Neutrino clustering in growing neutrino quintessence

被引：71

作者：

Mota, D. F. ^{[1
]}

Pettorino, V. ^{[1
]}

Robbers, G. ^{[1
]}

Wetterich, C. ^{[1
]}

机构：

[1] Heidelberg Univ, Inst Theoret Phys, D-69120 Heidelberg, Germany

来源：

PHYSICS LETTERS B | 2008年 / 663卷 / 03期

关键词：

D O I：

10.1016/j.physletb.2008.03.060

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A growing neutrino mass can stop the dynamical evolution of a dark energy scalar field, thus explaining the "why now" problem. We show that such models lead to a substantial neutrino clustering on the scales of superclusters. Non-linear neutrino lumps form at redshift z approximate to 1 and could partially drag the clustering of dark matter. If observed, large scale non-linear structures could be an indication for a new attractive "cosmon force" stronger than gravity. (C) 2008 Elsevier B.V. All rights reserved.

引用

页码：160 / 164

页数：5

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