Geodesic deviation, Raychaudhuri equation, and tidal forces in modified gravity with an arbitrary curvature-matter coupling

被引:47
|
作者
Harko, Tiberiu [1 ]
Lobo, Francisco S. N. [2 ]
机构
[1] UCL, Dept Math, London WC1E 6BT, England
[2] Univ Lisbon, Ctr Astron & Astrofis, P-1749016 Lisbon, Portugal
来源
PHYSICAL REVIEW D | 2012年 / 86卷 / 12期
关键词
COSMOLOGICAL CONSTANT; F(R) GRAVITY; DARK ENERGY; ROTATION CURVES; LAGRANGIANS; STABILITY; VIABILITY; UNIVERSE;
D O I
10.1103/PhysRevD.86.124034
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The geodesic deviation equation, describing the relative accelerations of nearby particles, and the Raychaudhury equation, giving the evolution of the kinematical quantities associated with deformations (expansion, shear, and rotation) are considered in the framework of modified theories of gravity with an arbitrary curvature-matter coupling, by taking into account the effects of the extra force. As a physical application of the geodesic deviation equation, the modifications of the tidal forces due to the supplementary curvature-matter coupling are obtained in the weak-field approximation. The tidal motion of test particles is directly influenced not only by the gradient of the extra force, which is basically determined by the gradient of the Ricci scalar, but also by an explicit coupling between the velocity and the Riemann curvature tensor. As a specific example, the expression of the Roche limit (the orbital distance at which a satellite will begin to be tidally torn apart by the body it is orbiting) is also obtained for this class of models. DOI: 10.1103/PhysRevD.86.124034
引用
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页数:10
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