Stephen F. King
Confronting SO(10) GUTs with proton decay and gravitational waves
King, Stephen F.; Pascoli, Silvia; Zhou, Ye-Ling; Turner, Jessica
Authors
Professor Silvia Pascoli silvia.pascoli@durham.ac.uk
Visiting Professor
Ye-Ling Zhou
Dr Jessica Turner jessica.turner@durham.ac.uk
Associate Professor
Abstract
Grand Unified Theories (GUT) predict proton decay as well as the formation of cosmic strings which can generate gravitational waves. We determine which non-supersymmetric SO(10) breaking chains provide gauge unification in addition to a gravitational signal from cosmic strings. We calculate the GUT and intermediate scales for these SO(10) breaking chains by solving the renormalisation group equations at the two-loop level. This analysis predicts the GUT scale, hence the proton lifetime, in addition to the scale of cosmic string generation and thus the associated gravitational wave signal. We determine which SO(10) breaking chains survive in the event of the null results of the next generation of gravitational waves and proton decay searches and determine the correlations between proton decay and gravitational waves scales if these observables are measured.
Citation
King, S. F., Pascoli, S., Zhou, Y., & Turner, J. (2021). Confronting SO(10) GUTs with proton decay and gravitational waves. Journal of High Energy Physics, 2021(10), Article 225 (2021). https://doi.org/10.1007/jhep10%282021%29225
Journal Article Type | Article |
---|---|
Acceptance Date | Oct 13, 2021 |
Online Publication Date | Oct 28, 2021 |
Publication Date | 2021-10 |
Deposit Date | Jan 12, 2022 |
Publicly Available Date | Jan 14, 2022 |
Journal | Journal of High Energy Physics |
Print ISSN | 1126-6708 |
Publisher | Scuola Internazionale Superiore di Studi Avanzati (SISSA) |
Peer Reviewed | Peer Reviewed |
Volume | 2021 |
Issue | 10 |
Article Number | 225 (2021) |
DOI | https://doi.org/10.1007/jhep10%282021%29225 |
Public URL | https://durham-repository.worktribe.com/output/1218707 |
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Publisher Licence URL
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Copyright Statement
Advance online version This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited.
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