Black hole pair production on cosmic strings in the presence of a background magnetic field

We investigate the pair creation of magnetically charged black holes on a cosmic string in the presence of a background magnetic field. The string may either break or fray to produce a pair of accelerating black holes described by Ernst metric. By using the instanton action we obtain the rate of suc...

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Main Authors: Amjad Ashoorioon, Mohammad Bagher Jahani Poshteh
Format: Article
Language:English
Published: Elsevier 2021-05-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269321001647
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spelling doaj-25207eaa6c634bf2b6ce5344fde98de42021-03-25T04:26:14ZengElsevierPhysics Letters B0370-26932021-05-01816136224Black hole pair production on cosmic strings in the presence of a background magnetic fieldAmjad Ashoorioon0Mohammad Bagher Jahani Poshteh1School of Physics, Institute for Research in Fundamental Sciences (IPM), P.O. Box 19395-5531, Tehran, IranCorresponding author.; School of Physics, Institute for Research in Fundamental Sciences (IPM), P.O. Box 19395-5531, Tehran, IranWe investigate the pair creation of magnetically charged black holes on a cosmic string in the presence of a background magnetic field. The string may either break or fray to produce a pair of accelerating black holes described by Ernst metric. By using the instanton action we obtain the rate of such production. For large values of background magnetic field the production of large black holes is probable. Comparing our results with the case of black hole pair creation in magnetic field with no string, we show that fraying/breaking of the cosmic string can substantially enhance the production rate. We also obtain the result of monopole-antimonopole pair production on cosmic string in an external magnetic field, using the WKB approximation and compare it with the black hole results. We also provide a heuristic study of black hole pair creation on cosmic string in the presence of a magnetic field in the de Sitter background, although the analog of Ernst metric with a cosmological constant is lacking. Like a cosmic string and/or a background magnetic field, a positive cosmological constant increases the production rate.http://www.sciencedirect.com/science/article/pii/S0370269321001647
collection DOAJ
language English
format Article
sources DOAJ
author Amjad Ashoorioon
Mohammad Bagher Jahani Poshteh
spellingShingle Amjad Ashoorioon
Mohammad Bagher Jahani Poshteh
Black hole pair production on cosmic strings in the presence of a background magnetic field
Physics Letters B
author_facet Amjad Ashoorioon
Mohammad Bagher Jahani Poshteh
author_sort Amjad Ashoorioon
title Black hole pair production on cosmic strings in the presence of a background magnetic field
title_short Black hole pair production on cosmic strings in the presence of a background magnetic field
title_full Black hole pair production on cosmic strings in the presence of a background magnetic field
title_fullStr Black hole pair production on cosmic strings in the presence of a background magnetic field
title_full_unstemmed Black hole pair production on cosmic strings in the presence of a background magnetic field
title_sort black hole pair production on cosmic strings in the presence of a background magnetic field
publisher Elsevier
series Physics Letters B
issn 0370-2693
publishDate 2021-05-01
description We investigate the pair creation of magnetically charged black holes on a cosmic string in the presence of a background magnetic field. The string may either break or fray to produce a pair of accelerating black holes described by Ernst metric. By using the instanton action we obtain the rate of such production. For large values of background magnetic field the production of large black holes is probable. Comparing our results with the case of black hole pair creation in magnetic field with no string, we show that fraying/breaking of the cosmic string can substantially enhance the production rate. We also obtain the result of monopole-antimonopole pair production on cosmic string in an external magnetic field, using the WKB approximation and compare it with the black hole results. We also provide a heuristic study of black hole pair creation on cosmic string in the presence of a magnetic field in the de Sitter background, although the analog of Ernst metric with a cosmological constant is lacking. Like a cosmic string and/or a background magnetic field, a positive cosmological constant increases the production rate.
url http://www.sciencedirect.com/science/article/pii/S0370269321001647
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