Add to ORKGIn this contribution, the motion of unitary mass test particles in a perturbed Kerr-like metric is studied using simulations in the configuration and phase space. Our metric represents the approximate exterior spacetime of a massive rotating body with mass quadrupole moment $q$. Chaotic behavior arises as the $q$ parameter increases. The rotation number is determined for an axis of symmetry in the corresponding Poincar\'e section. The existence of chaotic regions in the region near the source event horizon is shown.Comment: 30 pages, 32 figure
In this article, we explore the geodesics motion of neutral test particles and the process of energy...
We investigate the long-term orbital dynamics of spinless extended bodies in Schwarzschild geometry,...
The exact solution to the Einstein equations that represents a static axially symmetric source defor...
We study chaos dynamics of spinning particles in Kerr spacetime of rotating black holes use the Papa...
We investigate the dynamics of the Papapetrou equations in Kerr spacetime. These equations provide a...
While recent gravitational wave observations by LIGO and Virgo allow for tests of general relativity...
We analyze the motion of a massless and chargeless particle very near to the event horizon. It revea...
This work studies the dynamics of geodesic motion within a curved spacetime around a Schwarzschild b...
This paper builds up the necessary physical groundwork and motivates the derivation of the weak-fiel...
We investigate the dynamics of relativistic spinning test particles in the spacetime of a rotating b...
We introduce an action-angle formalism for bounded geodesic motion in Kerr black hole spacetime usin...
This paper builds up the necessary physical groundwork and motivates the derivation of the weak-fiel...
The motion of a test particle in the Schwarzschild background models the merger of a compact object ...
The Johannsen-Psaltis spacetime is a perturbation of the Kerr spacetime designed to avoid pathologie...
A recent work by Dubeibe et al. [Phys. Rev. D 75, 023008 (2007)] stated that chaos phenomenon of tes...
In this article, we explore the geodesics motion of neutral test particles and the process of energy...
We investigate the long-term orbital dynamics of spinless extended bodies in Schwarzschild geometry,...
The exact solution to the Einstein equations that represents a static axially symmetric source defor...
We study chaos dynamics of spinning particles in Kerr spacetime of rotating black holes use the Papa...
We investigate the dynamics of the Papapetrou equations in Kerr spacetime. These equations provide a...
While recent gravitational wave observations by LIGO and Virgo allow for tests of general relativity...
We analyze the motion of a massless and chargeless particle very near to the event horizon. It revea...
This work studies the dynamics of geodesic motion within a curved spacetime around a Schwarzschild b...
This paper builds up the necessary physical groundwork and motivates the derivation of the weak-fiel...
We investigate the dynamics of relativistic spinning test particles in the spacetime of a rotating b...
We introduce an action-angle formalism for bounded geodesic motion in Kerr black hole spacetime usin...
This paper builds up the necessary physical groundwork and motivates the derivation of the weak-fiel...
The motion of a test particle in the Schwarzschild background models the merger of a compact object ...
The Johannsen-Psaltis spacetime is a perturbation of the Kerr spacetime designed to avoid pathologie...
A recent work by Dubeibe et al. [Phys. Rev. D 75, 023008 (2007)] stated that chaos phenomenon of tes...
In this article, we explore the geodesics motion of neutral test particles and the process of energy...
We investigate the long-term orbital dynamics of spinless extended bodies in Schwarzschild geometry,...
The exact solution to the Einstein equations that represents a static axially symmetric source defor...