Endpoint of the Gregory-Laflamme instability of black strings revisited
dc.contributor.author | Figueras, P | |
dc.contributor.author | Franca, T | |
dc.contributor.author | Gu, C | |
dc.contributor.author | Andrade, T | |
dc.date.accessioned | 2023-11-24T14:46:20Z | |
dc.date.available | 2023-11-24T14:46:20Z | |
dc.date.issued | 2023 | |
dc.identifier.issn | 2470-0010 | |
dc.identifier.other | ARTN 044028 | |
dc.identifier.other | ARTN 044028 | |
dc.identifier.uri | https://qmro.qmul.ac.uk/xmlui/handle/123456789/92244 | |
dc.description.abstract | We reproduce and extend the previous studies of Lehner and Pretorius of the endpoint of the Gregory-Laflamme instability of black strings in five space-time dimensions. We consider unstable black strings of fixed thickness and different lengths, and in all cases we confirm that at the intermediate stages of the evolution the horizon can be interpreted as a quasistationary self-similar sequence of black strings connecting spherical black holes on different scales. However, we do not find any evidence for a global timescale relating subsequent generations. The endpoint of the instability is the pinch off of the horizon in finite asymptotic time, thus confirming the violation of the weak cosmic censorship conjecture around black string spacetimes. | en_US |
dc.publisher | American Physical Society | en_US |
dc.relation.ispartof | PHYSICAL REVIEW D | |
dc.rights | Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3. | |
dc.rights | Attribution 3.0 United States | * |
dc.rights.uri | http://creativecommons.org/licenses/by/3.0/us/ | * |
dc.title | Endpoint of the Gregory-Laflamme instability of black strings revisited | en_US |
dc.type | Article | en_US |
dc.rights.holder | © 2023 The Author(s). Published by the American Physical Society | |
dc.identifier.doi | 10.1103/PhysRevD.107.044028 | |
pubs.author-url | https://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000964332800003&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6a | en_US |
pubs.issue | 4 | en_US |
pubs.notes | Not known | en_US |
pubs.publication-status | Published | en_US |
pubs.volume | 107 | en_US |
rioxxterms.funder | Default funder | en_US |
rioxxterms.identifier.project | Default project | en_US |
qmul.funder | NewNGR::European Research Council | en_US |
qmul.funder | NewNGR::European Research Council | en_US |
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Except where otherwise noted, this item's license is described as Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.