Dark matter and gauge coupling unification in nonsupersymmetric SO(10) grand unified models

Yann Mambrini, Natsumi Nagata, Keith A. Olive, Jérémie Quevillon, and Jiaming Zheng
Phys. Rev. D 91, 095010 – Published 13 May 2015

Abstract

Unlike minimal SU(5), SO(10) provides a straightforward path towards gauge coupling unification by modifying the renormalization group evolution of the gauge couplings above some intermediate scale which may also be related to the seesaw mechanism for neutrino masses. Unification can be achieved for several different choices of the intermediate gauge group below the SO(10) breaking scale. In this work, we consider in detail the possibility that SO(10) unification may also provide a natural dark matter candidate, stability being guaranteed by a leftover Z2 symmetry. We systematically examine the possible intermediate gauge groups which allow a nondegenerate, fermionic, Standard Model singlet dark matter candidate while at the same time respecting gauge coupling unification. Our analysis is done at the two-loop level. Surprisingly, despite the richness of SO(10), we find that only two models survive the analysis of phenomenological constraints, which include suitable neutrino masses, proton decay, and reheating.

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  • Received 3 March 2015

DOI:https://doi.org/10.1103/PhysRevD.91.095010

© 2015 American Physical Society

Authors & Affiliations

Yann Mambrini1, Natsumi Nagata2,3, Keith A. Olive2, Jérémie Quevillon4, and Jiaming Zheng2

  • 1Laboratoire de Physique Théorique Université Paris-Sud, F-91405 Orsay, France
  • 2William I. Fine Theoretical Physics Institute, School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
  • 3Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan
  • 4Theoretical Particle Physics & Cosmology, Department of Physics, King’s College London, London WC2R 2LS, United Kingdom

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Issue

Vol. 91, Iss. 9 — 1 May 2015

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