Khronometric Theories of Modified Newtonian Dynamics

被引:2
|
作者
Flanagan, Eanna. E. [1 ]
机构
[1] Cornell Univ, Dept Phys, Ithaca, NY 14853 USA
来源
ASTROPHYSICAL JOURNAL | 2023年 / 958卷 / 02期
关键词
HIDDEN MASS; GRAVITY;
D O I
10.3847/1538-4357/ad003d
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In 2011 Blanchet and Marsat suggested a fully relativistic version of Milgrom's modified Newtonian dynamics in which the dynamical degrees of freedom consist of the spacetime metric and a foliation of spacetime, the khronon field. This theory is simpler than the alternative relativistic formulations. We show that the theory has a consistent nonrelativistic or slow-motion limit. Blanchet and Marsat showed that in the slow motion limit, the theory reproduces stationary solutions of modified Newtonian dynamics. We show that these solutions are stable to khronon perturbations in the low acceleration regime, for the cases of spherical, cylindrical, and planar symmetry. For nonstationary systems in the low acceleration regime, we show that the khronon field generally gives an order unity correction to the modified Newtonian dynamics. In particular, there will be an order unity correction to the MOND version of Kepler's third law, potentially relevant to ongoing efforts to test MOND using GAIA observations of wide binaries.
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页数:7
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