Dark energy: the equation of state description versus scalar-tensor or modified gravity

被引：208

作者：

Capozziello, S

Nojiri, S ^{[1
]}

Odintsov, SD

机构：

[1] Natl Def Acad, Dept Appl Phys, Yokosuka, Kanagawa 2398686, Japan

[2] Univ Naples Federico II, Dipartimento Sci Fisiche, I-80126 Naples, Italy

[3] Compl Univ Monte S Angelo, Sez Napoli, Ist Nazl Fis Nucl, I-80126 Naples, Italy

[4] ICREA, E-08193 Barcelona, Spain

[5] CSIC, Inst Ciencies Espai, IEEC, Fac Ciencies, E-08193 Barcelona, Spain

来源：

PHYSICS LETTERS B | 2006年 / 634卷 / 2-3期

关键词：

D O I：

10.1016/j.physletb.2006.01.065

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Dark energy dynamics of the universe can be achieved by equivalent mathematical descriptions taking into account generalized fluid equations of state in General Relativity, scalar-tensor theories or modified F(R) gravity in Einstein or Jordan frames. The corresponding technique transforming equation of state description to scalar-tensor or modified gravity is explicitly presented. We show that such equivalent pictures can be discriminated by matching solutions with data capable of selecting the true physical frame. (c) 2006 Elsevier B.V. All rights reserved.

引用

页码：93 / 100

页数：8

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[11] A new method for the estimate of H0 from quadruply imaged gravitational lens systems [J].