Superquintessence

被引:191
作者
Faraoni, V
机构
[1] Univ No British Columbia, Dept Phys, Prince George, BC V2N 4Z9, Canada
[2] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Roma, Italy
来源
INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2002年 / 11卷 / 04期
关键词
D O I
10.1142/S0218271802001809
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
There is marginal evidence that the quintessential form of matter responsible for the acceleration of the universe observed today has ratio between pressure and energy density w < -1. Such a regime, called superacceleration, cannot be achieved with conventional scalar field models. The simplest nonexotic model achieving superacceleration is that of a scalar field nonminimally coupled to the Ricci curvature. This model is studied for general potentials and an exact superaccelerating solution is presented. In quintessential inflation, the model can have blue gravitational wave spectra, improving the prospects for the detection of cosmological gravitational waves.
引用
收藏
页码:471 / 481
页数:11
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