scholarly journals Zero-momentum trajectories inside a black hole and high energy particle collisions

2019 ◽  
Vol 2019 (12) ◽  
pp. 063-063 ◽  
Author(s):  
A.V. Toporensky ◽  
O.B. Zaslavskii
2020 ◽  
Vol 37 (22) ◽  
pp. 225010
Author(s):  
Anik Rudra ◽  
Hemwati Nandan ◽  
Radouane Gannouji ◽  
Soham Chakraborty ◽  
Arindam Kumar Chatterjee

2016 ◽  
Vol 31 (04) ◽  
pp. 1650029 ◽  
Author(s):  
O. B. Zaslavskii

We consider collision of two particles in rotating spacetimes without horizons. If the metric coefficient responsible for rotation of spacetime is big enough, the energy of collisions in the center of mass frame can be as large as one likes. This can happen in the ergoregion only. The results are model-independent and apply both to relativistic stars and wormholes.


Universe ◽  
2020 ◽  
Vol 6 (12) ◽  
pp. 227
Author(s):  
Oleg B. Zaslavskii

We suggest two new scenarios of high-energy particle collisions in the background of a wormhole. In scenario 1, the novelty consists of the fact 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.


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