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High energy collision of two particles in wormhole spacetimes

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arxiv 1411.5778 v2 pith:IUFAGEHB submitted 2014-11-21 gr-qc

High energy collision of two particles in wormhole spacetimes

classification gr-qc
keywords wormholeparticlescollisionenergyhigheventhorizonparticle
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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.

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    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.