Asymptotically Lifshitz black hole solutions in F(R) gravity

被引：21

作者：

Hendi, S. H. ^{[1
,2
,3
]}

Panah, B. Eslam ^{[4
,5
]}

Corda, C. ^{[6
,7
,8
,9
]}

机构：

[1] Shiraz Univ, Coll Sci, Dept Phys, Shiraz 71454, Iran

[2] Shiraz Univ, Coll Sci, Biruni Observ, Shiraz 71454, Iran

[3] Res Inst Astrophys & Astron Maragha, Maragha, Iran

[4] Univ Tabriz, Dept Phys, Tabriz 51664, Iran

[5] Islamic Azad Univ, Talesh Brach, Young Res Club, Talesh, Iran

[6] Inst Theoret Phys & Adv Math, I-59100 Prato, Italy

[7] Ist Univ Ric Santa Rita, I-50133 Florence, Italy

[8] Int Inst Applicable Math & Informat Sci, Hyderabad, Andhra Pradesh, India

[9] Int Inst Applicable Math & Informat Sci, Udine, Italy

来源：

CANADIAN JOURNAL OF PHYSICS | 2014年 / 92卷 / 01期

关键词：

DARK ENERGY; GRAVITATIONAL-WAVES; WEAK MODIFICATION; ROTATION CURVES; FIELD-EQUATIONS; BRANES; SPACE; UNIVERSE; TENSOR;

D O I：

10.1139/cjp-2013-0357

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We consider a class of spherically symmetric space-time to obtain some interesting solutions in F(R) gravity without matter field (pure gravity). We investigate the geometry of the solutions and find that there is an essential singularity at the origin. In addition, we show that there is an analogy between obtained solutions with the black holes of Einstein-Delta-power Maxwell invariant theory. Furthermore, we find that these solutions are equivalent to the asymptotically Lifshitz black holes. Also, we calculate d(2)F/dR(2) to examine the Dolgov-Kawasaki stability criterion.

引用

页码：76 / 81

页数：6

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