The red-shift effect and radiation decay on black hole spacetimes

2009 ◽  
Vol 62 (7) ◽  
pp. 859-919 ◽  
Author(s):  
Mihalis Dafermos ◽  
Igor Rodnianski
Keyword(s):  
Black Hole ◽  
Red Shift ◽  
Black Hole Spacetimes ◽  
Shift Effect ◽  
Radiation Decay

scholarly journals HIRE: Hidden Inter-packet Red-shift Effect

2020 ◽  
Author(s):  
Francesco Ciaccia ◽  
Ivan Romero ◽  
Rene Serral-Gracia ◽  
Mario Nemirovsky
Keyword(s):  
Red Shift ◽  
Shift Effect

scholarly journals Stable circular orbits in caged black hole spacetimes

2021 ◽  
Vol 103 (8) ◽  
Author(s):  
Takahisa Igata ◽  
Shinya Tomizawa
Keyword(s):  
Black Hole ◽  
Circular Orbits ◽  
Black Hole Spacetimes

scholarly journals Master equations and quasinormal modes of spin- 3/2 fields in Schwarzschild (A)dS black hole spacetimes

2019 ◽  
Vol 100 (10) ◽  
Author(s):  
Chun-Hung Chen ◽  
Hing-Tong Cho ◽  
Alan S. Cornell ◽  
Gerhard E. Harmsen
Keyword(s):  
Black Hole ◽  
Quasinormal Modes ◽  
Master Equations ◽  
Black Hole Spacetimes

scholarly journals Efficient asymptotic frame selection for binary black hole spacetimes using asymptotic radiation

2011 ◽  
Vol 84 (12) ◽  
Author(s):  
R. O’Shaughnessy ◽  
B. Vaishnav ◽  
J. Healy ◽  
Z. Meeks ◽  
D. Shoemaker
Keyword(s):  
Black Hole ◽  
Frame Selection ◽  
Black Hole Spacetimes ◽  
Binary Black Hole ◽  
Selection For

scholarly journals Non-conservation of Carter in black hole spacetimes

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

scholarly journals Fermat’s principle in black-hole spacetimes

2018 ◽  
Vol 27 (14) ◽  
pp. 1847025 ◽  
Author(s):  
Shahar Hod
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Black Hole Spacetimes ◽  
Fermat’S Principle ◽  
Kerr Black Holes ◽  
Fermat's Principle ◽  
Asymptotic Observers

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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