On the perturbation solutions to the Blandford-Znajek mechanism in the Kerr-Sen black hole

[1]
R. P. Fender, T. M. Belloni, and E. Gallo, Mon. Not. Roy. Astron. Soc. 355, 1105 (2004)
[2]
T. M. Belloni and S. E. Motta. Transient Black Hole Binaries, (Springer Berlin Heidelberg, 2016), p. 61.
[3]
R. D. Blandford and R. L. Znajek, Mon. Not. Roy. Astron. Soc. 179, 433 (1977)
[4]
H. K. Lee, R. A. M. J. Wijers, and G. E. Brown, Phys. Rept. 325, 83 (2000)
[5]
A. Gruzinov, Phys. Rev. Lett. 94, 021101 (2005)
[6]
D. A. Uzdensky, Astrophys. J. 603, 652 (2004)
[7]
D. A. Uzdensky, Astrophys. J. 620, 889 (2005)
[8]
J. Ogura and Y. Kojima, Prog. Theor. Phys. 109, 619 (2003)
[9]
I. Contopoulos, D. Kazanas, and C. Fendt, Astrophys. J. 511, 351 (1999)
[10]
J. C. McKinney and C. F. Gammie, Astrophys. J. 611, 977 (2004)
[11]
J. C. McKinney, Astrophys. J. Lett. 630, L5 (2005)
[12]
S. S. Komissarov, Direct numerical simulations of the blandford–znajek effect. 13th Rencontres de Blois on Frontiers of the Universe, 2004.
[13]
S. S. Komissarov, Mon. Not. Roy. Astron. Soc. 350, 407 (2004)
[14]
G. C. Pei, S. Nampalliwar, C. Bambi et al., Eur. Phys. J. C 76(10), 534 (2016)
[15]
R. Penrose, Phys. Rev. Lett. 14, 57 (1965)
[16]
S. W. Hawking, Phys. Rev. D 14, 2460 (1976)
[17]
D. Christodoulou, Commun. Pure Appl. Math. 44(3), 339 (1991)
[18]
C. M. Will, Living Rev. Rel. 17, 4 (2014)
[19]
M. Milgrom, Astrophys. J. 270, 371 (1983)
[20]
J. Bekenstein and M. Milgrom, Astrophys. J. 286, 7 (1984)
[21]
M. Milgrom and R. H. Sanders, Astrophys. J. Lett. 599, L25 (2003)
[22]
A. G. Riess et al. (Supernova Search Team), Astron. J. 116, 1009 (1998)
[23]
T. Clifton, P. G. Ferreira, A. Padilla et al., Phys. Rept. 513, 1 (2012)
[24]
M. Rogatko, Class. Quant. Grav. 19, 5063 (2002)
[25]
A. Sen, Phys. Rev. Lett. 69, 1006 (1992)
[26]
R. Catena and J. Moller, JCAP 03, 012 (2008)
[27]
J. Sonner and P. K. Townsend, Phys. Rev. D 74, 103508 (2006)
[28]
I. Banerjee, B. Mandal, and S. SenGupta, Mon. Not. Roy. Astron. Soc. 500(1), 481 (2020)
[29]
S. K. Sahoo, N. Yadav, and I. Banerjee, Phys. Rev. D 109(4), 044008 (2024)
[30]
B. A. Campbell, N. Kaloper, R. Madden et al., Nucl. Phys. B 399, 137 (1993)
[31]
C. Ganguly and S. SenGupta, Eur. Phys. J. C 76(4), 213 (2016)
[32]
D. Garfinkle, G. T. Horowitz, and A. Strominger, Phys. Rev. D 43, 3140 (1991) [Erratum: Phys. Rev. D 45, 3888 (1992)]
[33]
Z. Pan and C. Yu, arXiv: 1406.4936
[34]
Z. Pan and C. Yu. Highly-collimated, magnetically-dominated jets around rotating black holes, (2014)
[35]
I. Contopoulos, D. Kazanas, and D. B. Papadopoulos, Astrophys. J. 765, 113 (2013)
[36]
J. A. Petterson, Phys. Rev. D 10, 3166 (1974)
[37]
R. L. Znajek, Mon. Not. Roy. Astron. Soc. 179(3), 457 (1977)
[38]
Z. Pan and C. Yu, Phys. Rev. D 91(6), 064067 (2015)
[39]
I. D. Novikov and K. S. Thorne. Astrophysics and black holes, in Les Houches Summer School of Theoretical Physics: Black Holes, (1973), p. 343
[40]
H. Y. Feng, Y. D. Wu, R. J. Yang et al., Phys. Rev. D 109(6), 063014 (2024)
[41]
M. Ruiz, C. Palenzuela, F. Galeazzi et al., Mon. Not. Roy. Astron. Soc. 423, 1300 (2012)
[42]
K. Toma and F. Takahara, Mon. Not. Roy. Astron. Soc. 442(4), 2855 (2014)
[43]
R. Narayan and J. E. McClintock, Mon. Not. Roy. Astron. Soc. 419, L69 (2012)
[44]
J. F. Steiner, J. E. McClintock, and R. Narayan, Astrophys. J. 762(2), 104 (2012)
[45]
Z. H. Chen, L. J. Gou, J. E. McClintock, Astrophys. J. 825(1), 45 (2016)
[46]
R. Fender. Jets from X-ray binaries. Compact stellar X-ray sources, (Cambridge: Cambridge University Press, 2006), p. 381
[47]
M. Middleton, J. Miller-Jones, and R. Fender, Mon. Not. Roy. Astron. Soc. 439(2), 1740 (2014)
[48]
I. Banerjee, B. Mandal, and S. SenGupta, Phys. Rev. D 103, 044046 (2021)