热暗物质、卫星丢失问题和紫外亮度临界值的研究

B. Hoeneisen
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引用次数: 3

摘要

在热暗物质场景中,Press-Schechter形式只对星系质量大于“速度色散截止”有效。在这项工作中,我们将预测扩展到低于速度色散截止的质量,从而解决了“丢失卫星问题”,以及静止帧紫外线亮度截止要求不超过测量的再电离光学深度。我们发现对这两种现象的预测和观察是一致的。作为一个副产品,我们从第一性原理得到了经验的Tully-Fisher关系。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A Study of Warm Dark Matter, the Missing Satellites Problem, and the UV Luminosity Cut-Off
In the warm dark matter scenario, the Press-Schechter formalism is valid only for galaxy masses greater than the"velocity dispersion cut-off". In this work we extend the predictions to masses below the velocity dispersion cut-off, and thereby address the"Missing Satellites Problem", and the rest-frame ultra-violet luminosity cut-off required to not exceed the measured reionization optical depth. We find agreement between predictions and observations of these two phenomena. As a by-product, we obtain the empirical Tully-Fisher relation from first principles.
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