Neutrino dark energy in grand unified theories

Bhatt, Jitesh R. ; Gu, Pei-Hong ; Sarkar, Utpal ; Singh, Santosh K. (2009) Neutrino dark energy in grand unified theories Physical Review D - Particles, Fields, Gravitation and Cosmology, 80 (7). 073013_1-073013_14. ISSN 1550-7998

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Official URL: http://prd.aps.org/abstract/PRD/v80/i7/e073013

Related URL: http://dx.doi.org/10.1103/PhysRevD.80.073013

Abstract

We studied a left-right symmetric model that can accommodate the neutrino dark energy (νDE) proposal. The 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 detail in this model, which shows that at least 3 singlet fermions are required.

Item Type:Article
Source:Copyright of this article belongs to The American Physical Society.
ID Code:45444
Deposited On:28 Jun 2011 05:32
Last Modified:18 May 2016 01:43

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