Neutron to mirror-neutron oscillations in the presence of mirror magnetic fields
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology2009Vol. 80(3)
Citations Over TimeTop 17% of 2009 papers
I. Altarev, C.A. Baker, G. Ban, K. Bodek, M. Daum, P. Fierlinger, P. Geltenbort, K. Green, M. G. D. van der Grinten, E. Gutsmiedl, Philip Harris, R. Henneck, M. Horras, P. Iaydjiev, С. Н. Иванов, N. V. Khomutov, K. Kirch, St. Kistryn, A. Knecht, P. Knowles, A. Kozela, F. Kuchler, M. Kuźniak, T. Lauer, B. Lauss, T. Lefort, A. Mtchedlishvili, O. Naviliat-Cuncic, S. Paul, A. S. Pazgalev, J. M. Pendlebury, G. Petzoldt, E. Pierre, C. Plonka-Spehr, G. Qúeḿener, D. Rebreyend, S. Roccia, G. Rogel, N. Severijns, D. Shiers, Yu. Sobolev, R. Stoepler, A. Weis, J. Zejma, J. Zenner, G. Zsigmond
Abstract
We performed ultracold neutron storage measurements to search for additional losses due to neutron ($n$) to mirror-neutron (${n}^{\ensuremath{'}}$) oscillations as a function of an applied magnetic field $B$. In the presence of a mirror magnetic field ${B}^{\ensuremath{'}}$, ultracold neutron losses would be maximal for $B\ensuremath{\approx}{B}^{\ensuremath{'}}$. We did not observe any indication for $n{n}^{\ensuremath{'}}$ oscillations and placed a lower limit on the oscillation time of ${\ensuremath{\tau}}_{n{n}^{\ensuremath{'}}}>12.0\text{ }\text{ }\mathrm{s}$ at 95% C.L. for any ${B}^{\ensuremath{'}}$ between 0 and $12.5\text{ }\text{ }\ensuremath{\mu}\mathrm{T}$.
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