Particle Acceleration by Static Black Holes in a Model of Gravity
arXiv:1507.00633 · doi:10.1139/cjp-2017-0138
Abstract
Particle collisions are considered within the context of gravity described by , where stands for the Ricci scalar and is a non-zero constant. The center of mass (CM) energy of head-on colliding particles moving in opposite radial directions near the naked singularity/horizon are considered. Collision of particles in the same direction near the event horizon yields finite energy while the energy of oppositely moving particles grows unbounded. Addition of a cosmological constant does not change the feature. Collision of a massless outgoing photon with an infalling particle and collision of two oppositely moving photons following null-geodesics are also taken into account.
8 pages, 1 figure, Accepted for publication in Canadian Journal of Physics
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