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.
13 pages. One more scenario considered, ref. 15 added. To appear in Universe (special issue on wormholes)
References in corpus (7)
- Wormholes as Black Hole Foils
- The Collisional Penrose Process
- High energy collision of two particles in wormhole spacetimes
- Are black holes totally black?
- Collisional Penrose Process in Rotating Wormhole Spacetime
- Horizon closeness bounds for static black hole mimickers
- On geodesics with negative energies in the ergoregions of dirty black holes