Forecasting cosmic doomsday from CMB-LSS cross-correlations

被引:35
作者
Garriga, J
Pogosian, L
Vachaspati, T
机构
[1] Univ Barcelona, Dept Fis Fonamental, Barcelona 08028, Spain
[2] Tufts Univ, Dept Phys & Astron, Inst Cosmol, Medford, MA 02155 USA
[3] Case Western Reserve Univ, Dept Phys, CERCA, Cleveland, OH 44106 USA
来源
PHYSICAL REVIEW D | 2004年 / 69卷 / 06期
关键词
D O I
10.1103/PhysRevD.69.063511
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A broad class of dark energy models, which have been proposed in attempts at solving the cosmological constant problems, predict a late time variation of the equation of state with redshift. The variation occurs as a scalar field picks up speed on its way to negative values of the potential. The negative potential energy eventually turns the expansion into contraction and the local universe undergoes a big crunch. In this paper we show that cross-correlations of the cosmic microwave background anisotropy and matter distribution, in combination with other cosmological data, can be used to forecast the imminence of such cosmic doomsday.
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页数:11
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