无质量拓扑缺陷对宇宙学结构的束缚

Richard Lieu
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引用次数: 0

摘要

假设存在球面对称性和弱场,结果表明,如果求解由拓扑缺陷(即形式非常特殊的奇点)引起的泊松方程或爱因斯坦场方程,就会产生一个局部引力场,该引力场能够在没有任何底层质量的薄球壳上驱动测试质量的平直旋转(即在所有半径上以恒定速度运行开普勒圆形轨道)。此外,一个大尺度结构利用这一解决方案,同心组装了许多这样的拓扑缺陷,就能建立一条平坦的恒星或银河旋转曲线,还能以与等势(等温)球相同的方式偏转光线。因此,对暗物质或修正引力理论的需求至少在一定程度上得到了缓解。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The binding of cosmological structures by massless topological defects
Assuming spherical symmetry and weak field, it is shown that if one solves the Poisson equation or the Einstein field equations sourced by a topological defect, i.e. a singularity of a very specific form, the result is a localised gravitational field capable of driving flat rotation (i.e. Keplerian circular orbits at a constant speed for all radii) of test masses on a thin spherical shell without any underlying mass. Moreover, a large-scale structure which exploits this solution by assembling concentrically a number of such topological defects can establish a flat stellar or galactic rotation curve, and can also deflect light in the same manner as an equipotential (isothermal) sphere. Thus the need for dark matter or modified gravity theory is mitigated, at least in part.
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