Laboratory Constraints on the Neutron-Spin Coupling of feV-Scale Axions

Ultralight axionlike particles can contribute to the dark matter near the Sun, leading to a distinct, stochastic signature in terrestrial experiments. We search for such particles through their neutron-spin coupling by reanalyzing approximately 40 days of data from a K-^{3}He comagnetometer with a n...

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Main Authors: Junyi Lee, Mariangela Lisanti, William A. Terrano, Michael Romalis
Format: Article
Language:English
Published: American Physical Society 2023-03-01
Series:Physical Review X
Online Access:http://doi.org/10.1103/PhysRevX.13.011050
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author Junyi Lee
Mariangela Lisanti
William A. Terrano
Michael Romalis
author_facet Junyi Lee
Mariangela Lisanti
William A. Terrano
Michael Romalis
author_sort Junyi Lee
collection DOAJ
description Ultralight axionlike particles can contribute to the dark matter near the Sun, leading to a distinct, stochastic signature in terrestrial experiments. We search for such particles through their neutron-spin coupling by reanalyzing approximately 40 days of data from a K-^{3}He comagnetometer with a new frequency-domain likelihood-based formalism that properly accounts for stochastic effects over all axion coherence times relative to the experimental time span. Assuming that axions make up all of the dark matter in the Sun’s vicinity, we find a median 95% upper limit on the neutron-spin coupling of 2.4×10^{-10}  GeV^{-1} for most axion masses from 0.4 to 4 feV, which is about 5 orders of magnitude more stringent than previous laboratory bounds in that mass range. Although several peaks in the experiment’s magnetic power spectrum suggest the rejection of a white-noise null hypothesis, further analysis of their line shapes yields no positive evidence for a dark-matter axion.
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spelling doaj.art-be614d89406044068d41fae4ba972d682023-03-31T16:13:55ZengAmerican Physical SocietyPhysical Review X2160-33082023-03-0113101105010.1103/PhysRevX.13.011050Laboratory Constraints on the Neutron-Spin Coupling of feV-Scale AxionsJunyi LeeMariangela LisantiWilliam A. TerranoMichael RomalisUltralight axionlike particles can contribute to the dark matter near the Sun, leading to a distinct, stochastic signature in terrestrial experiments. We search for such particles through their neutron-spin coupling by reanalyzing approximately 40 days of data from a K-^{3}He comagnetometer with a new frequency-domain likelihood-based formalism that properly accounts for stochastic effects over all axion coherence times relative to the experimental time span. Assuming that axions make up all of the dark matter in the Sun’s vicinity, we find a median 95% upper limit on the neutron-spin coupling of 2.4×10^{-10}  GeV^{-1} for most axion masses from 0.4 to 4 feV, which is about 5 orders of magnitude more stringent than previous laboratory bounds in that mass range. Although several peaks in the experiment’s magnetic power spectrum suggest the rejection of a white-noise null hypothesis, further analysis of their line shapes yields no positive evidence for a dark-matter axion.http://doi.org/10.1103/PhysRevX.13.011050
spellingShingle Junyi Lee
Mariangela Lisanti
William A. Terrano
Michael Romalis
Laboratory Constraints on the Neutron-Spin Coupling of feV-Scale Axions
Physical Review X
title Laboratory Constraints on the Neutron-Spin Coupling of feV-Scale Axions
title_full Laboratory Constraints on the Neutron-Spin Coupling of feV-Scale Axions
title_fullStr Laboratory Constraints on the Neutron-Spin Coupling of feV-Scale Axions
title_full_unstemmed Laboratory Constraints on the Neutron-Spin Coupling of feV-Scale Axions
title_short Laboratory Constraints on the Neutron-Spin Coupling of feV-Scale Axions
title_sort laboratory constraints on the neutron spin coupling of fev scale axions
url http://doi.org/10.1103/PhysRevX.13.011050
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