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arXiv 1706.01434physics.atom-phquant-ph
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惰性气体中的正电子冷却和湮灭

Positron cooling and annihilation in noble gases

D. G. Green

摘要:

了解气体中正电子冷却的动力学,包括幸存到热化的正电子的比例,对于准确解释正电子寿命谱,对于在陷阱和陷阱中开发有效的正电子冷却以及低温冷却,超高能量分辨率,基于陷阱的正电子束至关重要。在这里,正电子冷却和湮没在惰性气体中使用精确的散射和湮没截面计算\emph{ab initio}与多体理论。结果表明,一个惊人的小比例的正电子存活到热化:$\sim$ 0.1在He中,$\sim$ 0在Ne中(由于冷却有效地停滞在相对深的动量转移截面最小值),$\sim$ 0.15在Ar中,$\sim$ 0.05在Kr中和$\sim$ 0.01在Ar中。对于双光子晶体,随时间变化的湮灭率$\bar{Z}_{\rm eff}(τ)$被证明是高度敏感的耗尽的分布由于湮灭,最终解释了长期存在的差异之间的气体电池和陷阱为基础的测量双光子晶体。的\emph{ab initio}计算使第一次同时探测的散射截面和湮灭率的能量依赖性。总的来说,使用精确的原子数据得到的$\bar{Z}_{\rm eff}(τ)$与除Ne以外的所有稀有气体的实验结果非常一致,因为Ne的实验对热化和/或杂质存在时幸存的正电子的分数的了解不完全。

英文摘要:

Understanding the dynamics of positron cooling in gases, including the fraction of positrons surviving to thermalisation, is critical for accurate interpretation of positron lifetime spectra, for the development of efficient positron cooling in traps and accumulators, and for a cryogenically cooled, ultra-high-energy-resolution, trap-based positron beam. Here, positron cooling and annihilation in noble gases is simulated using accurate scattering and annihilation cross sections calculated \emph{ab initio} with many-body theory. It is shown that a strikingly small fraction of positrons survive to thermalisation: $\sim$0.1 in He, $\sim$0 in Ne (due to cooling effectively stalling in the relatively deep momentum-transfer cross-section minimum), $\sim$0.15 in Ar, $\sim$0.05 in Kr and $\sim$0.01 in Xe. For Xe, the time-varying annihilation rate $\bar{Z}_{\rm eff}(τ)$ is shown to be highly sensitive to the depletion of the distribution due to annihilation, conclusively explaining the long-standing discrepancy between gas-cell and trap-based measurements in Xe. The \emph{ab initio} calculations enable the first simultaneous probing of the energy dependence of the the scattering cross section and annihilation rate. Overall, the use of the accurate atomic data gives $\bar{Z}_{\rm eff}(τ)$ in close agreement with experiment for all noble gases except Ne, the experiment for which is proffered to have suffered from incomplete knowledge of the fraction of positrons surviving to thermalisation and/or the presence of impurities.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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