论文标题

改良的爱因斯坦与深色物质改良的Euler

Modified Einstein versus Modified Euler for Dark Matter

论文作者

Bonvin, Camille, Pogosian, Levon

论文摘要

一般相对论的修改通常包含额外的自由度,可以介导物质颗粒之间的力。第五力在替代重力理论​​中的常见表现之一是相对论和非偏见颗粒所感受到的重力之间的差异,也称为“重力滑移”。相比之下,由于暗区域相互作用,暗物质颗粒之间的第五力不会引起重力滑动,使后者成为可能具有改性重力的吸烟枪。在本文中,我们指出,像耦合的典型模型一样,作用于暗物质颗粒的力也将表现为对大规模结构的宇宙学调查对有效重力滑移的测量。这与以下事实有关:如果星系的特殊运动引起的红移空间变形,如果暗物质受到第五力的影响,则不会提供对真正的重力电位的测量。因此,仅用宇宙学数据将黑暗扇区相互作用与重力的修饰区分开是极具挑战性的。通过直接测量时间的扭曲,对星系调查的重力红移的未来观察可以帮助打破这些可能性之间的堕落。我们讨论了解决这个重要问题的其他可能方法。

Modifications of General Relativity generically contain additional degrees of freedom that can mediate forces between matter particles. One of the common manifestations of a fifth force in alternative gravity theories is a difference between the gravitational potentials felt by relativistic and non-relativistic particles, also known as "the gravitational slip". In contrast, a fifth force between dark matter particles, due to dark sector interaction, does not cause a gravitational slip, making the latter a possible smoking gun of modified gravity. In this article, we point out that a force acting on dark matter particles, as in models of coupled quintessence, would also manifest itself as a measurement of an effective gravitational slip by cosmological surveys of large-scale structure. This is linked to the fact that redshift-space distortions due to peculiar motion of galaxies do not provide a measurement of the true gravitational potential if dark matter is affected by a fifth force. Hence, it is extremely challenging to distinguish a dark sector interaction from a modification of gravity with cosmological data alone. Future observations of gravitational redshift from galaxy surveys can help to break the degeneracy between these possibilities, by providing a direct measurement of the distortion of time. We discuss this and other possible ways to resolve this important question.

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