-
[1]
B. P. Abbott et al. (LIGO Scientific and Virgo), Phys. Rev. Lett. 116(24), 241103 (2016)
-
[2]
B. P. Abbott et al. (LIGO Scientific and Virgo), Phys. Rev. Lett. 116(24), 241102 (2016)
-
[3]
B. P. Abbott et al. (LIGO Scientific and Virgo), Phys. Rev. Lett. 116(6), 061102 (2016)
-
[4]
Kazunori Akiyama et al., Astrophys. J. 875(1), L1 (2019)
-
[5]
Kazunori Akiyama et al., Astrophys. J. Lett. 875(1), L4 (2019)
-
[6]
Kazunori Akiyama et al., Astrophys. J. Lett. 875(1), L5 (2019)
-
[7]
Kazunori Akiyama et al., Astrophys. J. Lett. 875(1), L6 (2019)
-
[8]
J. L. Synge, Mon. Not. Roy. Astron. Soc. 131(3), 463-466 (1966)
-
[9]
J. M. Bardeen, in Black Holes (Proceedings, Ecole d'Et de Physique Thorique: Les Astres Occlus: Les Houches, France, August, 1972) edited by C. DeWitt and B.S. Dewitt
-
[10]
James M. Bardeen, William H. Press, and Saul A Teukolsky, Astrophys. J. 178, 347 (1972)
-
[11]
J.-P. Luminet, Astron. Astrophys. 75, 228 (1979)
-
[12]
O. Porth et al. (Event Horizon Telescope), Astrophys. J. Suppl. 243(2), 26 (2019)
-
[13]
P. V. P. Cunha, N. A. Eiró, C. A. R. Herdeiro et al., JCAP 2003(3), 035 (2020)
-
[14]
R. Narayan, M. D. Johnson, and C. F. Gammie, Astrophys. J. 885(2), L33 (2019)
-
[15]
X. X. Zeng, H. Q. Zhang, and H. Zhang, Eur. Phys. J. C 80(9), 872 (2020)
-
[16]
S. Guo, K. J. He, G. R. Li et al., Class. Quant. Grav. 38(16), 165013 (2021)
-
[17]
X. Qin, S. Chen, and J. Jing, Class. Quant. Grav. 38(11), 115008 (2021)
-
[18]
S. E. Gralla, D. E. Holz, and R. M. Wald, Phys. Rev. D 100(2), 024018 (2019)
-
[19]
J. Peng, M. Guo, and X. H. Feng, Chin. Phys. C 45(8), 085103 (2021)
-
[20]
J. Peng, M. Guo, and X. H. Feng, Phys. Rev. D 104(12), 124010 (2021)
-
[21]
S. E. Gralla and A. Lupsasca, Phys. Rev. D 101(4), 044031 (2020)
-
[22]
X. X. Zeng and H. Q. Zhang, Eur. Phys. J. C 80(11), 1058 (2020)
-
[23]
K. J. He, S. C. Tan, and G. P. Li, Eur. Phys. J. C 82(1), 81 (2022)
-
[24]
Q. Gan, P. Wang, H. Wu et al., Phys. Rev. D 104(4), 044049 (2021)
-
[25]
M. Guerrero, G. J. Olmo, D. Rubiera-Garcia et al., JCAP 08, 036 (2021)
-
[26]
K. J. He, S. Guo, S. C. Tan et al., The feature of shadow images and observed luminosity of the Bardeen black hole surrounded by different accretions, arXiv: 2103.13664 [hep-th]
-
[27]
C. Bambi, K. Freese, S. Vagnozzi et al., Phys. Rev. D 100(4), 044057 (2019)
-
[28]
S. X. Tian and Z. H. Zhu, Phys. Rev. D 100(6), 064011 (2019)
-
[29]
S. Vagnozzi and L. Visinelli, Phys. Rev. D 100(2), 024020 (2019)
-
[30]
A. B. Abdikamalov, A. A. Abdujabbarov, D. Ayzenberg et al., Phys. Rev. D 100(2), 024014 (2019)
-
[31]
D. Psaltis, Gen. Rel. Grav. 51(10), 137 (2019)
-
[32]
K. Glampedakis and G. Pappas, Phys. Rev. D 99(12), 124041 (2019)
-
[33]
R. Roy and S. Chakrabarti, Phys. Rev. D 102(2), 024059 (2020)
-
[34]
Z. Zhong, Z. Hu, H. Yan et al., Phys. Rev. D 104(10), 104028 (2021)
-
[35]
P. C. Li, M. Guo, and B. Chen, Phys. Rev. D 101(8), 084041 (2020)
-
[36]
X. X. Zeng, K. J. He, and G. P. Li, Influence of dark matter on shadows and rings of a brane-world black hole illuminated by various accretions, arXiv: 2111.05090 [gr-qc].
-
[37]
P. V. P. Cunha, C. A. R. Herdeiro, B. Kleihaus et al., Phys. Lett. B 768, 373-379 (2017)
-
[38]
A. Allahyari, M. Khodadi, S. Vagnozzi et al., JCAP 02, 003 (2020)
-
[39]
J. W. Moffat and V. T. Toth, Phys. Rev. D 101(2), 024014 (2020)
-
[40]
G. P. Li and K. J. He, JCAP 06, 037 (2021)
-
[41]
X. X. Zeng, G. P. Li, and K. J. He, Nucl. Phys. B 974, 115639 (2022)
-
[42]
G. P. Li and K. J. He, Eur. Phys. J. C 81(11), 1018 (2021)
-
[43]
Z. Hu, Z. Zhong, P. C. Li et al., Phys. Rev. D 103(4), 044057 (2021)
-
[44]
D. Langlois, Prog. Theor. Phys. Suppl. 148, 181 (2002)
-
[45]
N. Arkani-Hamed, S. Dimopoulos, and G. R. Dvali, Phys. Lett. B 429, 263-272 (1998)
-
[46]
I. Antoniadis, N. Arkani-Hamed, S. Dimopoulos et al., Phys. Lett. B 436, 257-263 (1998)
-
[47]
G. Aad et al. (ATLAS), Phys. Lett. B 716, 1-29 (2012)
-
[48]
S. Chatrchyan et al. (CMS), Phys. Lett. B 716, 30-61 (2012)
-
[49]
L. Randall and R. Sundrum, Phys. Rev. Lett. 83, 3370-3373 (1999)
-
[50]
L. Randall and R. Sundrum, Phys. Rev. Lett. 83, 4690-4693 (1999)
-
[51]
T. Harko and M. K. Mak, Phys. Rev. D 69, 064020 (2004)
-
[52]
S. Chakraborty and S. SenGupta, Class. Quant. Grav. 33(22), 225001 (2016)
-
[53]
A. Chamblin, S. W. Hawking, and H. S. Reall, Phys. Rev. D 61, 065007 (2000)
-
[54]
A. Chamblin, H. S. Reall, H. a. Shinkai et al., Phys. Rev. D 63, 064015 (2001)
-
[55]
R. Emparan, G. T. Horowitz, and R. C. Myers, JHEP 01, 007 (2000)
-
[56]
U. Papnoi, F. Atamurotov, S. G. Ghosh et al., Phys. Rev. D 90(2), 024073 (2014)
-
[57]
A. Abdujabbarov, F. Atamurotov, N. Dadhich et al., Eur. Phys. J. C 75(8), 399 (2015)
-
[58]
B. P. Singh and S. G. Ghosh, Annals Phys. 395, 127-137 (2018)
-
[59]
N. Dadhich, R. Maartens, P. Papadopoulos et al., Phys. Lett. B 487, 1-6 (2000)
-
[60]
C. G. Boehmer, T. Harko, and F. S. N. Lobo, Class. Quant. Grav. 25, 045015 (2008)
-
[61]
A. Kotrlova, Z. Stuchlik, and G. Torok, Class. Quant. Grav. 25, 225016 (2008)
-
[62]
Z. Horvath and L. A. Gergely, Astron. Nachr. 334, 1047-1050 (2013)
-
[63]
A. F. Zakharov, Eur. Phys. J. C 78(8), 689 (2018)
-
[64]
J. C. S. Neves, Eur. Phys. J. C 80(8), 717 (2020)
-
[65]
L. Amarilla and E. F. Eiroa, Phys. Rev. D 85, 064019 (2012)
-
[66]
Y. Hou, M. Guo, and B. Chen, Phys. Rev. D 104(2), 024001 (2021)
-
[67]
C. Molina, A. B. Pavan, and T. E. Medina Torrejón, Phys. Rev. D 93(12), 124068 (2016)
-
[68]
C. Molina, Phys. Rev. D 88, 127501 (2013)
-
[69]
C. Molina and J. C. S. Neves, Phys. Rev. D 82, 044029 (2010)
-
[70]
T. Shiromizu, K. i. Maeda, and M. Sasaki, Phys. Rev. D 62, 024012 (2000)
-
[71]
A. N. Aliev and A. E. Gumrukcuoglu, Phys. Rev. D 71, 104027 (2005)
-
[72]
A. N. Aliev and P. Talazan, Phys. Rev. D 80, 044023 (2009)
-
[73]
J. C. S. Neves and C. Molina, Phys. Rev. D 86, 124047 (2012)
-
[74]
C. Bambi, Phys. Rev. D 87, 107501 (2013)
-
[75]
M. Jaroszynski and A. Kurpiewski, Astron. Astrophys. 326, 419 (1997)