\begin{document}$ z=1 $\end{document}, \begin{document}$ d=1 $\end{document}, and \begin{document}$ \theta\rightarrow0^{-} $\end{document}, we link WGC to hyperscaling violating black holes owing to the existence of \begin{document}$ r_{H} $\end{document} values larger and smaller than one. For the second black hole system, we study the conditions of WGC for Kerr-Newman-AdS black holes using rotation and radius parameters. Then, we show that the conditions of WGC are satisfied when the charged particle near the hyperscaling violating and Kerr-Newman black holes is \begin{document}$ \frac{1}{a} $\end{document} with a ratio \begin{document}$ \frac{a}{\ell}\ll 1 $\end{document}."> Weak gravity conjecture from conformal field theory: a challenge from hyperscaling violating and Kerr-Newman-AdS black holes -
  • [1]

    J. M. Maldacena, Adv. Theor. Math. Phys.2, 231-252 (1998)

  • [2]

    S. S. Gubser, I. R. Klebanov, and A. M. Polyakov, Phys. Lett. B428, 105-114 (1998)

  • [3]

    E. Witten, Adv. Theor. Math. Phys.2, 253-291 (1998)

  • [4]

    I. R. Klebanov and E. Witten, Nucl. Phys. B556, 89-114 (1999)

  • [5]

    M. Kioumarsipour and J. Sadeghi, Eur. Phys. J. C81(8), 735 (2021)

  • [6]

    Y. Bu and B. Zhang, Phys. Rev. D104(8), 086002 (2021)

  • [7]

    S. Fujiwara, Y. Imamura, and T. Mori, JHEP05, 221 (2021)

  • [8]

    N. Evans and J. Mitchell, Phys. Rev. D104(9), 094018 (2021)

  • [9]

    M. A. Martin Contreras, S. Diles, and A. Vega, Phys. Rev. D103(8), 086008 (2021)

  • [10]

    T. Gherghetta, J. I. Kapusta, and T. M. Kelley, Phys. Rev. D79, 076003 (2009)

  • [11]

    S. J. Brodsky and G. F. de Teramond, Phys. Rev. D77, 056007 (2008)

  • [12]

    E. Nakano, S. Teraguchi, and W.-Y. Wen, Phys. Rev. D75, 085016 (2007)

  • [13]

    E. Katz, A. Lewandowski, and M. D. Schwartz, Phys. Rev. D74, 086004 (2006)

  • [14]

    D. Meltzer, E. Perlmutter, and A. Sivaramakrishnan, JHEP03, 061 (2020)

  • [15]

    A. Karch, E. Katz, D. T. Son, and M. A. Stephanov, Phys. Rev. D74, 015005 (2006)

  • [16]

    O. Andreev and V. I. Zakharov, Phys. Rev. D74, 025023 (2006)

  • [17]

    A. Cavaglià, N. Gromov, and F. Levkovich-Maslyuk, JHEP06, 131 (2021)

  • [18]

    T. Harmark, J. Hartong, N. A. Obers, and G. Oling, JHEP03, 129 (2021)

  • [19]

    K. Bitaghsir Fadafan, A. O’Bannon, R. Rodgerset al., JHEP04, 162 (2021)

  • [20]

    M. De Leeuw, C. Paletta, A. Pribytoket al., JHEP02, 191 (2021)

  • [21]

    O. DeWolfe and K. Higginbotham, Phys. Rev. D103(2), 026011 (2021)

  • [22]

    S. Ishigaki and M. Matsumoto, JHEP04, 040 (2021)

  • [23]

    S. Terashima, Phys. Rev. D104(8), 086014 (2021)

  • [24]

    L. Yin, D. Hou, and H.-c. Ren, JHEP09, 117 (2021)

  • [25]

    A. K. Mes, R. W. Moerman, J. P. Shocket al., Annals Phys.436, 168675 (2022)

  • [26]

    D. Berenstein and D. Grabovsky, Class. Quant. Grav.38(10), 105008 (2021)

  • [27]

    R. J. Berman, T. C. Collins, and D. Persson, Nature Commun.13(1), 365 (2022)

  • [28]

    O. Aharony, S. S. Gubser, J. M. Maldacenaet al., Phys. Rept.323, 183-386 (2000)

  • [29]

    E. D’Hoker and D. Z. Freedman,Supersymmetric gauge theories and the AdS / CFT correspondence, in Theoretical Advanced Study Institute in Elementary Particle Physics (TASI 2001): Strings, Branes and EXTRA Dimensions, pp. 3–158, 1 2002

  • [30]

    S. A. Hartnoll, Class. Quant. Grav.26, 224002 (2009)

  • [31]

    J. McGreevy, Adv. High Energy Phys.2010, 723105 (2010)

  • [32]

    Y. Kim, I. J. Shin, and T. Tsukioka, Prog. Part. Nucl. Phys.68, 55-112 (2013)

  • [33]

    A. Adams, L. D. Carr, T. Schäferet al., New J. Phys.14, 115009 (2012)

  • [34]

    C. Vafa,The String landscape and the swampland, 9, 2005.

  • [35]

    H. Ooguri and C. Vafa, Nucl. Phys. B766, 21-33 (2007)

  • [36]

    N. Arkani-Hamed, L. Motl, A. Nicoliset al., JHEP06, 060 (2007)

  • [37]

    J. Sadeghi, B. Pourhassan, S. Noori Gashtiet al., Phys. Scripta96(12), 125317 (2021)

  • [38]

    C. Cordova, K. Ohmori, and T. Rudelius,Generalized Symmetry Breaking Scales and Weak Gravity Conjectures, 2, 2022.

  • [39]

    J. Henriksson, B. McPeak, F. Russoet al.,Bounding Violations of the Weak Gravity Conjecture, 3, 2022

  • [40]

    S. Kaya and T. Rudelius,Higher-Group Symmetries and Weak Gravity Conjecture Mixing, 2, 2022

  • [41]

    V. Collazuol, M. Graña, and A. Herráez,E9 symmetry in the Heterotic String on S1 and the Weak Gravity Conjecture, 3, 2022

  • [42]

    S. Capozziello, M. De Laurentis, S. D. Odintsovet al., Phys. Rev. D83, 064004 (2011)

  • [43]

    B. McInnes,Planar Black Holes as a Route to Understanding the Weak Gravity Conjecture, 1, 2022

  • [44]

    C. Cheung and G. N. Remmen, Phys. Rev. Lett.113, 051601 (2014)

  • [45]

    T. Rudelius,Constraints on Early Dark Energy from the Axion Weak Gravity Conjecture, 3, 2022

  • [46]

    N. Cribiori and G. Dall’Agata,Weak gravity versus scale separation, 3, 2022

  • [47]

    D. Klaewer, S.-J. Lee, T. Weigandet al., JHEP03, 252 (2021)

  • [48]

    B. Heidenreich, M. Reece, and T. Rudelius, JHEP02, 140 (2016)

  • [49]

    B. Heidenreich, M. Reece, and T. Rudelius, JHEP08, 025 (2017)

  • [50]

    S. Andriolo, D. Junghans, T. Noumiet al., Fortsch. Phys.66(5), 1800020 (2018)

  • [51]

    J. Polchinski, Int. J. Mod. Phys. A19S1, 145-156 (2004)

  • [52]

    H. Ooguri and C. Vafa, Adv. Theor. Math. Phys.21, 1787-1801 (2017)

  • [53]

    L. E. Ibanez, V. Martin-Lozano, and I. Valenzuela, JHEP11, 066 (2017)

  • [54]

    G. Shiu, P. Soler, and W. Cottrell, Sci. China Phys. Mech. Astron.62(11), 110412 (2019)

  • [55]

    Z. Fisher and C. J. Mogni,A Semiclassical, Entropic Proof of a Weak Gravity Conjecture, 6, 2017

  • [56]

    C. Cheung, J. Liu, and G. N. Remmen, JHEP10, 004 (2018)

  • [57]

    T. Crisford, G. T. Horowitz, and J. E. Santos, Phys. Rev. D97(6), 066005 (2018)

  • [58]

    D. Harlow, JHEP01, 122 (2016)

  • [59]

    Y. Hamada, T. Noumi, and G. Shiu, Phys. Rev. Lett.123(5), 051601 (2019)

  • [60]

    W. H. Kinney, S. Vagnozzi, and L. Visinelli, Class. Quant. Grav.36(11), 117001 (2019)

  • [61]

    D. Harlow, B. Heidenreich, M. Reeceet al.,The Weak Gravity Conjecture: A Review, 1, 2022

  • [62]

    P. Saraswat, Phys. Rev. D95(2), 025013 (2017)

  • [63]

    Y. Nakayama and Y. Nomura, Phys. Rev. D92(12), 126006 (2015)

  • [64]

    T. C. Bachlechner, C. Long, and L. McAllister, JHEP01, 091 (2016)

  • [65]

    B. Bellazzini, M. Lewandowski, and J. Serra, Phys. Rev. Lett.123(25), 251103 (2019)

  • [66]

    O. Aharony and E. Palti, Phys. Rev. D104(12), 126005 (2021)

  • [67]

    B. Heidenreich, M. Reece, and T. Rudelius, JHEP10, 055 (2019)

  • [68]

    K. Benakli, C. Branchina, and G. Lafforgue-Marmet, Eur. Phys. J. C80(12), 1118 (2020)

  • [69]

    S.-J. Lee, W. Lerche, and T. Weigand, Nucl. Phys. B938, 321-350 (2019)

  • [70]

    S. de Alwis, A. Eichhorn, A. Heldet al., Phys. Lett. B798, 134991 (2019)

  • [71]

    S. Andriolo, T.-C. Huang, T. Noumiet al., Phys. Rev. D, 1024, 046008 (2020)

  • [72]

    S. Cremonini, C. R. T. Jones, J. T. Liuet al., Phys. Rev. D103(10), 106011 (2021)

  • [73]

    L. E. Ibanez, M. Montero, A. Urangaet al., JHEP04, 020 (2016)

  • [74]

    A. Banerjee, H. Cai, L. Heisenberget al., Phys. Rev. D103(8), L081305 (2021)

  • [75]

    B. Heidenreich, M. Reece, and T. Rudelius, JHEP11, 004 (2021)

  • [76]

    S. Fichet and P. Saraswat, JHEP01, 088 (2020)

  • [77]

    T. Daus, A. Hebecker, S. Leonhardtet al., Nucl. Phys. B960, 115167 (2020)

  • [78]

    Y. Kats, L. Motl, and M. Padi, JHEP12, 068 (2007)

  • [79]

    M. van Beest, J. Calderón-Infante, D. Mirfendereskiet al.,Lectures on the Swampland Program in String Compactifications,2, 2021

  • [80]

    R. A. Konoplya and A. Zhidenko, Phys. Rev. D88, 024054 (2013)

  • [81]

    A. Urbano,Towards a proof of the Weak Gravity Conjecture, 10, 2018

  • [82]

    M. Alishahiha, M. R. Mohammadi Mozaffaret al., JHEP10, 003 (2012)

  • [83]

    G. T. Horowitz and V. E. Hubeny, Phys. Rev. D62, 024027 (2000)

  • [84]

    D. Birmingham, I. Sachs, and S. N. Solodukhin, Phys. Rev. Lett.88, 151301 (2002)

  • [85]

    S. Hod, Phys. Rev. D75, 064013 (2007)

  • [86]

    S. Hod, Int. J. Mod. Phys. D26(12), 1742004 (2017)

  • [87]

    S. Sachdev and J. Ye, Phys. Rev. Lett.70, 3339 (1993)

  • [88]

    J. Maldacena and D. Stanford, Phys. Rev. D94(10), 106002 (2016)

  • [89]

    A. Eberlein, V. Kasper, S. Sachdevet al., Phys. Rev. B96(20), 205123 (2017)

  • [90]

    A. Gruzinov,Kerr quasinormal modes and Hod’s time-temperature bound, 5, 2007

  • [91]

    S. Hod, Phys. Lett. A374, 2901 (2010)

  • [92]

    J. F. Pedraza, W. Sybesma, and M. R. Visser, Class. Quant. Grav.36(5), 054002 (2019)

  • [93]

    M. Alishahiha, E. O Colgain, and H. Yavartanoo, JHEP11, 137 (2012)

  • [94]

    M. M. Caldarelli, G. Cognola, and D. Klemm, Class. Quant. Grav.17, 399-420 (2000)

  • [95]

    B. Chen and J. Long, JHEP08, 065 (2010)

Baidu
map