Weakly-interacting massive particles in non-supersymmetric \(\mathrm{SO}(10)\) grand unified models

DOI10.1007/JHEP10(2015)193zbMath1387.81388arXiv1509.00809MaRDI QIDQ2636051

Natsumi Nagata, Keith A. Olive, Jia-Ming Zheng

Publication date: 31 May 2018

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1509.00809

zbMATH Keywords

cosmology of theories beyond the SMgut

Mathematics Subject Classification ID

Nuclear physics (81V35)

Related Items (4)

On minimal dark matter coupled to the Higgs ⋮ Dark matter from the vector of \(\mathrm{SO}(10)\) ⋮ Asymmetric dark matter models in SO(10) ⋮ Inflaton oscillations and post-inflationary reheating

Cites Work

• Unnamed Item
• Origins of inert Higgs doublets
• Direct detection of electroweak-interacting dark matter
• The minimal moose for a little Higgs
• Relic abundance of LKP dark matter in UED model including effects of second KK resonances
• Model-independent implications of the \(e^{\pm }\), \(\bar{p}\) cosmic ray spectra on properties of Dark Matter
• SO(10) group theory for the unified model building
• Congruence number, a generalization of SU(3) triality
• Neutrino Mass and Spontaneous Parity Nonconservation
• Electroweak symmetry breaking from dimensional deconstruction
• Complete cubic and quartic couplings of \(16\) and \(\overline{16}\) in SO\((10)\) unification

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