Particle collisions near static spherically symmetric black holes
Eva Hackmann, Hemwati Nandan, Pankaj Sheoran
Abstract
It has been shown by Bañados, Silk and West (BSW) that the center of mass energy (Ecm) of test particles starting from rest at infinity and colliding near the horizon of a Schwarzschild black hole is always finite. In this short note, we extent the BSW scenario and study two particles with different energies colliding near the horizon of a static spherically symmetric black hole. Interestingly, we find that even for the static spherically symmetric (i.e., Schwarzschild like) black holes it is possible to obtain an arbitrarily high Ecm from the two test particles colliding near but outside of the horizon of a black hole, if one fine-tunes the parameters of geodesic motion.
Topics & Concepts
PhysicsSchwarzschild radiusHorizonBlack hole (networking)Test particleSchwarzschild metricPhoton sphereSchwarzschild geodesicsParticle (ecology)GeodesicHawking radiationCircular symmetryClassical mechanicsCharged black holeGeometryGeneral relativityKerr metricGravitationRouting (electronic design automation)Routing protocolOceanographyGeologyLink-state routing protocolComputer scienceMathematicsComputer networkAstronomyAstrophysical Phenomena and ObservationsPulsars and Gravitational Waves ResearchBlack Holes and Theoretical Physics