Frequency-scanning considerations in axionlike dark matter spin-precession experiments
Frequency-scanning considerations in axionlike dark matter spin-precession experiments
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Galactic dark matter may consist of axionlike particles (ALPs) that can be described as an "ultralight bosonic field" oscillating at the ALP Compton frequency. The ALP field can be searched for using nuclear magnetic resonance (NMR), where resonant precession of spins of a polarized sample can be sensitively detected. The ALP mass to which the expe...
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Full title
Frequency-scanning considerations in axionlike dark matter spin-precession experiments
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TN_cdi_proquest_journals_2865941324
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2865941324
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2309.08462
