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Higgs vacuum decay from particle collisions?

Cuspinera, Leopoldo; Gregory, Ruth; Marshall, Katie M.; Moss, Ian G.

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Authors

Leopoldo Cuspinera

Ruth Gregory

Katie M. Marshall

Ian G. Moss



Abstract

We examine the effect of large extra dimensions on black hole seeded vacuum decay using the Randall-Sundrum model as a prototype for warped extra dimensions. We model the braneworld black hole by a tidal solution and solve the Higgs equations of motion for the instanton on the brane. Remarkably, the action of the static instanton can be shown to be the difference in the bulk areas of the seed and remnant black holes, and we estimate these areas assuming the black holes are small compared to the bulk anti–de Sitter radius. Comparing to the Hawking evaporation rate shows that small black hole seeds preferentially catalyze vacuum decay, thus extending our previous results to higher-dimensional braneworld scenarios. The parameter ranges do not allow for standard model Higgs decay from collider black holes, but they can be relevant for cosmic ray collisions.

Citation

Cuspinera, L., Gregory, R., Marshall, K. M., & Moss, I. G. (2019). Higgs vacuum decay from particle collisions?. Physical Review D, 99(2), Article 024046. https://doi.org/10.1103/physrevd.99.024046

Journal Article Type Article
Acceptance Date Dec 12, 2018
Online Publication Date Jan 30, 2019
Publication Date Jan 15, 2019
Deposit Date Jan 31, 2019
Publicly Available Date Jan 31, 2019
Journal Physical Review D
Print ISSN 2470-0010
Electronic ISSN 2470-0029
Publisher American Physical Society
Peer Reviewed Peer Reviewed
Volume 99
Issue 2
Article Number 024046
DOI https://doi.org/10.1103/physrevd.99.024046

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Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/

Copyright Statement
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.





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