Nonminimal coupling, exponential potentials and the w<-1 regime of dark energy -: art. no. 087302

被引:72
作者
Carvalho, FC
Saa, A
机构
[1] Univ Sao Paulo, Inst Fis, BR-05315970 Sao Paulo, Brazil
[2] Univ Estadual Campinas, IMECC, BR-13083859 Campinas, SP, Brazil
来源
PHYSICAL REVIEW D | 2004年 / 70卷 / 08期
基金
巴西圣保罗研究基金会;
关键词
D O I
10.1103/PhysRevD.70.087302
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Recent observations and theoretical considerations have motivated the study of models for dark energy with equation of state characterized by a parameter w=p/rho<-1. Such models, however, are usually believed to be inviable due to their instabilities against classical perturbations or potentially catastrophic vacuum decays. In this Brief Report, we show that a simple quintessential model with potential V(phi)=Ae(-sigmaphi) and a gravitational coupling of the form (1+|xi|phi(2))R can exhibit, for large sets of initial conditions, asymptotic de Sitter behavior with w<-1 regimes. Nevertheless, the model is indeed stable at classical and quantum level.
引用
收藏
页码:087302 / 1
页数:4
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