Quantum statistical modified entropic gravity as a theoretical basis for MOND

被引:22
|
作者
Pazy, Ehoud [1 ]
机构
[1] Univ Connecticut, Dept Phys, Storrs, CT 06269 USA
来源
PHYSICAL REVIEW D | 2013年 / 87卷 / 08期
关键词
NEWTONIAN DYNAMICS; SPACETIME; ENERGY;
D O I
10.1103/PhysRevD.87.084063
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Considering the quantum statistics of the degrees of freedom on the holographic screen, it is shown that the ratio of the number of excited bulk degrees of freedom to the number of excited surface degrees of freedom is given by the modified Newtonian dynamics (MOND) interpolating function (mu) over bar. This relationship is shown to hold also in aquadratic Lagrangian theory and in the extension of MOND to de Sitter space. Based on the relationship between the entropy and the number of degrees of freedom on the holographic screen, a simple expression, relating the MOND interpolating function to the ratio of the two-dimensional entropy to Bekenstein-Hawking entropy, is obtained. In terms of this expression MOND can be viewed as a modification of gravity arising due to a bound on the maximum entropy for the holographic screen. DOI: 10.1103/PhysRevD.87.084063
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页数:8
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