Phys. Rev. Lett.
103,
081602
(2009)
[4 pages]
Test of Lorentz Invariance with Spin Precession of Ultracold Neutrons
I. Altarev et al.
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I. Altarev1, C. A. Baker2, G. Ban3, G. Bison4, K. Bodek5, M. Daum6, P. Fierlinger7, P. Geltenbort8, K. Green2,9, M. G. D. van der Grinten2,9, E. Gutsmiedl1, P. G. Harris9, W. Heil10, R. Henneck6, M. Horras7,6, P. Iaydjiev2,*, S. N. Ivanov2,†, N. Khomutov11, K. Kirch6, S. Kistryn5, A. Knecht6,‡, P. Knowles12, A. Kozela13, F. Kuchler7, M. Kuźniak5,6, T. Lauer14, B. Lauss6, T. Lefort3, A. Mtchedlishvili6, O. Naviliat-Cuncic3, A. Pazgalev12, J. M. Pendlebury9, G. Petzoldt6, E. Pierre3,6, G. Pignol15,§, G. Quéméner3, M. Rebetez12, D. Rebreyend15,**, S. Roccia15,††, G. Rogel3,8, N. Severijns16, D. Shiers9, Yu. Sobolev10, A. Weis12, J. Zejma5, and G. Zsigmond6
1Technische Universität München, D–85748 Garching, Germany 2Rutherford Appleton Laboratory, Chilton, Didcot, Oxon OX11 0QX, United Kingdom 3LPC Caen, ENSICAEN, Université de Caen, CNRS/IN2P3, F–14050 Caen, France 4Department of Neurology, Friedrich–Schiller–University, Jena, Germany 5Marian Smoluchowski Institute of Physics, Jagiellonian University, 30–059 Cracow, Poland 6Paul Scherrer Institut (PSI), CH–5232 Villigen PSI, Switzerland 7Excellence Cluster “Universe,” Technische Universität München, D–85748 Garching, Germany 8Institut Laue–Langevin, F–38042 Grenoble Cedex, France 9Department of Physics and Astronomy, University of Sussex, Falmer, Brighton BN1 9QH, United Kingdom 10Institut für Physik, Johannes–Gutenberg–Universität, D–55128 Mainz, Germany 11JINR, 141980 Dubna, Moscow Region, Russia 12University of Fribourg, CH–1700, Fribourg, Switzerland 13Henryk Niedwodniczański Institute for Nuclear Physics, 31–342 Cracow, Poland 14Institut für Kernchemie, Johannes–Gutenberg–Universität, D–55128 Mainz, Germany 15LPSC, Université Joseph Fourier Grenoble 1, CNRS/IN2P3, Institut National Polytechnique de Grenoble 53, F–38026 Grenoble Cedex, France 16Instituut voor Kern–en Stralingsfysica, Katholieke Universiteit Leuven, B–3001 Leuven, Belgium
Received 19 May 2009; published 20 August 2009
A clock comparison experiment, analyzing the ratio of spin precession frequencies of stored ultracold neutrons and 199Hg atoms, is reported. No daily variation of this ratio could be found, from which is set an upper limit on the Lorentz invariance violating cosmic anisotropy field b⊥<2×10-20 eV (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 |gn|<0.3 eV/c2 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 |gn|<3×10-4 eV/c2 m.
© 2009 The American Physical Society
URL:
http://link.aps.org/doi/10.1103/PhysRevLett.103.081602
DOI:
10.1103/PhysRevLett.103.081602
PACS:
11.30.Cp, 04.80.Cc, 11.30.Er, 28.20.−v
*On leave of absence from INRNE, Sofia, Bulgaria †On leave from PNPI, Russia ‡Also at University of Zürich §pignol@lpsc.in2p3.fr **rebreyend@lpsc.in2p3.fr ††roccia@lpsc.in2p3.fr
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