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We consider collision of two particles near static electrically charged extremal black holes and elucidate the conditions under which the energy in the centre of mass frame E_{c.m.} grows unbounded. For a single black hole, we generalize…

General Relativity and Quantum Cosmology · Physics 2015-04-10 O. B. Zaslavskii

We analyze scenarios of particle collisions in the metric of a nonextremal black hole that can potentially lead to ultrahigh energy $E_{c.m.}$ in their centre of mass frame. Particle 1 comes from infinity to the black hole horizon while…

General Relativity and Quantum Cosmology · Physics 2018-04-04 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 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

We consider collision of two particles in the axially symmetric black hole metric in the magnetic field. If the value of the angular momentum |L| of one particles grows unbound (but its Killing energy remains fixed) one can achieve unbound…

General Relativity and Quantum Cosmology · Physics 2014-09-25 O. B. Zaslavskii

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

We consider collision of two geodesic particles near the horizon of such an axially symmetric black hole (rotating or static) that the metric coefficient $g_{\phi \phi }\rightarrow 0$ there. It is shown that (both for regular and singular…

General Relativity and Quantum Cosmology · Physics 2016-09-07 O. B. Zaslavskii

We consider particle collisions in the background of a nonextremal black hole. Two particles fall from infinity, particle 1 is fine-tuned (critical), collision occurs in its turning point. The first example is the Reissner-Nordstr\"{o}m…

General Relativity and Quantum Cosmology · Physics 2020-11-11 O. B. Zaslavskii

We consider collision between two charged (or charged and neutral) particles near the black hole horizon in the strong magnetic field B. It is shown that there exists a strip near the horizon within which collision of any two such particles…

General Relativity and Quantum Cosmology · Physics 2014-07-09 O. B. Zaslavskii

We consider particle collision inside the inner horizon of the Reissner-Nordstrom metric in the so-called R region. We show that there exist scenario in which the enrgy in the center of mass frame grows unbounded. In contrast to the…

General Physics · Physics 2026-03-24 A. V. Toporensky , O. B. Zaslavskii

There are different versions of collisions of two particles near black holes with unbound energy $E_{c.m.}$ in the centre of mass frame. The so-called BSW effect arises when a slow fine-tuned "critical" particle hits a rapid "usual" one. We…

General Relativity and Quantum Cosmology · Physics 2015-02-20 O. B. Zaslavskii

Black holes have sometimes been described as astrophysical particle accelerators because finite energy particles can collide near the horizon with divergent center-of-mass (CM) energy. The collisions are classified by the radial motion of…

General Relativity and Quantum Cosmology · Physics 2025-08-12 Delilah E. A. Gates

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

We investigate particle collisions in non-extremal black hole that can probably induced to extremely high center of mass energy $E_{\text{cm}}$. We consider the collision of two particles where first particle comes from far to the outer…

General Relativity and Quantum Cosmology · Physics 2018-08-22 Ayesha Zakria , Qurat-ul-Ain Satti

We consider collisions between massive (electrons) and massless (photons) particles near the horizon of a rotating black hole. Similarly to collisions between massive particles, the infinite energy in the centre of mass frame occurs in some…

General Relativity and Quantum Cosmology · Physics 2011-05-03 O. B. Zaslavskii

It is shown that the energy in the centre of mass frame of two colliding particles in free fall at any point of the ergosphere of the rotating black hole can grow without limit for fixed energy values of particles on infinity. The effect…

General Relativity and Quantum Cosmology · Physics 2014-09-16 A. A. Grib , Yu. V. Pavlov

The aim of the paper is the consideration of particle collisions in the vicinity of the horizon of rotating black holes. Existence of geodesics for massive and massless particles arising from the region inside of the gravitational radius in…

General Relativity and Quantum Cosmology · Physics 2015-11-09 A. A. Grib , Yu. V. Pavlov

Scattering of particles in the gravitational field of rotating black holes is considered. Expressions for scattering energy of particles in the centre of mass system are obtained. It is shown that scattering energy of particles in the…

General Relativity and Quantum Cosmology · Physics 2014-11-05 A. A. Grib , Yu. V. Pavlov

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

Scattering of particles with different masses and energy in the gravitational field of rotating black holes is considered as outside as inside the black hole. Expressions for scattering energy of particles in the centre of mass system are…

General Relativity and Quantum Cosmology · Physics 2014-11-05 A. A. Grib , Yu. V. Pavlov
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