Can the Reissner-Nordström black hole or Schwarzschild black hole be the stable Planck-scale particle accelerator?
arXiv:1108.1843 · doi:10.1103/PhysRevD.84.123002
Abstract
It is shown that the extremal Reissner-Nordström black hole, the non-extremal one with multiple scattering particles, and the Schwarzschild black hole with radial head-on particles are stable under the collision of the particles near the horizon, if the back-reaction effect and the effect generated by gravity of particles are involved. Moreover, the collision near Reissner-Nordström black holes with astrophysically typical mass can not generate the Planck-scale center-of-mass energy. However, the head-on collision near the typical primordial black hole could just occur at the Planck-energy scale.
14 pages, 4 figures, minor changes, accepted for publication in Phys. Rev. D
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- Characterizing repulsive gravity with curvature eigenvalues
- Acceleration of particles by Janis-Newman-Winicour singularities
- Kerr black holes as accelerators of spinning test particles
- Charged spinning black holes as accelerators of spinning particles
- Ultra-high energy particle collisions in a regular spacetime without blackholes or naked singularities
- Effects of acceleration on the collision of particles in the rotating black hole spacetime
- Charged Dilation Black Holes as Particle Accelerators
- Particle collisions in the lower dimensional rotating black hole space-time with the cosmological constant
- Particle acceleration by Majumdar-Papapetrou di-hole
- Schwarzschild black hole surrounded by quintessential matter field as an accelerator for spinning particles
- An Investigation of the Casimir Energy for a Fermion Coupled to the Sine-Gordon Soliton with Parity Decomposition
- BSW process of the slowly evaporating charged black hole