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arXiv 1111.4884physics.gen-ph
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量子真空与暗物质

Quantum vacuum and dark matter

Dragan Slavkov Hajdukovic

摘要:

最近,量子真空的引力极化被提出作为暗物质范式的替代方案。在本文中,我们考虑了四个基准测量:星系暗物质晕的中心表面密度的普遍性,在矮球状星系的核心暗物质晕,在旋涡星系的暗盘的不存在和星系团碰撞后的暗物质的分布(子弹星系团是一个著名的例子)。这些现象中只有一部分(但不是全部)可以(原则上)用暗物质和修正引力理论来解释。然而,我们认为,量子真空的引力极化的框架允许理解这些现象的整体。

英文摘要:

Recently, the gravitational polarization of the quantum vacuum was proposed as alternative to the dark matter paradigm. In the present paper we consider four benchmark measurements: the universality of the central surface density of galaxy dark matter haloes, the cored dark matter haloes in dwarf spheroidal galaxies, the non-existence of dark disks in spiral galaxies and distribution of dark matter after collision of clusters of galaxies (the Bullet cluster is a famous example). Only some of these phenomena (but not all of them) can (in principle) be explained by the dark matter and the theories of modified gravity. However, we argue that the framework of the gravitational polarization of the quantum vacuum allows the understanding of the totality of these phenomena.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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