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arXiv 2002.12772gr-qcastro-ph.GA
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暗物质中的黑洞与银河系的转动曲线

A Black Hole inside Dark Matter and the Rotation Curves of Galaxies

Fateen Haddad, Nidal Haddad

摘要:

在这篇文章中,我们找到了一个四维度规的大黑洞沉浸在暗物质。具体地说,我们寻找并找到一个静态的球对称黑洞解的爱因斯坦方程,给出了,在牛顿极限,星系的旋转曲线,包括平坦的区域和重子Tully-Fisher关系,并有一个规则的视界。我们还得到了作为这个时空来源的暗物质的能量-动量张量,特别地,它在视界之外的任何地方都满足四个能量条件(主导、弱、零和强)。这个黑洞-暗物质系统代表了一个成功的星系简化模型,为探索暗物质的相对论机制开辟了新的领域,并表明广义相对论理论和暗物质可以解释星系的自转曲线。

英文摘要:

In this article we find a four-dimensional metric for a large black hole immersed in dark matter. Specifically, we look for and find a static spherically symmetric black hole solution to the Einstein equations which gives, in the Newtonian limit, the rotation curves of galaxies, including the flat region and the Baryonic Tully-Fisher relation, and which has a regular horizon. We obtain as well the energy-momentum tensor of the dark matter sourcing this space-time and it turns, in special, to satisfy the four energy conditions (dominant, weak, null, and strong) everywhere outside the horizon. This black-hole-dark-matter system represents a successful simplified model for galaxies, opens a new area for exploring the relativistic regime of dark matter, and shows that the theory of General Relativity together with dark matter can account for the rotation curves of galaxies.

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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