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arXiv 2405.20060hep-phnucl-th
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相干弹性中微子-核散射的详细核结构计算

Detailed nuclear structure calculations for coherent elastic neutrino-nucleus scattering

Raghda Abdel Khaleq, Jayden L. Newstead, Cedric Simenel, Andrew E. Stuchbery

AI总结:

为提升CEvNS实验对新物理的探测能力,本文基于强子流一致理论结合核壳模型计算核形状因子,优化标准模型预测,使不确定性降低最多10倍,增强了实验灵敏度。

摘要:

中微子领域任何“新物理”的发现首先都需要对标准模型预期截面进行精确预测。当前相干弹性中微子-核散射(CEvNS)实验受统计量限制,但随着现有及未来实验规模扩大,需改进理论预测。本文回顾了强子流一致理论中CEvNS截面的计算,并用核壳模型计算相关核形状因子;通过采用不同壳模型相互作用重复计算,结合Skyme-Hartree-Fock评估弱电荷半径,探索形状因子的不确定性;随后优化了COHERENT实验近期结果的标准模型预测,发现截面与先前预测一致,但不确定性显著降低(最多达10倍)。近未来CEvNS实验将通过提升对新物理信号的灵敏度,从改进的预测中显著获益。

英文摘要:

Any discovery of `new physics' in the neutrino sector first requires a precise prediction of the expected Standard Model cross section. Currently, Coherent Elastic neutrino-Nucleus Scattering (CEvNS) experiments are statistics limited. However, as new and future experiments scale up, it will be necessary to improve the theoretical predictions. Here we review the calculation of the CEvNS cross section in a consistent theory of hadronic currents and compute the relevant nuclear form factors using the nuclear shell model. The uncertainty on the form factors is explored by repeating the calculation for various shell model interactions and with Skyme-Hartree-Fock evaluations of the Weak-charge radii. We then refine the Standard Model predictions for the recent experimental results of the COHERENT experiment. We find that our cross sections are in good agreement with previous predictions, but with significantly smaller uncertainties - by up to a factor of 10. Near-future CEvNS experiments will meaningfully benefit from improved predictions through an increased sensitivity to new-physics signals.

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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