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PhysRevD.100.034501.pdf
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Author
Bazavov, A.Bernard, C.
DeTar, C.
Du, Daping
El-Khadra, A. X.
Freeland, E. D.
Gámiz, E.
Gelzer, Z.
Gottlieb, Steven
Heller, U. M.
Kronfeld, A. S.
Laiho, J.
Liu, Yuzhi
Mackenzie, P. B.
Meurice, Y.
Neil, E. T.
Simone, J. N.
Sugar, R.
Toussaint, D.
Van de Water, R. S.
Zhou, Ran
Affiliation
Univ Arizona, Dept PhysIssue Date
2019-08-01
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AMER PHYSICAL SOCCitation
Lattice, F., Collaborations, M. I. L. C., Bazavov, A., Bernard, C., DeTar, C., Du, D., ... & Gottlieb, S. (2019). B s→ K ℓ ν decay from lattice QCD. Physical Review D, 100(3), 034501.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
We use lattice QCD to calculate the form factors f(+) (q(2)) and f(0) (q(2)) for the semileptonic decay B-s -> Kl nu. Our calculation uses six MILC asqtad 2 + 1 flavor gauge-field ensembles with three lattice spacings. At the smallest and largest lattice spacing the light-quark sea mass is set to 1/10 the strange-quark mass. At the intermediate lattice spacing, we use four values for the light-quark sea mass ranging from 1/5 to 1/20 of the strange-quark mass. We use the asqtad improved staggered action for the light valence quarks, and the clover action with the Fermilab interpolation for the heavy valence bottom quark. We use SU(2) hard-kaon heavy-meson rooted staggered chiral perturbation theory to take the chiral-continuum limit. A functional z expansion is used to extend the form factors to the full kinematic range. We present predictions for the differential decay rate for both Bs -> K mu nu and B-s -> K tau nu. We also present results for the forward-backward asymmetry, the lepton polarization asymmetry, ratios of the scalar and vector form factors for the decays B-s -> Kl nu and B-s -> D(s)l nu. Our results, together with future experimental measurements, can be used to determine the magnitude of the Cabibbo-Kobayashi-Maskawa matrix element vertical bar V-ub vertical bar.Note
Open access articleISSN
2470-0010Version
Final published versionSponsors
Office of Science of the U.S. Department of Energy [DE-AC02-05CH11231]; DOE Office of Science User Facility [DE-AC02-06CH11357]; National Science Foundation [OCI-0725070, ACI-1238993, 0832315, 1615006, ACI-1548562 [90]]; State of Illinois; NSF MRI Grant [CNS-0421498, CNS-0420873, CNS-0420985]; NSF sponsorship of the National Center for Atmospheric Research; IBM Shared University Research (SUR) program; URA Visiting Scholar Award [12-S-15]; U.S. Department of Energy [DE-FG02-91ER40628, DE-FC02-12ER41879, DE-FG02-13ER42001, DE-SC0015655, DE-SC0010120, DE-FG02-91ER40661, DE-SC0010113, DE-SC0010005, DE-FG02-13ER41976]; U.S. National Science Foundation [PHY14-14614, PHY17-19626, PHY14-17805]; MINECO (Spain) [FPA2013-47836-C-1-P, FPA2016-78220-C3-3-P]; Junta de Andalucia(Spain) [FQM-101]; Fermilab Distinguished Scholars program; German Excellence Initiative; European Union [291763]; European Union's Marie Curie COFUND program; United States Department of Energy, Office of Science, Office of High Energy Physics [DE-SC0012704];[DE-AC02-07CH11359]ae974a485f413a2113503eed53cd6c53
10.1103/physrevd.100.034501
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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.