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arXiv · 0812.1895

Neutrino Dark Energy in Grand Unified Theories

Jitesh R. Bhatt·Pei-Hong Gu·Utpal Sarkar·Santosh K. Singh
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Abstract

We studied a left-right symmetric model that can accommodate the neutrino dark energy (\nd) proposal. Type III seesaw mechanism is implemented to give masses to the neutrinos. After explaining the model, we study the consistency of the model by minimizing the scalar potential and obtaining the conditions for the required vacuum expectation values of the different scalar fields. This model is then embedded in an SO(10) grand unified theory and the allowed symmetry breaking scales are determined by the condition of the gauge coupling unification. Although $SU(2)_{R}$ breaking is required to be high, its Abelian subgroup $U(1)_{R}$ is broken in the TeV range, which can then give the required neutrino masses and predicts new gauge bosons that could be detected at LHC. The neutrino masses are studied in details in this model, which shows that at least 3 singlet fermions are required.

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Jitesh R. Bhatt, Pei-Hong Gu, Utpal Sarkar, Santosh K. Singh. 2009-09-30. Neutrino Dark Energy in Grand Unified Theories. https://doi.org/10.1103/physrevd.80.073013

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