Recovering MOND from extended metric theories of gravity

被引:51
作者
Bernal, T. [1 ]
Capozziello, S. [2 ,3 ]
Hidalgo, J. C. [1 ,4 ]
Mendoza, S. [1 ]
机构
[1] Univ Nacl Autonoma Mexico, Inst Astron, Mexico City 04510, DF, Mexico
[2] Univ Naples Federico 2, Dipartimento Sci Fis, I-80126 Naples, Italy
[3] Ist Nazl Fis Nucl, Sez Napoli, I-80126 Naples, Italy
[4] Inst Nacl Invest Nucl, Dept Fis, Mexico City 11801, DF, Mexico
来源
EUROPEAN PHYSICAL JOURNAL C | 2011年 / 71卷 / 11期
关键词
NEWTONIAN DYNAMICS; F(R) GRAVITY; DARK-MATTER; GALAXIES; PHYSICS; ENERGY;
D O I
10.1140/epjc/s10052-011-1794-z
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We show that the Modified Newtonian Dynamics (MOND) regime can be fully recovered as the weak-field limit of a particular theory of gravity formulated in the metric approach. This is possible when Milgrom's acceleration constant is taken as a fundamental quantity which couples to the theory in a very consistent manner. As a consequence, the scale invariance of the gravitational interaction is naturally broken. In this sense, Newtonian gravity is the weakfield limit of general relativity and MOND is the weak-field limit of that particular extended theory of gravity. We also prove that a Noether's symmetry approach to the problem yields a conserved quantity coherent with this relativistic MONDian extension.
引用
收藏
页码:1 / 7
页数:7
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