Weakly-interacting massive particles in non-supersymmetric SO(10) grand unified models
Abstract
Here, non-supersymmetric SO(10) grand unified theories provide a framework in which the stability of dark matter is explained while gauge coupling unification is realized. In this work, we systematically study this possibility by classifying weakly interacting dark matter candidates in terms of their quantum numbers of SU(2)L Ⓧ U(1)Y, B – L, and SU(2)R. We consider both scalar and fermion candidates. We show that the requirement of a sufficiently high unification scale to ensure a proton lifetime compatible with experimental constraints plays a strong role in selecting viable candidates. Among the scalar candidates originating from either a 16 or 144 of SO(10), only SU(2)L singlets with zero hypercharge or doublets with Y = 1/2 satisfy all constraints for SU(4)C Ⓧ SU(2)L Ⓧ SU(2)R and SU(3)C Ⓧ SU(2)L Ⓧ SU(2)R Ⓧ U(1)B–L intermediate scale gauge groups. Among fermion triplets with zero hypercharge, only a triplet in the 45 with intermediate group SU(4)C Ⓧ SU(2)L Ⓧ SU(2)R leads to solutions with MGUT > M int and a long proton lifetime. We find three models with weak doublets and Y = 1/2 as dark matter candidates for the SU(4)C Ⓧ SU(2)L Ⓧ SU(2)R and SU(4)C Ⓧ SU(2)L Ⓧ U(1)R intermediate scale gauge groupsmore »
- Authors:
-
- Univ. of Minnesota, Minneapolis, MN (United States); Univ. of Tokyo, Chiba (Japan)
- Univ. of Minnesota, Minneapolis, MN (United States)
- Publication Date:
- Research Org.:
- Minnesota State Univ., Mankato, MN (United States)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1436122
- Grant/Contract Number:
- SC0011842
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Journal of High Energy Physics (Online)
- Additional Journal Information:
- Journal Name: Journal of High Energy Physics (Online); Journal Volume: 2015; Journal Issue: 10; Journal ID: ISSN 1029-8479
- Publisher:
- Springer Berlin
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; 79 ASTRONOMY AND ASTROPHYSICS; GUT; Cosmology of Theories beyond the SM
Citation Formats
Nagata, Natsumi, Olive, Keith A., and Zheng, Jiaming. Weakly-interacting massive particles in non-supersymmetric SO(10) grand unified models. United States: N. p., 2015.
Web. doi:10.1007/JHEP10(2015)193.
Nagata, Natsumi, Olive, Keith A., & Zheng, Jiaming. Weakly-interacting massive particles in non-supersymmetric SO(10) grand unified models. United States. https://doi.org/10.1007/JHEP10(2015)193
Nagata, Natsumi, Olive, Keith A., and Zheng, Jiaming. Wed .
"Weakly-interacting massive particles in non-supersymmetric SO(10) grand unified models". United States. https://doi.org/10.1007/JHEP10(2015)193. https://www.osti.gov/servlets/purl/1436122.
@article{osti_1436122,
title = {Weakly-interacting massive particles in non-supersymmetric SO(10) grand unified models},
author = {Nagata, Natsumi and Olive, Keith A. and Zheng, Jiaming},
abstractNote = {Here, non-supersymmetric SO(10) grand unified theories provide a framework in which the stability of dark matter is explained while gauge coupling unification is realized. In this work, we systematically study this possibility by classifying weakly interacting dark matter candidates in terms of their quantum numbers of SU(2)L Ⓧ U(1)Y, B – L, and SU(2)R. We consider both scalar and fermion candidates. We show that the requirement of a sufficiently high unification scale to ensure a proton lifetime compatible with experimental constraints plays a strong role in selecting viable candidates. Among the scalar candidates originating from either a 16 or 144 of SO(10), only SU(2)L singlets with zero hypercharge or doublets with Y = 1/2 satisfy all constraints for SU(4)C Ⓧ SU(2)L Ⓧ SU(2)R and SU(3)C Ⓧ SU(2)L Ⓧ SU(2)R Ⓧ U(1)B–L intermediate scale gauge groups. Among fermion triplets with zero hypercharge, only a triplet in the 45 with intermediate group SU(4)C Ⓧ SU(2)L Ⓧ SU(2)R leads to solutions with MGUT > M int and a long proton lifetime. We find three models with weak doublets and Y = 1/2 as dark matter candidates for the SU(4)C Ⓧ SU(2)L Ⓧ SU(2)R and SU(4)C Ⓧ SU(2)L Ⓧ U(1)R intermediate scale gauge groups assuming a minimal Higgs content. We also discuss how these models may be tested at accelerators and in dark matter detection experiments.},
doi = {10.1007/JHEP10(2015)193},
journal = {Journal of High Energy Physics (Online)},
number = 10,
volume = 2015,
place = {United States},
year = {Wed Oct 28 00:00:00 EDT 2015},
month = {Wed Oct 28 00:00:00 EDT 2015}
}
Web of Science
Figures / Tables:
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