Perfect fluid tori orbiting Kehagias-Sfetsos naked singularities
arXiv:1412.4149 · doi:10.1140/epjc/s10052-015-3663-7
Abstract
We construct perfect fluid tori in the field of the Kehagias-Sfetsos (K-S) naked singularity representing spherically symmetric vacuum solution of the modified Hořava quantum gravity that is characterized by a dimensionless parameter , combining the gravitational mass parameter of the spacetime with the Hořava parameter reflecting the role of the quantum corrections. In dependence on the value of , the K-S naked singularities demonstrate a variety of qualitatively different behavior of their circular geodesics that is fully reflected in the properties of the toroidal structures. In all of the K-S naked singularity spacetimes the tori are located above an "antigravity" sphere where matter can stay in stable equilibrium position, that is relevant for the stability of the orbiting fluid toroidal accretion structures.
44 pages, 27 figures multi panels
References in corpus (22)
- Quantum Gravity at a Lifshitz Point
- Spectral Dimension of the Universe in Quantum Gravity at a Lifshitz Point
- The Black Hole and Cosmological Solutions in IR modified Horava Gravity
- Circular motion of neutral test particles in Reissner-Nordström spacetime
- Lifshitz Gravity for Lifshitz Holography
- Influence of the relict cosmological constant on accretion discs
- Slowly rotating black holes in Horava-Lifshitz gravity
- Particle Motion around Black Hole in Horava-Lifshitz Gravity
- Quasiperiodic oscillations in a strong gravitational field around neutron stars testing braneworld models
- Gravitational lensing by massless braneworld black holes
- Spherical Boson Stars as Black Hole mimickers
- Thin accretion disk signatures of slowly rotating black holes in Hořava gravity
- Circular geodesics of naked singularities in the Kehagias-Sfetsos metric of Hořava's gravity
- Optical effects related to Keplerian discs orbiting Kehagias-Sfetsos naked singularities
- A no-go theorem for slowly rotating black holes in Horava-Lifshitz gravity
- Slowly rotating black holes in the Horava-Lifshitz gravity
- Charged tori in spherical gravitational and dipolar magnetic fields
- Solar system constraints on asymptotically flat IR modified Horava gravity through light deflection
- Charged Annular Disks and Reissner-Nordström Type Black Holes from Extremal Dust
- Quantum Interference Effects in Horava-Lifshitz Gravity
- Local thermodynamics of KS black hole
- Weak and strong field approximations and circular orbits of Kehagias-Sfetsos space-time
Cited by in corpus (13)
- Iron K line of boson stars
- Ringed accretion disks: instabilities
- Distinguishing Brans-Dicke-Kerr type naked singularities and black holes with their thin disk electromagnetic radiation properties
- Observers in Kerr spacetimes: the ergoregion on the equatorial plane
- Gravitational lensing around Kehagias-Sfetsos compact objects surrounded by plasma
- Influence of toroidal magnetic field in multi-accreting tori
- Equilibrium non-selfgravitating tori around black holes in parameterised spherically symmetric spacetimes
- Magnetized Thick Disks around Boson Stars
- Repulsive gravity effects in horizon formation. Horizon remnants in naked singularities
- Conservative limits on the electric charge of Sgr A* in the Reissner-Nordstrom metric
- Strong gravitational lensing around Kehagias-Sfetsos compact objects surrounded by plasma
- Evolution of Braneworld Kerr-Newman Naked Singularities
- Polish Doughnuts around Scalarized Kerr Black Holes