A Slowly Rotating Black Hole in Horava-Lifshitz Gravity and a 3+1 Dimensional Topological Black Hole: Motion of Particles and BSW Mechanism
arXiv:1412.1112 · doi:10.1007/s10773-014-2355-7
Abstract
The motion of a neutral particle in the vicinity of a slowly rotating black hole in the Horava-Lifshitz theory of gravity and 3+1 dimensional topological Lifshitz black hole is investigated. Geodesics for radial motion of the particles are also plotted. Some different cases of the orbital motion of the particle are discussed where maximum and minimum values of the effective potential are calculated. Further the Bañados, Silk and West (BSW) mechanism is studied for these black holes. It is shown that the centre-of-mass energy (CME) of two colliding uncharged particles at the horizon of these black holes remains finite. Thus the BSW effect cannot be seen in these cases.
14 pages, 2 figures, published in IJTP
References in corpus (16)
- Quantum Gravity at a Lifshitz Point
- Solutions to Horava Gravity
- Black holes in Einstein-aether and Horava-Lifshitz gravity
- Thermodynamics of Black Holes in Horava-Lifshitz Gravity
- Circular motion of neutral test particles in Reissner-Nordström spacetime
- Charged Spinning Black Holes as Particle Accelerators
- Acceleration of particles by nonrotating charged black holes
- Slowly rotating black holes in Horava-Lifshitz gravity
- Particle Motion around Black Hole in Horava-Lifshitz Gravity
- Particle Collisions on Stringy Black Hole Background
- A no-go theorem for slowly rotating black holes in Horava-Lifshitz gravity
- Particle Motion and Scalar Field Propagation in Myers-Perry Black Hole Spacetimes in All Dimensions
- Spacing of the entropy spectrum for KS Black hole in Horava-Lifshitz gravity
- Slowly rotating black holes in the Horava-Lifshitz gravity
- Holographic superconductors in a model of non-relativistic gravity
- Non-monotonic Keplerian velocity profiles around near-extreme braneworld Kerr black holes
Cited by in corpus (4)
- Center of Mass Energy of the Collision for Two General Geodesic Particles Around a Kerr-Newman-Taub-NUT Black Hole
- Dynamics and center of mass energy of colliding particles around black hole in f(R) gravity
- Schwarzschild black hole surrounded by quintessential matter field as an accelerator for spinning particles
- Orbital motion of test particles in regular Hayward black hole space-time