Particle acceleration by static black holes in a model of f (R) gravity

M. Halilsoy, ALI OVGUN

Research output: Contribution to journalArticlepeer-review

5 Scopus citations

Abstract

Particle collisions are considered within the context of f(R) gravity described by f(R)=R+2αR, where R stands for the Ricci scalar and α is a nonzero constant. The center of mass energy of head-on colliding particles moving in opposite radial directions near the naked singularity or 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 this 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.

Original languageEnglish
Pages (from-to)1037-1041
Number of pages5
JournalCanadian Journal of Physics
Volume95
Issue number11
DOIs
StatePublished - 1 Jan 2017

Keywords

  • Black holes
  • f (R) gravity
  • Motion of particles

Fingerprint Dive into the research topics of 'Particle acceleration by static black holes in a model of f (R) gravity'. Together they form a unique fingerprint.

Cite this