Test of Lorentz invariance with spin precession of ultracold neutrons
I. Altarev, C. A. Baker, G. Ban, G. Bison, K. Bodek, M. Daum, P., Fierlinger, P. Geltenbort, K. Green, M. G. D. van der Grinten, E. Gutsmiedl,, P. G. Harris, W. Heil, R. Henneck, M. Horras, P. Iaydjiev, S. N. Ivanov, N., Khomutov, K. Kirch, S. Kistryn, A. Knecht, P. Knowles

TL;DR
This study tests Lorentz invariance using ultracold neutrons and mercury atoms, setting new limits on cosmic anisotropy and neutron gravitational dipole moment through spin precession measurements.
Contribution
It provides the first experimental limit on Lorentz invariance violation for free neutrons using ultracold neutron spin precession.
Findings
No daily variation in spin precession ratio detected
Sets an upper limit on Lorentz invariance violating field $b_{ot} < 2 imes 10^{-20} eV$
Establishes a limit on the neutron's gravitational dipole moment $|g_n| < 3 imes 10^{-4} eV/c^2$
Abstract
A clock comparison experiment, analyzing the ratio of spin precession frequencies of stored ultracold neutrons and Hg atoms is reported. %57 No daily variation of this ratio could be found, from which is set an upper limit on the Lorentz invariance violating cosmic anisotropy field (95% C.L.). This is the first limit for the free neutron. This result is also interpreted as a direct limit on the gravitational dipole moment of the neutron eV/ m from a spin-dependent interaction with the Sun. Analyzing the gravitational interaction with the Earth, based on previous data, yields a more stringent limit eV/m.
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