Left-right symmetric model of neutrino dark energy

被引：5

作者：

Bhatt, Jitesh R. ^{[2
]}

Gu, Pei-Hong ^{[1
]}

Sarkar, Utpal ^{[2
]}

Singh, Santosh K. ^{[2
]}

机构：

[1] Abdus Salam Int Ctr Theoret Phys, I-34014 Trieste, Italy

[2] Phys Res Lab, Ahmadabad 380009, Gujarat, India

来源：

PHYSICS LETTERS B | 2008年 / 663卷 / 1-2期

关键词：

D O I：

10.1016/j.physletb.2008.03.059

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We implemented the neutrino dark energy (nu DE) proposal in a left-right symmetric model. Unlike earlier models of mass varying neutrinos, in the present model the mass parameter that depends on the scalar field (acceleron) remains very light naturally. The required neutrino masses then predicts the U(1)(R) breaking scale to be in the TeV range, providing new signals for LHC. Compared to all other nu DE proposals, this model has the added advantage that it can also be embedded into a grand unified theory. In this scenario leptogenesis occurs through decays of scalars at very high energy. (C) 2008 Elsevier B.V. All rights reserved.

引用

页码：83 / 85

页数：3

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