Weakly-interacting massive particles in non-supersymmetric SO(10) grand unified models

Nagata, Natsumi; Olive, Keith A.; Zheng, Jiaming

doi:10.1007/JHEP10(2015)193

Title: Weakly-interacting massive particles in non-supersymmetric SO(10) grand unified models

Journal Article · Wed Oct 28 00:00:00 EDT 2015 · Journal of High Energy Physics (Online)

DOI:https://doi.org/10.1007/JHEP10(2015)193· OSTI ID:1436122

Nagata, Natsumi ^[1]; Olive, Keith A. ^[2]; Zheng, Jiaming ^[2]

Univ. of Minnesota, Minneapolis, MN (United States); Univ. of Tokyo, Chiba (Japan)
Univ. of Minnesota, Minneapolis, MN (United States)

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 M_GUT > 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.

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Research Organization:: Minnesota State Univ., Mankato, MN (United States)

Sponsoring Organization:: USDOE

Grant/Contract Number:: SC0011842

OSTI ID:: 1436122

Journal Information:: Journal of High Energy Physics (Online), Vol. 2015, Issue 10; ISSN 1029-8479

Publisher:: Springer BerlinCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 42 works

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Inflation and leptogenesis in high-scale supersymmetry Kaneta, Kunio; Mambrini, Yann; Olive, Keith A. Physical Review D, Vol. 101, Issue 1 https://doi.org/10.1103/physrevd.101.015002	journal	January 2020
Supersymmetric versus SO(10) models of dark matter Olive, Keith A. International Journal of Modern Physics A, Vol. 32, Issue 13 https://doi.org/10.1142/s0217751x17300101	journal	May 2017
Supersymmetric versus SO(10) Models of Dark Matter Olive, Keith A. Conference on Cosmology, Gravitational Waves and Particles https://doi.org/10.1142/9789813231801_0009	conference	January 2018
Axion Predictions in $SO(10)×U(1)_{PQ}$ Models Ernst, Anne; Ringwald, Andreas; Tamarit, Carlos Deutsches Elektronen-Synchrotron, DESY, Hamburg https://doi.org/10.3204/pubdb-2018-00658	text	January 2018
Vacuum Stability and Radiative Electroweak Symmetry Breaking in an SO(10) Dark Matter Model Mambrini, Yann; Nagata, Natsumi; Olive, Keith A. arXiv https://doi.org/10.48550/arxiv.1602.05583	text	January 2016
Enhancement of the Dark Matter Abundance Before Reheating: Applications to Gravitino Dark Matter Garcia, Marcos A. G.; Mambrini, Yann; Olive, Keith A. arXiv https://doi.org/10.48550/arxiv.1709.01549	text	January 2017
Radiative Production of Non-thermal Dark Matter Kaneta, Kunio; Mambrini, Yann; Olive, Keith A. arXiv https://doi.org/10.48550/arxiv.1901.04449	text	January 2019
Inflation and Leptogenesis in High-Scale Supersymmetry Kaneta, Kunio; Mambrini, Yann; Olive, Keith A. arXiv https://doi.org/10.48550/arxiv.1911.02463	text	January 2019