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arXiv · 1711.08999

Overview of the Cosmic Axion Spin Precession Experiment (CASPEr)

D. F. Jackson Kimball·S. Afach·D. Aybas·J. W. Blanchard·D. Budker·G. Centers·M. Engler·N. L. Figueroa·A. Garcon·P. W. Graham·H. Luo·S. Rajendran·M. G. Sendra·A. O. Sushkov·T. Wang·A. Wickenbrock·A. Wilzewski·T. Wu
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Abstract

An overview of our experimental program to search for axion and axion-like-particle (ALP) dark matter using nuclear magnetic resonance (NMR) techniques is presented. An oscillating axion field can exert a time-varying torque on nuclear spins either directly or via generation of an oscillating nuclear electric dipole moment (EDM). Magnetic resonance techniques can be used to detect such an effect. The first-stage experiments explore many decades of ALP parameter space beyond the current astrophysical and laboratory bounds. It is anticipated that future versions of the experiments will be sensitive to the axions associated with quantum chromodynamics (QCD) having masses $\lesssim 10^{-9}~{\rm eV}/c^2$.

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D. F. Jackson Kimball, S. Afach, D. Aybas, J. W. Blanchard, D. Budker, G. Centers, M. Engler, N. L. Figueroa, A. Garcon, P. W. Graham, H. Luo, S. Rajendran, M. G. Sendra, A. O. Sushkov, T. Wang, A. Wickenbrock, A. Wilzewski, T. Wu. 2018-10-31. Overview of the Cosmic Axion Spin Precession Experiment (CASPEr). https://arxiv.org/abs/1711.08999

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