It is shown that in the Schwarzschild background there exists a direct counterpart of the Bañados-Silk-West effect for spinning particles. This means that if two particles collide near the black-hole horizon, their energy in the centre-of-mass frame can grow unbounded. In doing so, the crucial role is played by the so-called near-critical trajectories when the particle parameters are almost fine-tuned. A direct scenario of the collision under discussion is possible with restriction on the energy-to-mass ratio $E/m<\frac{1}{2\sqrt{3}}$ only. However, if one takes into account multiple scattering, this becomes possible for $E\geq m$ as well
© 2014 American Physical Society. If two particles moving towards a black hole collide near the hori...
If two geodesic particles collide near a rotating black hole, their energy in the centre of mass fra...
© 2014 American Physical Society. If two particles moving towards a black hole collide near the hori...
© CopyrightEPLA, 2016.It is shown that in the Schwarzschild background there exists a direct counter...
© CopyrightEPLA, 2016.It is shown that in the Schwarzschild background there exists a direct counter...
© CopyrightEPLA, 2016.It is shown that in the Schwarzschild background there exists a direct counter...
© 2020 American Physical Society. If two particles collide near the rotating extremal black hole and...
© 2020, Pleiades Publishing, Inc. We consider collision of two particles near the horizon of a nonex...
© 2015 World Scientific Publishing Company. If two particles move toward a black hole and collide ne...
© 2014 American Physical Society. If two particles moving towards a black hole collide near the hori...
© 2015 World Scientific Publishing Company. If two particles move toward a black hole and collide ne...
Bañados et al. (BSW) found that Kerr black holes can act as particle accelerators with collisions at...
© 2014 American Physical Society. If two particles moving towards a black hole collide near the hori...
© 2015 World Scientific Publishing Company. If two particles move toward a black hole and collide ne...
If two geodesic particles collide near a rotating black hole, their energy in the centre of mass fra...
© 2014 American Physical Society. If two particles moving towards a black hole collide near the hori...
If two geodesic particles collide near a rotating black hole, their energy in the centre of mass fra...
© 2014 American Physical Society. If two particles moving towards a black hole collide near the hori...
© CopyrightEPLA, 2016.It is shown that in the Schwarzschild background there exists a direct counter...
© CopyrightEPLA, 2016.It is shown that in the Schwarzschild background there exists a direct counter...
© CopyrightEPLA, 2016.It is shown that in the Schwarzschild background there exists a direct counter...
© 2020 American Physical Society. If two particles collide near the rotating extremal black hole and...
© 2020, Pleiades Publishing, Inc. We consider collision of two particles near the horizon of a nonex...
© 2015 World Scientific Publishing Company. If two particles move toward a black hole and collide ne...
© 2014 American Physical Society. If two particles moving towards a black hole collide near the hori...
© 2015 World Scientific Publishing Company. If two particles move toward a black hole and collide ne...
Bañados et al. (BSW) found that Kerr black holes can act as particle accelerators with collisions at...
© 2014 American Physical Society. If two particles moving towards a black hole collide near the hori...
© 2015 World Scientific Publishing Company. If two particles move toward a black hole and collide ne...
If two geodesic particles collide near a rotating black hole, their energy in the centre of mass fra...
© 2014 American Physical Society. If two particles moving towards a black hole collide near the hori...
If two geodesic particles collide near a rotating black hole, their energy in the centre of mass fra...
© 2014 American Physical Society. If two particles moving towards a black hole collide near the hori...