Add to ORKGIt is demonstrated that, in the adiabatic approximation, nonequatorial circular orbits of particles in the Kerr metric (i.e., orbits of constant Boyer-Lindquist radius) remain circular under the influence of gravitational radiation reaction. A brief discussion is given of conditions for breakdown of adiabaticity and of whether slightly noncircular orbits are stable against the growth of eccentricity
In an extreme binary black hole system, an orbit will increase its angle of inclination (ι) as it ev...
In an extreme mass-ratio binary black hole system, a non-equatorial orbit will list (i.e. increase i...
We present two methods for integrating forced geodesic equations in the Kerr spacetime. The methods ...
It is demonstrated that, in the adiabatic approximation, non-Equatorial circular orbits of particles...
The effect of gravitational radiation reaction on orbits around a spinning black hole is analyzed. S...
We use the Teukolsky perturbation formalism to show that (i) a particle in circular motion around a ...
A major focus of much current research in gravitation theory is on understanding how radiation react...
We study eccentric equatorial orbits of a test-body around a Kerr black hole under the influence of ...
We study eccentric equatorial orbits of a test-body around a Kerr black hole under the influence of ...
We have performed a detailed analysis of orbital motion in the vicinity of a nearly extremal Kerr bl...
We have performed a detailed analysis of orbital motion in the vicinity of a nearly extremal Kerr bl...
We have performed a detailed analysis of orbital motion in the vicinity of a nearly extremal Kerr bl...
We present exact solutions of test particle orbits spiralling inward from the innermost stable circu...
We analyze the properties of circular orbits of test particles on the equatorial plane of a rotating...
General orbits of a particle of small mass $\mu$ around a Kerr black hole of mass $M$ are characteri...
In an extreme binary black hole system, an orbit will increase its angle of inclination (ι) as it ev...
In an extreme mass-ratio binary black hole system, a non-equatorial orbit will list (i.e. increase i...
We present two methods for integrating forced geodesic equations in the Kerr spacetime. The methods ...
It is demonstrated that, in the adiabatic approximation, non-Equatorial circular orbits of particles...
The effect of gravitational radiation reaction on orbits around a spinning black hole is analyzed. S...
We use the Teukolsky perturbation formalism to show that (i) a particle in circular motion around a ...
A major focus of much current research in gravitation theory is on understanding how radiation react...
We study eccentric equatorial orbits of a test-body around a Kerr black hole under the influence of ...
We study eccentric equatorial orbits of a test-body around a Kerr black hole under the influence of ...
We have performed a detailed analysis of orbital motion in the vicinity of a nearly extremal Kerr bl...
We have performed a detailed analysis of orbital motion in the vicinity of a nearly extremal Kerr bl...
We have performed a detailed analysis of orbital motion in the vicinity of a nearly extremal Kerr bl...
We present exact solutions of test particle orbits spiralling inward from the innermost stable circu...
We analyze the properties of circular orbits of test particles on the equatorial plane of a rotating...
General orbits of a particle of small mass $\mu$ around a Kerr black hole of mass $M$ are characteri...
In an extreme binary black hole system, an orbit will increase its angle of inclination (ι) as it ev...
In an extreme mass-ratio binary black hole system, a non-equatorial orbit will list (i.e. increase i...
We present two methods for integrating forced geodesic equations in the Kerr spacetime. The methods ...