Journal
PHYSICAL REVIEW LETTERS
Volume 121, Issue 24, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.121.241804
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Funding
- Deutsche Forschungsgemeinschaft [GO 2604/2-1]
- National Natural Science Foundation of China (NSFC) [11575110, 11655002, 11735010]
- Natural Science Foundation of Shanghai [15DZ2272100, 15ZR1423100]
- Shanghai Key Laboratory for Particle Physics and Cosmology
- Key Laboratory for Particle Physics, Astrophysics and Cosmology, Ministry of Education
- Recruitment Program of Foreign Young Talents from the State Administration of Foreign Expert Affairs, China
- US Department of Energy [DE-SC0011095]
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We analyze the universal radiative correction Delta(V)(R) to neutron and superallowed nuclear beta decay by expressing the hadronic gamma W-box contribution in terms of a dispersion relation, which we identify as an integral over the first Nachtmann moment of the gamma W interference structure function F-3((0)). By connecting the needed input to existing data on neutrino and antineutrino scattering, we obtain an updated value of Delta(V)(R) = 0.02467(22), wherein the hadronic uncertainty is reduced. Assuming other standard model theoretical calculations and experimental measurements remain unchanged, we obtain an updated value of vertical bar V-ud vertical bar = 0.97370(14), raising tension with the first row Cabibbo-Kobayashi-Maskawa unitarity constraint. We comment on ways current and future experiments can provide input to our dispersive analysis.
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