Radiative neutrino mass generation and dark energy

被引：6

作者：

Bamba, K. ^{[1
]}

Geng, C. Q. ^{[1
]}

Ho, S. H. ^{[1
]}

机构：

[1] Natl Tsing Hua Univ, Dept Phys, Hsinchu 300, Taiwan

来源：

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2008年 / 09期

关键词：

dark energy theory; neutrino properties; cosmology of theories beyond the SM;

D O I：

10.1088/1475-7516/2008/09/001

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We study models with radiative neutrino mass generation and explore the relation between the neutrino masses and dark energy. In these models, the pseudo-Nambu-Goldstone bosons (pNGBs) arise at two-loop level via the Majorana neutrino masses. In particular, we demonstrate that the potential energy of the pNGB could be the dark energy potential and the observed value of the equation of state parameter of the universe, i.e., w similar or equal to-1, can be realized.

引用

页数：8

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