Abstract
Photons emitted by primordial black holes (PBHs) due to the Hawking effect are among the factors of interstellar dust heating. Based on the data on the temperature of dust, constraints on the fraction of PBHs in the dark matter were found for various distributions of PBHs with masses \({{10}^{{15}}} \leqslant M \leqslant {{10}^{{17}}}\) g.
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ACKNOWLEDGMENTS
The authors thank V.N. Lukash and P.B. Ivanov for the review of the paper and their remarks, as well as the referee for comments and suggestions.
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The study was supported by the Russian Foundation for Basic Research, grant no. 19-02-00199.
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Translated by M. Chubarova
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Melikhov, A.N., Mikheeva, E.V. Constraints on the Number of Primordial Black Holes Due to Interaction with Dust. Astron. Rep. 66, 387–392 (2022). https://doi.org/10.1134/S1063772922050043
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DOI: https://doi.org/10.1134/S1063772922050043