Hawking Radiation from non-evaporating primordial black holes cannot enable the formation of direct collapse black holes
The formation of supermassive black holes (SMBHs) in the early Universe is a subject of significant debate. In this study, we examine whether non-evaporating primordial black holes (PBHs) can offer a solution. We establish initial constraints on the range of PBH masses that correspond to Hawking rad...
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| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
Maynooth Academic Publishing
2025-03-01
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| Series: | The Open Journal of Astrophysics |
| Online Access: | https://doi.org/10.33232/001c.132347 |
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