论文标题
非局部重力：太阳系中牛顿重力的修饰
Nonlocal Gravity: Modification of Newtonian Gravitational Force in the Solar System
论文作者
论文摘要
非局部重力（NLG）是爱因斯坦重力理论的经典非局部概括，与培养基的非局部电动力学相似。似乎通用引力相互作用的非局部方面可以模拟暗物质。在NLG的牛顿政权中，我们研究了由于有效的暗物质的存在而导致引力与牛顿反平方法的偏差。特别是，我们算出太阳系中这种偏差的幅度到100个天文单位。此外，我们为NLG的相互核的短距离参数提供了改进的下限。
Nonlocal gravity (NLG) is a classical nonlocal generalization of Einstein's theory of gravitation developed in close analogy with the nonlocal electrodynamics of media. It appears that the nonlocal aspect of the universal gravitational interaction could simulate dark matter. Within the Newtonian regime of NLG, we investigate the deviation of the gravitational force from the Newtonian inverse square law as a consequence of the existence of the effective dark matter. In particular, we work out the magnitude of this deviation in the solar system out to 100 astronomical units. Moreover, we give an improved lower limit for the short-range parameter of the reciprocal kernel of NLG.
