Constraints on the Number of Primordial Black Holes Due to Interaction with Dust
Fuente:
arXiv
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| Auteurs principaux: | , |
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| Format: | Preprint |
| Publié: |
2025
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| _version_ | 1866910989281132544 |
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| author | Melikhov, A. N. Mikheeva, E. V. |
| author_facet | Melikhov, A. N. Mikheeva, E. V. |
| contents | 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 $10^{15}\leq M\leq10^{17}$~g. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2506_04731 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Constraints on the Number of Primordial Black Holes Due to Interaction with Dust Melikhov, A. N. Mikheeva, E. V. Cosmology and Nongalactic Astrophysics 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 $10^{15}\leq M\leq10^{17}$~g. |
| title | Constraints on the Number of Primordial Black Holes Due to Interaction with Dust |
| topic | Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2506.04731 |