pith. machine review for the scientific record. sign in

arxiv: 1411.5778 · v2 · submitted 2014-11-21 · 🌀 gr-qc

Recognition: unknown

High energy collision of two particles in wormhole spacetimes

Authors on Pith no claims yet
classification 🌀 gr-qc
keywords wormholeparticlescollisionenergyhigheventhorizonparticle
0
0 comments X
read the original abstract

We study the collision of two particles in the Teo wormhole spacetime, in which the wormhole is stationary and axisymmetric. We show that a non-rotating Teo wormhole cannot be a particle accelerator, while a rotating Teo wormhole can be used to accelerate particles and create high energy collisions because of the deep effective potential of the colliding particles. The process is different from that in the vicinity of a near-extremal black hole, since here there is no event horizon. This is the first example of particle collision with high center-of-mass energy in a spacetime with no event horizon, no naked singularity, and not being extremal in a clear sense. The process can unlikely have direct implications for astrophysical observations, but it is interesting as a tool to investigate wormhole instabilities.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Dymnikova-Schwinger quantum-corrected slowly rotating wormholes: Photon and spinning particle dynamics

    gr-qc 2026-04 unverdicted novelty 5.0

    GUP-corrected rotating wormholes based on the Dymnikova-Schwinger profile produce split co- and counter-rotating photon spheres and asymmetric shadows.