We present exact solutions of test particle orbits spiralling inward from the innermost stable circular orbit (ISCO) of a Kerr black hole. Our results are valid for any allowed value of the angular momentum $a$-parameter of the Kerr metric. These solutions are of considerable physical interest. In particular, the radial 4-velocity of these orbits is both remarkably simple and, with the radial coordinate scaled by its ISCO value, universal in form, otherwise completely independent of the black hole spin.Comment: Accepted for publication in Physical Review Letters. 5 pages 3 figure
As a consequence of Birkhoff's theorem, the exterior gravitational field of a spherically symmetric ...
It is demonstrated that, in the adiabatic approximation, nonequatorial circular orbits of particles ...
Abstract ? Bound geodesic orbits around a Kerr black hole can be parametrized by three constants of ...
We present exact solutions of test particle orbits spiraling inward from the innermost stable circul...
The innermost stable circular orbit (ISCO) delimits the transition from circular orbits to those tha...
The innermost stable circular orbit (ISCO) delimits the transition from circular orbits to those tha...
We have performed a detailed analysis of orbital motion in the vicinity of a nearly extremal Kerr bl...
In this paper, we study rotating horizon less black shells as an alternative to Kerr black holes. We...
International audienceIn a recent work [Phys. Rev. D 94, 104010 (2016)PRVDAQ2470-001010.1103/PhysRev...
In this article, we explore the geodesics motion of neutral test particles and the process of energy...
In this paper, we continue our study of the motion of spinning test bodies orbiting Kerr black holes...
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 analyze the properties of circular orbits of test particles on the equatorial plane of a rotating...
The worldline of a spinning test body moving in curved spacetime can be provided by the Mathisson-Pa...
As a consequence of Birkhoff's theorem, the exterior gravitational field of a spherically symmetric ...
It is demonstrated that, in the adiabatic approximation, nonequatorial circular orbits of particles ...
Abstract ? Bound geodesic orbits around a Kerr black hole can be parametrized by three constants of ...
We present exact solutions of test particle orbits spiraling inward from the innermost stable circul...
The innermost stable circular orbit (ISCO) delimits the transition from circular orbits to those tha...
The innermost stable circular orbit (ISCO) delimits the transition from circular orbits to those tha...
We have performed a detailed analysis of orbital motion in the vicinity of a nearly extremal Kerr bl...
In this paper, we study rotating horizon less black shells as an alternative to Kerr black holes. We...
International audienceIn a recent work [Phys. Rev. D 94, 104010 (2016)PRVDAQ2470-001010.1103/PhysRev...
In this article, we explore the geodesics motion of neutral test particles and the process of energy...
In this paper, we continue our study of the motion of spinning test bodies orbiting Kerr black holes...
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 analyze the properties of circular orbits of test particles on the equatorial plane of a rotating...
The worldline of a spinning test body moving in curved spacetime can be provided by the Mathisson-Pa...
As a consequence of Birkhoff's theorem, the exterior gravitational field of a spherically symmetric ...
It is demonstrated that, in the adiabatic approximation, nonequatorial circular orbits of particles ...
Abstract ? Bound geodesic orbits around a Kerr black hole can be parametrized by three constants of ...