scholarly journals On the Gravitational Wave and Force Propagation Speed Impact on the GEM Decay of Circular Orbits

OALib ◽  
2020 ◽  
Vol 07 (08) ◽  
pp. 1-19
Author(s):  
Barbaro Quintero-Leyva
Keyword(s):  
Gravitational Wave ◽  
Propagation Speed ◽  
Circular Orbits ◽  
Force Propagation

The 2.5PN gravitational wave polarizations from inspiralling compact binaries in circular orbits

2005 ◽  
Vol 22 (14) ◽  
pp. 3115-3117 ◽  
Author(s):  
K G Arun ◽  
L Blanchet ◽  
B R Iyer ◽  
M S S Qusailah
Keyword(s):  
Gravitational Wave ◽  
Circular Orbits ◽  
Compact Binaries

scholarly journals The 2.5PN gravitational wave polarizations from inspiralling compact binaries in circular orbits

2004 ◽  
Vol 21 (15) ◽  
pp. 3771-3801 ◽  
Author(s):  
K G Arun ◽  
Luc Blanchet ◽  
Bala R Iyer ◽  
Moh'd S S Qusailah
Keyword(s):  
Gravitational Wave ◽  
Circular Orbits ◽  
Compact Binaries

Force propagation speed in a bed of particles due to an incident particle impact

2010 ◽  
Vol 21 (2) ◽  
pp. 150-164 ◽  
Author(s):  
M.S. Abd-Elhady ◽  
S. Abd-Elhady ◽  
C.C.M. Rindt ◽  
A.A. van Steenhoven
Keyword(s):  
Propagation Speed ◽  
Incident Particle ◽  
Particle Impact ◽  
Force Propagation

scholarly journals Qualifying ringdown and shadow of black holes under general parametrized metrics with photon orbits

2021 ◽  
Vol 81 (7) ◽  
Author(s):  
Song Li ◽  
Ahmadjon A. Abdujabbarov ◽  
Wen-Biao Han
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Lyapunov Exponent ◽  
Gravitational Wave ◽  
Decay Rate ◽  
Event Horizon ◽  
Equatorial Plane ◽  
Circular Orbits ◽  
The Future

AbstractThe motion of photons around black holes determines the shape of shadow and match the ringdown properties of a perturbed black hole. Observations of shadows and ringdown waveforms will reveal the nature of black holes. In this paper, we study the motion of photons in a general parametrized metric beyond the Kerr hypothesis. We investigated the radius and frequency of the photon circular orbits on the equatorial plane and obtained fitted formula with varied parameters. The Lyapunov exponent which connects to the decay rate of the ringdown amplitude is also calculated. We also analyzed the shape of shadow with full parameters of the generally axisymmetric metric. Our results imply the potential constraint on black hole parameters by combining the Event Horizon Telescope and gravitational wave observations in the future.

Sign in / Sign up

Export Citation Format

Share Document