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We study the possibility of obtaining unbound energy E_{c.m.} in the centre of mass frame when two particles collide near the inner black hole horizon. We consider two different cases - when both particles move (i) in the same direction or…

General Relativity and Quantum Cosmology · Physics 2013-05-30 O. B. Zaslavskii

If two particles collide near the black hole horizon, the energy in the centre of mass (CM) frame can grow indefinitely (the so-called the BSW effect). This requires fine-tuning the parameters (the energy, angular momentum or electric…

General Relativity and Quantum Cosmology · Physics 2015-06-11 O. B. Zaslavskii

We consider stationary axially symmetric black holes with the background scalar field and test particles that can interact with this field directly. Then, particle collision near a black hole can lead to the unbounded energy $% E_{c.m.}$ in…

General Relativity and Quantum Cosmology · Physics 2017-09-22 O. B. Zaslavskii

We investigate the effect of superradiance shielding for the analogue rotating black holes simulated by optical vortices by calculating the radial motion of massless particles in such spacetime background. We add the conditions…

General Relativity and Quantum Cosmology · Physics 2023-03-28 Hongbin Zhang , Baocheng Zhang

We consider generic nonextremal stationary dirty black holes. It is shown that in the vicinity of any bifurcation surface the energy of collision of two particles in the centre of mass frame can grow unbound. This is a generic property…

General Relativity and Quantum Cosmology · Physics 2015-06-04 O. B. Zaslavskii

A number of long-standing puzzles, such as the origin of ultrahigh-energy cosmic rays, could perhaps be solved if we found a mechanism for effectively transferring energy from black holes to particles and, correspondingly, accelerating the…

General Relativity and Quantum Cosmology · Physics 2019-04-12 S. Krasnikov , M. V. Skvortsova

If two particles collide near the horizon of a rotating extremal black hole, under certain conditions the energy E_{c.m.} in the center-of-mass frame can grow without limit (the so-called Banados-Silk-West effect). We consider collisions…

General Relativity and Quantum Cosmology · Physics 2015-06-05 O. B. Zaslavskii

The center-of-mass energy of two particles can become arbitrarily large if they collide near the event horizon of an extremal Kerr black hole, which is called the Ba$\rm \tilde n$ados-Silk-West (BSW) effect. We consider such a high-energy…

General Relativity and Quantum Cosmology · Physics 2016-03-02 Kota Ogasawara , Tomohiro Harada , Umpei Miyamoto

The classical Penrose process and the collisional Penrose processes involve particles decaying or interacting very close to a spinning black hole, in which some particles acquire negative energy and fall into the black hole while others…

High Energy Astrophysical Phenomena · Physics 2026-04-08 Shravan Vengalil Menon , Kun Hu , Henric Krawczynski

Recently, O.B.Zaslavskii considers the collision near the horizon of the extremal Kerr black hole that produces two particles and one of two particles has divergent conserved killing energy(the so called super Penrose process).…

General Relativity and Quantum Cosmology · Physics 2020-09-03 Shun Jiang

We consider the background of a rotating axially symmetric black hole. Let particle 0 decay to two fragments 1 and 2 in the direction parallel to that of particle 0. It is shown that if decay occurs inside the ergoregion, both particles 1…

General Relativity and Quantum Cosmology · Physics 2023-10-13 O. B. Zaslavskii

The Penrose process in the vicinity of an extremal Ban\~ados-Teitelboim-Zanelli(BTZ) black hole is studied. Due to the existence of negative cosmological constant, only massless particles could escape to infinity. Hence we analyse the…

General Relativity and Quantum Cosmology · Physics 2021-03-03 Xianglong Wu , Xiangdong Zhang

We consider a process where two identical massive particles fall inwards, starting from rest at infinity towards the extremal Kerr black hole, collide outside the event horizon in its vicinity and produce two massless particles. The center…

General Relativity and Quantum Cosmology · Physics 2020-07-07 Mandar Patil , Tomohiro Harada

We consider head-on collisions of two particles near the event horizon. Particle 1 is outgoing, particle 2 is ingoing. We elucidate, in which case the energy $E_{c.m.}$ in the center of mass frame can grow unbounded. If the proper time…

General Relativity and Quantum Cosmology · Physics 2025-01-09 H. V. Ovcharenko , O. B. Zaslavskii

It has been shown that ultraenergetic collisions can occur near the horizon of an extremal Kerr black hole. Previous studies mainly focused on geodesic motions of particles. In this paper, we consider spinning test particles whose orbits…

General Relativity and Quantum Cosmology · Physics 2016-05-04 Minyong Guo , Sijie Gao

Penrose described a process that, in principle, could extract energy and angular momentum from a rotating black hole. Here we examine two procedures that were claimed to be capable of implementing the Penrose idea; both make use of a…

General Relativity and Quantum Cosmology · Physics 2009-08-20 Leon Heller

The collisional Penrose process received much attention when Banados, Silk and West (BSW) pointed out the possibility of test-particle collisions with arbitrarily high center-of-mass energy in the vicinity of the horizon of an extremally…

General Relativity and Quantum Cosmology · Physics 2022-03-02 Filip Hejda , José P. S. Lemos , Oleg B. Zaslavskii

Energy extraction from a rotating or charged black hole is one of fascinating issues in general relativity. The collisional Penrose process is one of such extraction mechanisms and has been reconsidered intensively since Banados, Silk and…

General Relativity and Quantum Cosmology · Physics 2017-08-15 Ken-ichi Nakao , Hirotada Okawa , Kei-ichi Maeda

The collision of two particles in the background of a Sen black hole is studied. With the equations of motion of the particles, the center-of-mass energy is investigated when the collision takes place at the horizon of a Sen black hole. For…

High Energy Physics - Theory · Physics 2010-12-23 Shao-Wen Wei , Yu-Xiao Liu , Hai-Tao Li , Feng-Wei Chen

A universal geometric inequality for bodies relating energy, size, angular momentum, and charge is naturally implied by Bekenstein's entropy bounds. We establish versions of this inequality for axisymmetric bodies satisfying appropriate…

General Relativity and Quantum Cosmology · Physics 2018-06-20 Jaroslaw S. Jaracz , Marcus A. Khuri