论文标题
部分可观测时空混沌系统的无模型预测
Deconstructing experimental decay energy spectra: the $^{26}$O case
论文作者
论文摘要
在核反应实验中,测得的衰减能光谱可以洞悉衰减系统的壳结构。但是,由于检测器的分辨率和接受效应,从测量中提取基本物理学是具有挑战性的。 Richardson-Lucy(RL)算法是一种过度的方法,通常用于光学元件,已证明是恢复图像的成功技术,已应用于我们的实验性核物理数据。该方法的唯一输入是观察到的能量谱,而检测器的响应矩阵也称为转移矩阵。我们证明,该技术可以帮助从测量的衰减能谱中访问有关粒子无量系统的壳结构的信息,这些衰减能谱无法通过传统方法(例如卡方拟合)立即访问。出于类似的目的,我们开发了一种机器学习模型,该模型使用深神网络(DNN)分类器从测得的衰减能谱中识别共振状态。我们测试了两种方法在模拟数据和实验测量方面的性能。然后,我们将这两种算法应用于$ ^{26} \ Mathrm {O} \ rightArrow ^{24} \ Mathrm {O} $ + N + N的衰减能谱。使用RL算法恢复共振状态,以消除测得的衰减能谱与DNN分类器发现的衰减能谱。 DeBlurring和DNN方法都表明,$^{26} \ Mathrm {O} $的原始衰减能谱显示出三个峰值约为0.15〜MEV,1.50〜MEV和5.00 MEV,半脚别为0.29〜MEV,0.80 〜MEV,0.80〜MEV,和1.85 mev,和1.85〜mev,和1.85〜mev,和1.85〜mev。
In nuclear reaction experiments, the measured decay energy spectra can give insights into the shell structure of decaying systems. However, extracting the underlying physics from the measurements is challenging due to detector resolution and acceptance effects. The Richardson-Lucy (RL) algorithm, a deblurring method that is commonly used in optics and has proven to be a successful technique for restoring images, was applied to our experimental nuclear physics data. The only inputs to the method are the observed energy spectrum and the detector's response matrix also known as the transfer matrix. We demonstrate that the technique can help access information about the shell structure of particle-unbound systems from the measured decay energy spectrum that isn't immediately accessible via traditional approaches such as chi-square fitting. For a similar purpose, we developed a machine learning model that uses a deep neural network (DNN) classifier to identify resonance states from the measured decay energy spectrum. We tested the performance of both methods on simulated data and experimental measurements. Then, we applied both algorithms to the decay energy spectrum of $^{26}\mathrm{O} \rightarrow ^{24}\mathrm{O}$ + n + n measured via invariant mass spectroscopy. The resonance states restored using the RL algorithm to deblur the measured decay energy spectrum agree with those found by the DNN classifier. Both deblurring and DNN approaches suggest that the raw decay energy spectrum of $^{26}\mathrm{O}$ exhibits three peaks at approximately 0.15~MeV, 1.50~MeV, and 5.00~MeV, with half-widths of 0.29~MeV, 0.80~MeV, and 1.85~MeV, respectively.