Constraints on axion-like dark matter from a SERF comagnetometer

被引:20
|
作者
Bloch, Itay M. [1 ,2 ]
Shaham, Roy [3 ,4 ]
Hochberg, Yonit [5 ]
Kuflik, Eric [5 ]
Volansky, Tomer [6 ]
Katz, Or [7 ,8 ]
机构
[1] Univ Calif Berkeley, Berkeley Ctr Theoret Phys, Berkeley, CA 94720 USA
[2] Lawrence Berkeley Natl Lab, Theory Grp, Berkeley, CA 94720 USA
[3] Rafael Ltd, IL-31021 Haifa, Israel
[4] Weizmann Inst Sci, Dept Phys Complex Syst, IL-76100 Rehovot, Israel
[5] Hebrew Univ Jerusalem, Racah Inst Phys, IL-91904 Jerusalem, Israel
[6] Tel Aviv Univ, Dept Phys, Tel Aviv, Israel
[7] Duke Univ, Duke Quantum Ctr, Durham, NC 27701 USA
[8] Cornell Univ, Sch Appl & Engn Phys, Ithaca, NY 14853 USA
基金
欧洲研究理事会; 以色列科学基金会;
关键词
SPIN-EXCHANGE; INVARIANCE;
D O I
10.1038/s41467-023-41162-4
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Ultralight axion-like particles are well-motivated relics that might compose the cosmological dark matter and source anomalous time-dependent magnetic fields. We report on terrestrial bounds from the Noble And Alkali Spin Detectors for Ultralight Coherent darK matter (NASDUCK) collaboration on the coupling of axion-like particles to neutrons and protons. The detector uses nuclei of noble-gas and alkali-metal atoms and operates in the Spin-Exchange Relaxation-Free (SERF) regime, achieving high sensitivity to axion-like dark matter fields. Conducting a month-long search, we cover the mass range of 1.4 x 10-12 eV/c2 to 2 x 10-10 eV/c2 and provide limits which supersede robust astrophysical bounds, and improve upon previous terrestrial constraints by over two orders of magnitude for many masses within this range for protons, and up to two orders of magnitude for neutrons. These are the sole reliable terrestrial bounds reported on the coupling of protons with axion-like dark matter, covering an unexplored terrain in its parameter space. Axions are hypothetical particles that constitute leading candidates for the identity of dark matter. Here, the authors improve previous exclusion bounds on axion-like particles in the range of 1.4-200 peV, and report direct terrestrial limits on the coupling of protons and neutrons with axion-like dark matter.
引用
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页数:9
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