Theory of elastic neutrino-electron scattering

被引：42

作者：

Tomalak, Oleksandr ^{[1
,2
,3
,4
]}

Hill, Richard J. ^{[1
,2
]}

机构：

[1] Univ Kentucky, Dept Phys & Astron, Lexington, KY 40506 USA

[2] Fermilab Natl Accelerator Lab, Theoret Phys Dept, POB 500, Batavia, IL 60510 USA

[3] Johannes Gutenberg Univ Mainz, Inst Kernphys, D-55099 Mainz, Germany

[4] Johannes Gutenberg Univ Mainz, PRISM Cluster Excellence, D-55099 Mainz, Germany

来源：

PHYSICAL REVIEW D | 2020年 / 101卷 / 03期

基金：

美国能源部;

关键词：

RADIATIVE-CORRECTIONS; MAGNETIC-MOMENT; HADRONIC CONTRIBUTIONS; ELECTROMAGNETIC PROPERTIES; HARD BREMSSTRAHLUNG; WEINBERGS MODEL; STANDARD-MODEL; MUON-NEUTRINOS; CROSS-SECTIONS; CHARGE RADIUS;

D O I：

10.1103/PhysRevD.101.033006

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Theoretical predictions for elastic neutrino-electron scattering have no hadronic or nuclear uncertainties at leading order making this process an important tool for normalizing neutrino flux. However, the process is subject to large radiative corrections that differ according to experimental conditions. In this paper, we collect new and existing results for total and differential cross sections accompanied by radiation of one photon, nu e -> nu e(gamma). We perform calculations within the Fermi effective theory and provide analytic expressions for the electron energy spectrum and for the total electromagnetic energy spectrum as well as for double- and triple-differential cross sections with respect to electron energy, electron angle, photon energy, and photon angle. We discuss illustrative applications to accelerator-based neutrino experiments and provide the most precise up-to-date values of neutrino-electron scattering cross sections. We present an analysis of theoretical error, which is dominated by the similar to 0.2%-0.4% uncertainty of the hadronic correction. We also discuss how searches for new physics can be affected by radiative corrections.

引用

页数：36

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