New scenarios of high-energy particle collisions near wormholes
arXiv:2009.11894
Abstract
We suggest two new scenarios of high-energy particle collisions in the background of a wormhole. In scenario 1 the novelty consists in that the effect does not require two particles coming from different mouths. Instead, all such scenarios of high energy collisions develop, when an experimenter sends particles towards a wormhole from the same side of the throat. For static wormholes, this approach leads to indefinitely large energy in the center of mass. For rotating wormholes, it makes possible the super-Penrose process (unbounded energies measured at infinity). In scenario 2, one of colliding particles oscillates near the wormhole throat from the very beginning. In this sense, scenario 2 is intermediate between the standard one and scenario 1 since the particle under discussion does not come from infinity at all.
arXiv comment13 pages. One more scenario considered, ref. 15 added. To appear in Universe (special issue on wormholes)
References in corpus (13)
- Kerr Black Holes as Particle Accelerators to Arbitrarily High Energy
- Wormholes as Black Hole Foils
- Rotating traversable wormholes
- The Collisional Penrose Process
- High energy collision of two particles in wormhole spacetimes
- Are black holes totally black?
- Infinite efficiency of collisional Penrose process: Can over-spinning Kerr geometry be the source of ultra-high-energy cosmic rays and neutrinos ?
- Center of mass energy of colliding electrically neutral particles and super-Penrose process
- Collisional Penrose Process in Rotating Wormhole Spacetime
- Horizon closeness bounds for static black hole mimickers
- Super-Penrose process and rotating wormholes
- Schwarzschild-Like Wormholes as Accelerators
- On geodesics with negative energies in the ergoregions of dirty black holes