On the energy of particle collisions in the ergosphere of the rotating black holes
arXiv:1301.0698 · doi:10.1209/0295-5075/101/20004
Abstract
It is shown that the energy in the centre of mass frame of colliding particles in free fall at any point of the ergosphere of the rotating black hole can grow without limit for fixed energy values on infinity. The effect takes place for large negative values of the angular momentum of one of the particles.
arXiv comment4 pages, 1 figure
References in corpus (12)
- Kerr Black Holes as Particle Accelerators to Arbitrarily High Energy
- On particle collisions in the gravitational field of the Kerr black hole
- Collision of two general geodesic particles around a Kerr black hole
- On particles collisions near rotating black holes
- Acceleration of particles by black holes -- general explanation
- Acceleration of particles by black holes: kinematic explanation
- On the collisions between particles in the vicinity of rotating black holes
- Do active galactic nuclei convert dark matter into visible particles?
- Superheavy Particles in Friedmann Cosmology and the Dark Matter Problem
- High energy processes in the vicinity of the Kerr's black hole horizon
- On collisions with unlimited energies in the vicinity of Kerr and Schwarzschild black hole horizons
- Acceleration of particles by black holes as a result of deceleration: ultimate manifestation of kinematic nature of BSW effect
Cited by in corpus (17)
- Particle collisions and optical effects in the mining Kerr--Newman spacetimes
- Rotating Ayón-Beato-García black hole as a particle accelerator
- Geodesics with negative energy in the ergosphere of rotating black holes
- Are black holes totally black?
- Is the super-Penrose process possible near black holes?
- Unbound geodesics from the ergosphere and potential observability of debris from ultrahigh energy particle collisions
- Ultra-high-energy head-on collisions without horizons or naked singulrities: general approach
- Comparison of particle properties in Kerr metric and in rotating coordinates
- Schwarzschild black hole surrounded by quintessential matter field as an accelerator for spinning particles
- Black holes and particles with zero or negative energy
- High energy physics in the vicinity of rotating black holes
- Rotation as an origin of high energy particle collisions
- Several solutions of the Klein-Gordon equation in Kerr-Newman spacetime and the BSW effect
- Rapidly rotating spacetimes and collisional super-Penrose process
- On the limiting energy of the collision of elementary particles close to horizon of the rotating black hole
- High energy collision of particles in the magnetic field far from black holes
- Properties of particles in the ergosphere of black holes