A Lower Bound on Dark Matter Mass

Simple item page
dc.citation.articleNumber221004en_US
dc.citation.issueNumber22en_US
dc.citation.journalTitlePhysical Review Lettersen_US
dc.citation.volumeNumber132en_US
dc.contributor.authorAmin, Mustafa A.en_US
dc.contributor.authorMirbabayi, Mehrdaden_US
dc.date.accessioned2024-08-02T13:32:08Zen_US
dc.date.available2024-08-02T13:32:08Zen_US
dc.date.issued2024en_US
dc.description.abstractWe 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.en_US
dc.identifier.citationAmin, M. A., & Mirbabayi, M. (2024). A Lower Bound on Dark Matter Mass. Physical Review Letters, 132(22), 221004. https://doi.org/10.1103/PhysRevLett.132.221004en_US
dc.identifier.digitalPhysRevLett-132-221004en_US
dc.identifier.doihttps://doi.org/10.1103/PhysRevLett.132.221004en_US
dc.identifier.urihttps://hdl.handle.net/1911/117564en_US
dc.language.isoengen_US
dc.publisherAmerican Physical Societyen_US
dc.rightsExcept where otherwise noted, this work is licensed under a Creative Commons Attribution (CC BY) license.  Permission to reuse, publish, or reproduce the work beyond the terms of the license or beyond the bounds of fair use or other exemptions to copyright law must be obtained from the copyright holder.en_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.titleA Lower Bound on Dark Matter Massen_US
dc.typeJournal articleen_US
dc.type.dcmiTexten_US
dc.type.publicationpublisher versionen_US
Files
Original bundle
Now showing 1 - 1 of 1
Thumbnail Image
Name:
PhysRevLett-132-221004.pdf
Size:
269.15 KB
Format:
Adobe Portable Document Format
Download
Collections
Faculty Publications
Physics and Astronomy Publications