Unifying Einstein and Palatini gravities

被引:54
作者
Amendola, Luca [1 ]
Enqvist, Kari [2 ,3 ]
Koivisto, Tomi [4 ,5 ]
机构
[1] Heidelberg Univ, Inst Theoret Phys, D-69120 Heidelberg, Germany
[2] Univ Helsinki, Dept Phys, FIN-00014 Helsinki, Finland
[3] Univ Helsinki, Helsinki Inst Phys, FIN-00014 Helsinki, Finland
[4] Inst Theoret Phys, NL-3584 CE Utrecht, Netherlands
[5] Spinoza Inst, NL-3584 CE Utrecht, Netherlands
来源
PHYSICAL REVIEW D | 2011年 / 83卷 / 04期
基金
芬兰科学院;
关键词
DARK ENERGY; EQUIVALENCE; FORMULATION;
D O I
10.1103/PhysRevD.83.044016
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider a novel class of f(R) gravity theories where the connection is related to the conformally scaled metric (g) over cap (mu nu) = C(R)g(mu nu) with a scaling that depends on the scalar curvature R only. We call them C theories and show that the Einstein and Palatini gravities can be obtained as special limits. In addition, C theories include completely new physically distinct gravity theories even when f(R) = R. With nonlinear f(R), C theories interpolate and extrapolate the Einstein and Palatini cases and may avoid some of their conceptual and observational problems. We further show that C theories have a scalar-tensor formulation, which in some special cases reduces to simple Brans-Dicke-type gravity. If matter fields couple to the connection, the conservation laws in C theories are modified. The stability of perturbations about flat space is determined by a simple condition on the Lagrangian.
引用
收藏
页数:14
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