期刊
PHYSICAL REVIEW D
卷 103, 期 11, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.103.113007
关键词
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资金
- Austrian Fonds zur Forderung der Wissenschaftlichen Forschung (FWF) [P31702-N27, P26636-N20]
- Deutsche Forderungsgemeinschaft (DFG) [AB 128/5-2]
- Deutsche Forschungsgemeinschaft [SFB/TR 55]
- MA 23
This study investigates the contributions of the hadronic structure of the neutron to radiative corrections in neutron beta decay, showing that after renormalization, the corrections are on the order of a few parts of 10(-5)-10(-4). The calculated results align well with previous research findings, indicating the reliability of the approach used.
We investigate the contributions of the hadronic structure of the neutron to radiative O(alpha E-e/m(N)) corrections [or the inner O(alpha E-e/m(N)) RC] to the neutron beta decay, where alpha, E-e, and m(N) are the fine-structure constant, the electron energy, and the nucleon mass, respectively. We perform the calculation within the effective quantum field theory of strong low-energy pion-nucleon interactions described by the linear sigma model with chiral SU(2) x SU(2) symmetry and electroweak hadron-hadron, hadron-lepton, and lepton-lepton interactions for the electron-lepton family with SU(2)(L) x U(1)(Y) symmetry of the standard electroweak theory [Ivanov et al., Phys. Rev. D 99, 093006 (2019)]. We show that after renormalization, carried out in accordance with Sirlin's prescription [Sirlin, Phys. Rev. 164, 1767 (1967)], the inner O(alpha E-e/m(N)) RC are of the order of a few parts of 10(-5)-10(-4). This agrees well with the results obtained in [Ivanov et al., Phys. Rev. D 99, 093006 (2019)].
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