关于 "根据太阳系星历排除作为暗物质的原始黑洞 "的评论

James M. Cline
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引用次数: 0

摘要

最近有人声称(https://arxiv.org/pdf/2408.10799),太阳系星历数据可以排除质量范围在1018-1022 g的原始黑洞(PBH)暗物质。我的研究表明,这一结论是基于一个难以置信的隐含假设:即太阳系质量在 50 au 范围内的不确定性与太阳质量的不确定性一样小。修正这一误差后,我发现星历表数据只能约束质量低于1016 g的PBH,而通过霍金辐射对其蒸发的约束已经排除了这一质量。修正有关这种波动的时间平均速率的进一步误差,甚至会使这种较弱的约束失效。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Comment on “Excluding Primordial Black Holes as Dark Matter Based on Solar System Ephemeris”
It was recently claimed (https://arxiv.org/pdf/2408.10799) that solar system ephemeris data can exclude primordial black hole (PBH) dark matter in the mass range 1018–1022 g. I show that this conclusion is based on an implausible, implicit assumption; namely the uncertainty on the solar system mass within 50 au is as small as the uncertainty on the mass of the Sun. Correcting for this error, I find that ephemeris data can only constrain PBH’s with mass below 1016 g, which is already excluded by constraints on their evaporation via Hawking radiation. Correcting a further error concerning the time-averaged rate of such fluctuations nullifies even this weaker constraint.
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