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PhysRevD.99.114509.pdf
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Author
Bazavov, A.Bernard, C.
DeTar, C.
Du, Daping
El-Khadra, A. X.
Freeland, E. D.
Gámiz, E.
Gottlieb, Steven
Heller, U. M.
Komijani, J.
Kronfeld, A. S.
Laiho, J.
Mackenzie, P. B.
Neil, E. T.
Primer, T.
Simone, J. N.
Sugar, R.
Toussaint, D.
Van de Water, R. S.
Affiliation
Univ Arizona, Dept PhysIssue Date
2019-06-24
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American Physical Society (APS)Citation
Lattice, F., Collaborations, M. I. L. C., Bazavov, A., Bernard, C., DeTar, C., Du, D., ... & Heller, U. M. (2019). | V u s| from K ℓ 3 decay and four-flavor lattice QCD. Physical Review D, 99(11), 114509.Journal
Physical Review DRights
Copyright © The Author(s). Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
Using highly improved staggered quark (HISQ) Nf=2+1+1 MILC ensembles with five different values of the lattice spacing, including four ensembles with physical quark masses, we perform the most precise computation to date of the K→πℓν vector form factor at zero momentum transfer, fK0π−+(0)=0.9696(15)stat(12)syst. This is the first calculation that includes the dominant finite-volume effects, as calculated in chiral perturbation theory at next-to-leading order. Our result for the form factor provides a direct determination of the Cabibbo-Kobayashi-Maskawa (CKM) matrix element |Vus|=0.22333(44)f+(0)(42)exp, with a theory error that is, for the first time, at the same level as the experimental error. The uncertainty of the semileptonic determination is now similar to that from leptonic decays and the ratio fK+/fπ+, which uses |Vud| as input. Our value of |Vus| is in tension at the 2–2.6σ level both with the determinations from leptonic decays and with the unitarity of the CKM matrix. In the test of CKM unitarity in the first row, the current limiting factor is the error in |Vud|, although a recent determination of the nucleus-independent radiative corrections to superallowed nuclear β decays could reduce the |Vud|2 uncertainty nearly to that of |Vus|2. Alternative unitarity tests using only kaon decays, for which improvements in the theory and experimental inputs are likely in the next few years, reveal similar tensions and could be further improved by taking correlations between the theory inputs. As part of our analysis, we calculated the correction to fKπ+(0) due to nonequilibrated topological charge at leading order in chiral perturbation theory, for both the full-QCD and the partially quenched cases. We also obtain the combination of low-energy constants in the chiral effective Lagrangian [Cr12+Cr34−(Lr5)2](Mρ)=(2.92±0.31)×10−6.ISSN
2470-0010Version
Final published versionSponsors
Office of Science of the U.S. Department of Energy [DE-AC02-05CH11231]; Department of Energy Office of Science User Facility [DE-AC02-06CH11357]; National Science Foundation [OCI-0725070, ACI-1238993, 0832315, 1615006, ACI-1548562 [161]]; State of Illinois; NSF [TG-MCA93S002]; NSF MRI [CNS-0421498, CNS-0420873, CNS-0420985]; NSF sponsorship of the National Center for Atmospheric Research; University of Colorado; IBM Shared University Research (SUR) program; U.S. Department of Energy [DE-FG02-91ER40628, DE-FC02-12ER41879, DE-SC0010120, DE-FG02-91ER40661, DE-FG02-13ER42001, DE-SC0015655, DE-SC0010005, DE-FG02-13ER41976]; U.S. National Science Foundation [PHY14-14614, PHY 17-19626, PHY14-17805, PHY13-16748, PHY16-20625]; MINECO (Spain) [FPA2013-47836-C-1-P, FPA2016-78220-C3-3-P]; Junta de Andalucia (Spain) [FQM-101]; European Commission (EC) [PCIG10-GA-2011-303781]; U.K. Science and Technology Facilities Council; German Excellence Initiative; European Union [291763]; European Union Marie Curie COFUND program; United States Department of Energy. Office of Science, Office of High Energy Physics [DE-SC0012704]; United States Department of Energy. Office of Science. Office of High Energy Physics [DE-AC02-07CH11359]ae974a485f413a2113503eed53cd6c53
10.1103/physrevd.99.114509
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Except where otherwise noted, this item's license is described as Copyright © The Author(s). Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license.