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SO(10) grand unified theories can ensure the stability of new particles in terms of the gauge group structure itself, and in this respect are well suited to accommodate dark matter (DM) candidates in the form of new stable massive particles.
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2001
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S. Davidson and A. Ibarra, A Lower bound on the right-handed neutrino mass from leptogenesis
2002
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G. Servant and T. M. P. Tait, Is the lightest Kaluza-Klein particle a viable dark matter candidate?
2003
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E. Ma, Verifiable radiative seesaw mechanism of neutrino mass and dark matter
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2012
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2012
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M. S. Boucenna, R. A. Lineros and J. W. F. Valle, Planck-scale effects on WIMP dark matter
2013
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A. Dueck and W. Rodejohann, Fits to SO(10) Grand Unified Models
2013
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2014
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R. J. Hill and M. P. Solon, WIMP-nucleon scattering with heavy WIMP effective theory
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C. Arbeláez, M. Hirsch, M. Malinský and J. C. Romão, LHC-scale left-right symmetry and unification
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