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Motion and high energy collision of magnetized particles around a Hořava-Lifshitz black hole

Ahmadjon Abdujabbarov
- Vol. 41
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TLDR
In this article, the authors studied the orbits of magnetized particles around Hořava-Lifshitz black hole with mass M$M$ immersed in an asymptotically uniform magnetic field in the infrared approximation when ωM2≫1$\omega M^{2}\gg 1$.
Abstract
We have studied the orbits of magnetized particles around Hořava-Lifshitz black hole with mass M$M$ immersed in an asymptotically uniform magnetic field in the infrared approximation when ωM2≫1$\omega M^{2}\gg 1$. It is shown that magnetized particle’s orbit in Hořava-Lifshitz spacetime is different with compare to one in Schwarzschild spacetime due to the presence of additional terms related to the Kehagias-Sfetsos (KS) parameter ω$\omega$. Using the Hamilton-Jacobi formalism, we have found the dependence of the area of stable circular orbits of the magnetized particle on dimensionless KS parameter ω˜$\tilde{\omega}$ and have plotted them for several values of magnetic coupling parameter β$\beta$ as well as obtained the equations of motion of the magnetized particle. Moreover, we have studied the dependence of the collision of (magnetized, charged, non-charged) particles on KS parameter ω$\omega$ for some fixed values of the magnetic coupling parameter β$\beta$.

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Citations
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Dynamics of test particles around a Bardeen black hole surrounded by perfect fluid dark matter

TL;DR: In this paper, the authors studied the dynamics of neutral test particles, magnetically charged test particles and test magnetic dipole around a regular Bardeen black hole surrounded by perfect fluid dark matter (PFDM).
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Dynamics of magnetized particles around 4-D Einstein Gauss–Bonnet black hole

TL;DR: In this article, the dynamics of magnetized particles around 4-D Einstein Gauss-Bonnet black hole immersed in an external asymptotically uniform magnetic field was investigated, and it was shown that the magnetic interaction parameter responsible for circular orbits decreases for negative values of the Gauss−Bonnet parameter α and the range where magnetized particle's stable circular orbits are allowed increases for the positive values of α.
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Charged particle motion and electromagnetic field in γ spacetime

TL;DR: In this article, the authors consider the electromagnetic field occurring in the background of a static, axially symmetric vacuum solution of Einstein's field equations immersed in an external magnetic field and study the motion of charged and uncharged particles in this spacetime and particle collision in the vicinity of the singular surface.
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Magnetized particle motion around non-Schwarzschild black hole immersed in an external uniform magnetic field

TL;DR: In this paper, a magnetized particle orbiting around a non-Schwarzschild black hole immersed in an external uniform magnetic field is considered and the influence of deformation parameter $h$ on the effective potential of the radial motion of the magnetized particles around the black hole using Hamilton-Jacobi formalism is studied.
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Effect of an external magnetic field on particle acceleration by a rotating black hole surrounded with quintessential energy

TL;DR: In this article, the authors investigate particle motion and collisions in the vicinity of rotating black holes immersed in combined cosmological quintessential scalar field and external magnetic field, and show that the resulting collisions can be caused by collisions.
References
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Journal ArticleDOI

Quantum Gravity at a Lifshitz Point

TL;DR: In this article, a quantum field theory of gravity with dynamical critical exponent equal to $z = 3$ in the UV is presented. But this theory is restricted to satisfy the condition of detailed balance.
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Spectral dimension of the universe in quantum gravity at a lifshitz point.

TL;DR: It is shown that in gravity with dynamical critical exponent z in D+1 dimensions, the spectral dimension of spacetime is d_{s}=1+D/z, which is similar to the behavior found numerically by Ambjørn et al. in their causal dynamical triangulations approach to quantum gravity.
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Kerr Black Holes as Particle Accelerators to Arbitrarily High Energy

TL;DR: It is shown that intermediate mass black holes conjectured to be the early precursors of supermassive black holes and surrounded by relic cold dark matter density spikes can act as particle accelerators with collisions, in principle, at arbitrarily high center-of-mass energies in the case of Kerr black holes.
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The Black hole and FRW geometries of non-relativistic gravity

TL;DR: In this article, the authors considered the non-relativistic Ho\v{r}ava-Lifshitz four-dimensional theory of gravity and showed that it has the same Newtonian and post-Newtonian limits as GR and thus, it passes the classical tests.
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