The shape of the beta decay energy distribution is sensitive to the mass of the electron neutrino. Attempts to measure the endpoint shape of tritium decay have so far seen no distortion from the zero-mass form, thus placing an upper limit of m_nu_beta < 2.3 eV. Here we show that a new type of electron energy spectroscopy could improve future measurements of this spectrum and therefore of the neutrino mass. We propose to detect the coherent cyclotron radiation emitted by an energetic electron in a magnetic field. For mildly relativistic electrons, like those in tritium decay, the relativistic shift of the cyclotron frequency allows us to extract the electron energy from the emitted radiation. We present calculations for the energy resolution, noise limits, high-rate measurement capability, and systematic errors expected in such an experiment.
Cryogenic source of atomic tritium for neutrino-mass measurements and precision spectroscopy
University of Turku(图尔库大学);Sorbonne Université(索邦大学);ENS-PSL Université(巴黎文理研究大学);Collège de France(法兰西公学院);Institut Max von Laue - Paul Langevin(马克斯·冯·劳厄-保罗·朗之万研究所);Marietta Blau Institute for Particle Physics, Austrian Academy of Sciences(奥地利科学院玛丽亚·布劳粒子物理研究所);Institute for Particle Physics and Astrophysics, ETH(苏黎世联邦理工学院粒子物理与天体物理研究所);Institute for Astroparticle Physics (IAP), Karlsruhe Institute of Technology (KIT)(卡尔斯鲁厄理工学院亚原子物理研究所)
Beam Energy Measurement using a Bayesian Approach with the Stacked Foil Method
University of Bern(伯尔尼大学);Albert Einstein Center for Fundamental Physics (AEC)(阿尔伯特·爱因斯坦基础物理中心);Laboratory for High Energy Physics (LHEP)(高能物理实验室);Department of Nuclear Medicine, Inselspital, Bern University Hospital(伯尔尼大学医院因塞尔斯皮塔尔核医学科);ARTORG Center for Biomedical Engineering Research(ARTORG生物医学工程研究中心)
Direct determination of the atomic mass difference of the pairs $^{76}$As-$^{76}$Se and $^{155}$Tb-$^{155}$Gd rules out $^{76}$As and $^{155}$Tb as possible candidates for electron (anti)neutrino mass measurements
使用双潘宁阱质谱仪JYFLTRAP进行$β^-$衰变$^{76}$ As $\rightarrow$ $^{76}$ Se和电子捕获衰变$^{155}$ Tb $\rightarrow$ $^{155}$ Gd的基态-基态$Q$值的第一次直接测定。通过相位成像离子回旋共振(PI-ICR)技术测量衰变对的原子质量差,$^{76}$ As $\rightarrow$ $^{76}$ Se和$^{155}$ Tb $\rightarrow$ $^{155}$ Gd的$Q$值分别被确定为2959.265(74)keV和814.94(18)keV。相对于早期的测量,精度分别提高了12倍和57倍。新的$Q$值比最新的2020年原子质量评估中采用的值低1.33 keV和5 keV。利用新确定的基态到基态$Q$值与来自$γ$射线光谱的激发能相结合,基态到激发态跃迁的$Q$值$^{76}$ As(基态)$\rightarrow$ $^{76}$ Se $^*$(2968.4(7)keV)和$^{155}$ Tb(基态)$\rightarrow$ $^{155}$ Gd $^*$(815.731(3)keV)分别为-9.13(70)keV和-0.79(18)keV。因此,我们已经证实,无论是$β^{-}$衰变和EC衰变的候选跃迁是积极禁止在至少4 $σ$的水平,从而明确排除这两种情况下,从潜在的候选人…