论文标题

搜索中子镜中的中子振荡

A search for neutron to mirror-neutron oscillations

论文作者

Abel, C., Ayres, N. J., Ban, G., Bison, G., Bodek, K., Bondar, V., Chanel, E., Chiu, P. -J., Crawford, C., Daum, M., Dinani, R. T., Emmenegger, S., Flaux, P., Ferraris-Bouchez, L., Griffith, W. C., Grujic, Z. D., Hild, N., Kirch, K., Koch, H. -C., Koss, P. A., Kozela, A., Krempel, J., Lauss, B., Lefort, T., Leredde, A., Mohanmurthy, P., Naviliat-Cuncic, O., Pais, D., Piegsa, F. M., Pignol, G., Rawlik, M., Rebreyend, D., Rienaecker, I., Ries, D., Roccia, S., Rozpedzik, D., Schmidt-Wellenburg, P., Severijns, N., Thorne, J., Weis, A., Wursten, E., Zejma, J., Zsigmond, G.

论文摘要

已经提出,标准模型粒子可能会有一个镜像副本,从而在全球级别的弱相互作用中恢复了奇偶校验对称性。中性标准模型粒子(例如中子)及其镜子对应物之间的振荡可能会回答当今物理学的各种常规问题。由超速中子储存测量结果领导的天体物理研究和陆地实验已经研究了中子对镜像中的振荡,并对理论参数施加了约束。最近,对这些超速中子存储实验的进一步分析产生了具有统计学意义的异常信号,这些信号可以解释为假设非零镜面磁场,可以将其解释为镜像中的振荡。中子电偶极时刻的合作在保罗·舍雷学院(Paul Scherrer Institute)进行了专门的搜索,但没有发现对镜像中振荡的中子证据。因此,获得了以下新的振荡时间下限:$τ_{nn'}> 352〜 $ s at $ b'= 0 $(95%c.l.),$τ_{nn'}> 6〜 \ 6〜 \ text {s} $ for $ 0.4〜μ \ text $ 0.4〜μ \文本{ c.l.)和$τ_{nn'}/\ sqrt {\cosβ}> 9〜 \ text {s} $ for las $ 5.0〜μ \ text {t} <t} <b'<b'<25.4〜μ \ text {t} $ c.l.(95%c.l. 地球。这些新约束是迄今为止最佳测量的$ b'\ sim10〜μ $ t,$ b'\ sim20〜μ $ t。

It has been proposed that there could be a mirror copy of the standard model particles, restoring the parity symmetry in the weak interaction on the global level. Oscillations between a neutral standard model particle, such as the neutron, and its mirror counterpart could potentially answer various standing issues in physics today. Astrophysical studies and terrestrial experiments led by ultracold neutron storage measurements have investigated neutron to mirror-neutron oscillations and imposed constraints on the theoretical parameters. Recently, further analysis of these ultracold neutron storage experiments has yielded statistically significant anomalous signals that may be interpreted as neutron to mirror-neutron oscillations, assuming nonzero mirror magnetic fields. The neutron electric dipole moment collaboration performed a dedicated search at the Paul Scherrer Institute and found no evidence of neutron to mirror-neutron oscillations. Thereby, the following new lower limits on the oscillation time were obtained: $τ_{nn'} > 352~$s at $B'=0$ (95% C.L.), $τ_{nn'} > 6~\text{s}$ for all $0.4~μ\text{T}<B'<25.7~μ\text{T}$ (95% C.L.), and $τ_{nn'}/\sqrt{\cosβ}>9~\text{s}$ for all $5.0~μ\text{T}<B'<25.4~μ\text{T}$ (95% C.L.), where $β$ is the fixed angle between the applied magnetic field and the local mirror magnetic field which is assumed to be bound to the Earth. These new constraints are the best measured so far around $B'\sim10~μ$T, and $B'\sim20~μ$T.

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