Quantum sensitivity limits of nuclear magnetic resonance experiments searching for new fundamental physics

被引：13

作者：

Aybas, Deniz ^{[1
,2
]}

Bekker, Hendrik ^{[3
]}

Blanchard, John W. ^{[4
]}

Budker, Dmitry ^{[3
,4
,5
]}

Centers, Gary P. ^{[3
,4
]}

Figueroa, Nataniel L. ^{[3
,4
]}

Gramolin, Alexander, V ^{[1
]}

Kimball, Derek F. Jackson ^{[6
]}

Wickenbrock, Arne ^{[3
,4
]}

Sushkov, Alexander O. ^{[1
,2
,7
]}

机构：

[1] Boston Univ, Dept Phys, Boston, MA 02215 USA

[2] Boston Univ, Dept Elect & Comp Engn, Boston, MA 02215 USA

[3] Johannes Gutenberg Univ Mainz, D-55128 Mainz, Germany

[4] GSI Helmholtzzentrum Schwerionenforsch, Helmholtz Inst, D-55128 Mainz, Germany

[5] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[6] Calif State Univ East Bay, Dept Phys, Hayward, CA 94542 USA

[7] Boston Univ, Photon Ctr, Boston, MA 02215 USA

来源：

QUANTUM SCIENCE AND TECHNOLOGY | 2021年 / 6卷 / 03期

基金：

欧洲研究理事会; 美国国家科学基金会;

关键词：

magnetic resonance; spin projection noise; NMR; standard quantum limit; ultra-light dark matter; axion; axion-like dark matter; ELECTRIC-DIPOLE MOMENT; SPIN-NOISE; NMR; SUPPRESSION; SIGNAL; AXION;

D O I：

10.1088/2058-9565/abfbbc

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Nuclear magnetic resonance is a promising experimental approach to search for ultra-light axion-like dark matter. Searches such as the cosmic axion spin-precession experiments (CASPEr) are ultimately limited by quantum-mechanical noise sources, in particular, spin-projection noise. We discuss how such fundamental limits can potentially be reached. We consider a circuit model of a magnetic resonance experiment and quantify three noise sources: spin-projection noise, thermal noise, and amplifier noise. Calculation of the total noise spectrum takes into account the modification of the circuit impedance by the presence of nuclear spins, as well as the circuit back-action on the spin ensemble. Suppression of the circuit back-action is especially important in order for the spin-projection noise limits of searches for axion-like dark matter to reach the quantum chromodynamic axion sensitivity.

引用

页数：13

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