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Particle collisions near static spherically symmetric black holes

It has been shown by Bañados, Silk and West (BSW) that the center of mass energy ( Ecm ) of test particles starting from rest at infinity and colliding near the horizon of a Schwarzschild black hole is always finite. In this short note, we extent the BSW scenario and study two particles with differe...

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Detalles Bibliográficos
Autores principales: Hackmann, Eva, Nandan, Hemwati, Sheoran, Pankaj
Lenguaje:eng
Publicado: 2020
Materias:
Acceso en línea:https://dx.doi.org/10.1016/j.physletb.2020.135850
http://cds.cern.ch/record/2764475
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author Hackmann, Eva
Nandan, Hemwati
Sheoran, Pankaj
author_facet Hackmann, Eva
Nandan, Hemwati
Sheoran, Pankaj
author_sort Hackmann, Eva
collection CERN
description It has been shown by Bañados, Silk and West (BSW) that the center of mass energy ( Ecm ) of test particles starting from rest at infinity and colliding near the horizon of a Schwarzschild black hole is always finite. In this short note, we extent the BSW scenario and study two particles with different energies colliding near the horizon of a static spherically symmetric black hole. Interestingly, we find that even for the static spherically symmetric (i.e., Schwarzschild like) black holes it is possible to obtain an arbitrarily high Ecm from the two test particles colliding near but outside of the horizon of a black hole, if one fine-tunes the parameters of geodesic motion.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2020
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spelling cern-27644752021-05-04T07:19:28Zdoi:10.1016/j.physletb.2020.135850doi:10.1016/j.physletb.2020.135850http://cds.cern.ch/record/2764475engHackmann, EvaNandan, HemwatiSheoran, PankajParticle collisions near static spherically symmetric black holesgr-qcGeneral Relativity and CosmologyIt has been shown by Bañados, Silk and West (BSW) that the center of mass energy ( Ecm ) of test particles starting from rest at infinity and colliding near the horizon of a Schwarzschild black hole is always finite. In this short note, we extent the BSW scenario and study two particles with different energies colliding near the horizon of a static spherically symmetric black hole. Interestingly, we find that even for the static spherically symmetric (i.e., Schwarzschild like) black holes it is possible to obtain an arbitrarily high Ecm from the two test particles colliding near but outside of the horizon of a black hole, if one fine-tunes the parameters of geodesic motion.It has been shown by Ba\~{n}ados, Silk and West (BSW) that the center of mass energy (E_cm) of test particles starting from rest at infinity and colliding near the horizon of a Schwarzschild black hole is always finite. In this communication, we extent the BSW scenario and study two particles with different energies colliding near the horizon of a static spherically symmetric black hole. Surprisingly, we find that even for the static spherically symmetric (i.e., Schwarzschild like) black holes it is possible to obtain an arbitrarily high E cm from the two test particles colliding near the horizon of a black hole, if one fine-tunes the parameters of geodesic motion.arXiv:2006.05045oai:cds.cern.ch:27644752020-06-09
spellingShingle gr-qc
General Relativity and Cosmology
Hackmann, Eva
Nandan, Hemwati
Sheoran, Pankaj
Particle collisions near static spherically symmetric black holes
title Particle collisions near static spherically symmetric black holes
title_full Particle collisions near static spherically symmetric black holes
title_fullStr Particle collisions near static spherically symmetric black holes
title_full_unstemmed Particle collisions near static spherically symmetric black holes
title_short Particle collisions near static spherically symmetric black holes
title_sort particle collisions near static spherically symmetric black holes
topic gr-qc
General Relativity and Cosmology
url https://dx.doi.org/10.1016/j.physletb.2020.135850
https://dx.doi.org/10.1016/j.physletb.2020.135850
http://cds.cern.ch/record/2764475
work_keys_str_mv AT hackmanneva particlecollisionsnearstaticsphericallysymmetricblackholes
AT nandanhemwati particlecollisionsnearstaticsphericallysymmetricblackholes
AT sheoranpankaj particlecollisionsnearstaticsphericallysymmetricblackholes