Cosmology with massive neutrinos coupled to dark energy - art. no. 061301

被引：153

作者：

Brookfield, AW

van de Bruck, C

Mota, DF

Tocchini-Valentini, D

机构：

[1] Univ Sheffield, Dept Appl Math, Sheffield S3 7RH, S Yorkshire, England

[2] Univ Sheffield, Dept Phys, Astroparticle Theory & Cosmol Grp, Sheffield S3 7RH, S Yorkshire, England

[3] Univ Oxford, Dept Astrophys, Oxford OX1 3RH, England

[4] Univ Oslo, Inst Theoret Astrophys, N-0315 Oslo, Norway

来源：

PHYSICAL REVIEW LETTERS | 2006年 / 96卷 / 06期

关键词：

D O I：

10.1103/PhysRevLett.96.061301

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Cosmological consequences of a coupling between massive neutrinos and dark energy are investigated. In such models, the neutrino mass is a function of a scalar field, which plays the role of dark energy. The evolution of the background and cosmological perturbations are discussed. We find that mass-varying neutrinos can leave a significant imprint on the anisotropies in the cosmic microwave background and even lead to a reduction of power on large angular scales.

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