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A Lower Bound on Dark Matter Mass
We argue that there is a lower bound of order 10^{-19} eV on dark matter mass if it is produced after inflation via a process with finite correlation length. We rely on nondetection of free-streaming suppression and white-noise enhancement of density perturbations as the observational inputs.
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Published in: | Physical review letters 2024-05, Vol.132 (22), p.221004, Article 221004 |
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Main Authors: | , |
Format: | Article |
Language: | English |
Citations: | Items that this one cites |
Online Access: | Get full text |
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Summary: | We argue that there is a lower bound of order 10^{-19} eV on dark matter mass if it is produced after inflation via a process with finite correlation length. We rely on nondetection of free-streaming suppression and white-noise enhancement of density perturbations as the observational inputs. |
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ISSN: | 0031-9007 1079-7114 1079-7114 |
DOI: | 10.1103/PhysRevLett.132.221004 |