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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...
Autores principales: | , , |
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Lenguaje: | eng |
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2020
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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. |
id | cern-2764475 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2020 |
record_format | invenio |
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 |