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Color breaking in the early universe

Patel, Hiren H. and Ramsey-Musolf, Michael J. and Wise, Mark B. (2013) Color breaking in the early universe. Physical Review D, 88 (1). Art. No. 015003 . ISSN 1550-7998. doi:10.1103/PhysRevD.88.015003. https://resolver.caltech.edu/CaltechAUTHORS:20130812-151057238

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Abstract

We explore the possibility that SU(3)_C was not an exact symmetry at all times in the early Universe, using minimal extensions of the standard model that contain a color triplet scalar field and perhaps other fields. We show that, for a range of temperatures, there can exist a phase in which the free energy is minimized when the color triplet scalar has a nonvanishing vacuum expectation value, spontaneously breaking color. At very high temperatures and at lower temperatures, color symmetry is restored. The breaking of color in this phase is accompanied by the spontaneous breaking of B - L if the color triplet scalar Yukawa couples to quarks and/or leptons. We discuss the requirements on the minimal extensions needed for consistency of this scenario with present collider bounds on new colored scalar particles.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1103/PhysRevD.88.015003 DOIArticle
http://link.aps.org/doi/10.1103/PhysRevD.88.015003PublisherArticle
ORCID:
AuthorORCID
Patel, Hiren H.0000-0002-2582-6189
Ramsey-Musolf, Michael J.0000-0001-8110-2479
Wise, Mark B.0000-0002-9125-801X
Additional Information:© 2013 American Physical Society. Received 27 March 2013; published 2 July 2013. We thank G. Senjanovic for helpful discussions and for pointing out references to some of the earlier literature. This work of was supported in part by the U.S. Department of Energy Contracts No. DE-FG02-08ER41531 (H. H. P. and M. J. R.-M.) and No. DE-FG02-92ER40701 (M. B.W.) and by the Wisconsin Alumni Research Foundation (H. H. P. and M. J. R.-M.). The research of M. B.W. was supported in part by the Perimeter Institute for Theoretical Physics. Research at the Perimeter Institute is supported by the government of Canada and by the province of Ontario through the Ministry of Economic Development and Innovation.
Group:Caltech Theory
Funders:
Funding AgencyGrant Number
Department of Energy (DOE)DE-FG02-08ER41531
Department of Energy (DOE)DE-FG02-92ER40701
Wisconsin Alumni Research FoundationUNSPECIFIED
Perimeter Institute for Theoretical PhysicsUNSPECIFIED
Ontario Ministry of Economic Development and InnovationUNSPECIFIED
Issue or Number:1
Classification Code:PACS: 98.80.Cq
DOI:10.1103/PhysRevD.88.015003
Record Number:CaltechAUTHORS:20130812-151057238
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20130812-151057238
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:39880
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:12 Aug 2013 22:24
Last Modified:09 Nov 2021 23:47

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