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Comagnetometer probes of dark matter and new physics

Author(s): Terrano, WA; Romalis, MV

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dc.contributor.authorTerrano, WA-
dc.contributor.authorRomalis, MV-
dc.date.accessioned2024-03-12T00:53:45Z-
dc.date.available2024-03-12T00:53:45Z-
dc.date.issued2021-11-05en_US
dc.identifier.citationTerrano, WA, Romalis, MV. (2022). Comagnetometer probes of dark matter and new physics. Quantum Science and Technology, 7 (1), 014001 - 014001. doi:10.1088/2058-9565/ac1ae0en_US
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr1r49g91p-
dc.description.abstractModern comagnetometry is—in absolute energy units—the most sensitive experimental technique for measuring the energy splitting between quantum states, with certain implementations measuring the nuclear spin-up/spin-down splitting at the 10−26 eV level. By measuring and subtracting the leading magnetic effects on the spins, comagnetometry can be used to study non-standard-model spin interactions. New physics scenarios that comagnetometers can probe include EDMs, violations of Lorentz invariance, Goldstone bosons from new high-energy symmetries, spin-dependent and CP-violating long-range forces, and axionic dark matter. We describe the many implementations that have been developed and optimized for these applications, and consider the prospects for improvements in the technique. Based purely on existing technology, there is room for several orders of magnitude in further improvement in statistical sensitivity. We also evaluate sources of systematic error and instability that may limit attainable improvements.en_US
dc.language.isoen_USen_US
dc.relation.ispartofQuantum Science and Technologyen_US
dc.rightsAuthor's manuscripten_US
dc.titleComagnetometer probes of dark matter and new physicsen_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1088/2058-9565/ac1ae0-
dc.identifier.eissn2058-9565-
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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