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Просмотр по теме "Particle collision"

Просмотр по теме "Particle collision"

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  • Zaslavskii O. (2017)
    © 2017 World Scientific Publishing CompanyWe consider stationary axially symmetric black holes with the background scalar field and test particles that can interact with this field directly. Then, particle collision near ...
  • Zaslavskii O. (2016)
    © 2016 World Scientific Publishing Company.We consider collision of two geodesic particles near the lightlike surface (black hole horizon or naked singularity) of such an axially symmetric rotating or static metric that ...
  • Zaslavskii O.B. (2021)
    We consider electrogeodesics on which the energy E 0 in the Reissner-Nordström metric. It is shown that outside the horizon there is exactly one turning point inside the ergoregion for such particles. This entails that ...
  • Zaslavskii O. (2016)
    © 2016, Springer Science+Business Media New York.We consider generic axially symmetric rotating spacetimes and examine particle collisions in the ergoregion. The results are generic and agree with those obtained in the ...
  • Zaslavskii O. (2016)
    © 2016 World Scientific Publishing Company.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 ...
  • Zaslavskii O. (2016)
    © 2016 World Scientific Publishing Company 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 ...
  • Zaslavskii O. (2017)
    © 2017 World Scientific Publishing Company.If two particles collide inside the ergosphere, the energy in the center of mass frame can be made unbound provided at least one of particles has a large negative angular momentum ...
  • Zaslavskii O. (2016)
    © 2017 World Scientific Publishing CompanyIf two particles collide inside the ergosphere, the energy in the center of mass frame can be made unbound provided at least one of particles has a large negative angular momentum ...
  • Zaslavskii O.B. (2020)
    © 2020 World Scientific Publishing Company. We consider collision of two particles 1 and 2 near the horizon of the extremal Reissner-Nordström (RN) black hole that produces two other particles 3 and 4. There exists such a ...
  • Zaslavskii O.B. (2020)
    © 2020, Springer Science+Business Media, LLC, part of Springer Nature. We consider collision of two particles 1 and 2 near the horizon of the extremal rotating axially symmetric neutral generic black hole producing particles ...

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