Extended bodies with structure up to the quadrupole in black hole spacetimes

Author(s):  
Donato Bini ◽  
Andrea Geralico
2021 ◽  
Vol 103 (8) ◽  
Author(s):  
Takahisa Igata ◽  
Shinya Tomizawa

2019 ◽  
Vol 100 (10) ◽  
Author(s):  
Chun-Hung Chen ◽  
Hing-Tong Cho ◽  
Alan S. Cornell ◽  
Gerhard E. Harmsen

2011 ◽  
Vol 84 (12) ◽  
Author(s):  
R. O’Shaughnessy ◽  
B. Vaishnav ◽  
J. Healy ◽  
Z. Meeks ◽  
D. Shoemaker

2015 ◽  
Vol 32 (15) ◽  
pp. 157001 ◽  
Author(s):  
Alexander Grant ◽  
Éanna É Flanagan

2018 ◽  
Vol 27 (14) ◽  
pp. 1847025 ◽  
Author(s):  
Shahar Hod

Black-hole spacetimes are known to possess closed light rings. We here present a remarkably compact theorem which reveals the physically intriguing fact that these unique null circular geodesics provide the fastest way, as measured by asymptotic observers, to circle around spinning Kerr black holes.


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