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arXiv · 2409.14731

Probing Ultralight Primordial Black Hole Dark Matter with XMM Telescopes

Jun Guo·Qiang Yuan·Bin Zhu
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Abstract

Primordial black holes (PBHs), originating from the gravitational collapse of large overdensities in the early Universe, emerge as a compelling dark matter (DM) candidate across a broad mass range. Of particular interest are ultra-light PBHs with masses around $10^{14}$ to $10^{17}$ g, which are typically probed by searching their evaporation products. Using the soft X-ray signal measured by the XMM telescopes, we derive constraints on the fraction of PBHs dark matter with masses in the range $10^{15}$-$10^{16}$ g. We find that observations exclude fraction $f>10^{-6}$ at 95\% C.L. for mass $M_{\rm PBH}=10^{15}$ g.

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Jun Guo, Qiang Yuan, Bin Zhu. 2024-09-23. Probing Ultralight Primordial Black Hole Dark Matter with XMM Telescopes. https://arxiv.org/abs/2409.14731

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