Circular geodesics in a New Generalization of q-metric
arXiv:2010.15723 · doi:10.3390/universe8030195
Abstract
This paper introduces an alternative generalization of the static solution with quadrupole moment, the -metric, that describes a deformed compact object in the presence of the external fields characterized by multipole moments. In addition, we also examine the impact of the external fields up to quadrupole on the circular geodesics and the interplay of these two quadrupoles on the place of the innermost stable circular orbit (ISCO) in the equatorial plane.
References in corpus (12)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Millisecond Oscillations in X-Ray Binaries
- A review of quasi-periodic oscillations from black hole X-ray binaries: observation and theory
- Black hole mimickers: regular versus singular behavior
- Geometrically Thin Disk Accreting Into a Black Hole
- The upper kHz QPO: a gravitationally lensed vertical oscillation
- Motion of test particles in the field of a naked singularity
- Mass Quadrupole as a Source of Naked Singularities
- A model for a dark matter core at the galactic center
- Retarded coordinates based at a world line, and the motion of a small black hole in an external universe
- Exterior and interior metrics with quadrupole moment
- Magnetized tori in the background of a deformed compact object
Cited by in corpus (6)
- Dynamics of charged particles and quasi-periodic oscillations in the vicinity of a distorted, deformed compact object embedded in a uniform magnetic field
- The space-time line element for static ellipsoidal objects
- Shadow of quadrupole-deformed compact objects in a local dark matter shell
- Relativistic equilibrium fluid configurations around rotating deformed compact objects
- Oscillation properties of relativistic tori in the vicinity of a distorted deformed compact object
- Vacuum polarization effects in the background of a deformed compact object and implications for photon velocity