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 10 18 –10 22 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 10 16 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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James M. Cline (2024) studied this question.
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