field, arXiv: 2001.09008[physics.gen-ph]

  • [75]

    B. Gwak, Thermodynamics in Rotating Anti-de Sitter Black Holes with Massive Scalar Field in Three Dimensions, arXiv: 2002.09729 [gr-qc]

  • [76]

    P. Wang, H. Wu, and S. Ying, Validity of Thermodynamic Laws and Weak Cosmic Censorship for AdS Black Holes and Black Holes in a Cavity, arXiv: 2002.12233[gr-qc]

  • [77]

    Y. Zhang and S. Gao, Int. J. Mod. Phys. D, 23: 1450044 (2014), arXiv:1309.2027[gr-qc

  • [78]

    D. Glavan and C. Lin, Phys. Rev. Lett., 124(8): 081301 (2020), arXiv:1905.03601[gr-qc

  • [79]

    H. Lu and Y. Pang, Horndeski Gravity as D → 4 Limit of Gauss-Bonnet, arXiv: 2003.11552[gr-qc]

  • [80]

    W. Y. Ai, A note on the novel 4D Einstein-Gauss-Bonnet gravity, arXiv: 2004.02858[gr-qc]

  • [81]

    P. G. S. Fernandes, Charged Black Holes in AdS Spaces in 4D Einstein Gauss-Bonnet Gravity, arXiv: 2003.05491[gr-qc]

  • [82]

    K. Hegde, A. Naveena Kumara, C. L. A. Rizwan et al., Thermodynamics, Phase Transition and Joule Thomson Expansion of novel 4-D Gauss Bonnet AdS Black Hole, arXiv: 2003.08778 [gr-qc]

  • [83]

    D. V. Singh and S. Siwach, Thermodynamics and P-v criticality of Bardeen-AdS Black Hole in 4-D Einstein-Gauss-Bonnet Gravity, arXiv: 2003.11754[gr-qc]

  • [84]

    S. A. Hosseini Mansoori, Thermodynamic geometry of novel 4-D Gauss Bonnet AdS Black Hole, arXiv: 2003.13382[gr-qc]

  • [85]

    S. W. Wei and Y. X. Liu, Extended thermodynamics and microstructures of four-dimensional charged Gauss-Bonnet black hole in AdS space, arXiv: 2003.14275[gr-qc]

  • [86]

    B. Eslam Panah and K. Jafarzade, 4D Einstein-Gauss-Bonnet AdS Black Holes as Heat Engine, arXiv: 2004.04058[hep-th]

  • [87]

    R. A. Konoplya and A. F. Zinhailo, Quasinormal modes, stability and shadows of a black hole in the novel 4D Einstein-Gauss-Bonnet gravity, arXiv: 2003.01188[gr-qc]

  • [88]

    R. A. Konoplya and A. Zhidenko, (In)stability of black holes in the 4D Einstein-Gauss-Bonnet and EinsteinLovelock gravities, arXiv: 2003.12492[gr-qc]

  • [89]

    S. L. Li, P. Wu, and H. Yu, Stability of the Einstein Static Universe in 4D Gauss-Bonnet Gravity, arXiv: 2004.02080[gr-qc]

  • [90]

    C. Y. Zhang, S. J. Zhang, P. C. Li et al., Superradiance and stability of the novel 4D charged Einstein-Gauss-Bonnet black hole, arXiv: 2004.03141[gr-qc]

  • [91]

    A. K. Mishra, Quasinormal modes and Strong Cosmic Censorship in the novel 4D Einstein-Gauss-Bonnet gravity, arXiv: 2004.01243[gr-qc]

  • [92]

    S. Hendi, S. Panahiyan, and M. Momennia, Int. J. Mod. Phys. D, 25(06): 1650063 (2016), arXiv:1503.03340[gr-qc

  • [93]

    S. H. Hendi, G. Q. Li, J. X. Mo et al., Eur. Phys. J. C, 76(10): 571 (2016), arXiv:1608.03148[gr-qc

  • [94]

    S. Hendi, B. Panah, and S. Panahiyan, Fortsch. Phys., 66(3): 1800005 (2018), arXiv:1708.02239[hep-th

  • [95]

    B. Mu, P. Wang, and H. Yang, Adv. High Energy Phys., 2017: 3191839 (2017), arXiv:1408.5055[gr-qc

  • [96]

    J. Tao, P. Wang, and H. Yang, Nucl. Phys. B, 922: 346 (2017), arXiv:1505.03045[grqc

  • [97]

    S. Yang, J. Wan, J. Chen et al., Weak cosmic censorship conjecture for the novel 4D charged Einstein-Gauss-Bonnet black hole with test scalar field and particle, arXiv: 2004.07934[gr-qc]