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Determination of |Vus| from a Lattice QCD Calculation of the Kπν Semileptonic Form Factor with Physical Quark Masses

A. Bazavov, C. Bernard, C. M. Bouchard, C. DeTar, Daping Du, A. X. El-Khadra, J. Foley, E. D. Freeland, E. Gámiz, Steven Gottlieb, U. M. Heller, Jongjeong Kim, A. S. Kronfeld, J. Laiho, L. Levkova, P. B. Mackenzie, E. T. Neil, M. B. Oktay, Si-Wei Qiu, J. N. Simone, R. Sugar, D. Toussaint, R. S. Van de Water, and Ran Zhou (Fermilab Lattice and MILC Collaborations)
Phys. Rev. Lett. 112, 112001 – Published 17 March 2014

Abstract

We calculate the kaon semileptonic form factor f+(0) from lattice QCD, working, for the first time, at the physical light-quark masses. We use gauge configurations generated by the MILC Collaboration with Nf=2+1+1 flavors of sea quarks, which incorporate the effects of dynamical charm quarks as well as those of up, down, and strange. We employ data at three lattice spacings to extrapolate to the continuum limit. Our result, f+(0)=0.9704(32), where the error is the total statistical plus systematic uncertainty added in quadrature, is the most precise determination to date. Combining our result with the latest experimental measurements of K semileptonic decays, one obtains the Cabibbo-Kobayashi-Maskawa matrix element |Vus|=0.22290(74)(52), where the first error is from f+(0) and the second one is from experiment. In the first-row test of Cabibbo-Kobayashi-Maskawa unitarity, the error stemming from |Vus| is now comparable to that from |Vud|.

  • Figure
  • Received 5 December 2013

DOI:https://doi.org/10.1103/PhysRevLett.112.112001

© 2014 American Physical Society

Authors & Affiliations

A. Bazavov1,2, C. Bernard3, C. M. Bouchard4, C. DeTar5, Daping Du6, A. X. El-Khadra6,7, J. Foley5, E. D. Freeland8, E. Gámiz9,*, Steven Gottlieb10, U. M. Heller11, Jongjeong Kim12, A. S. Kronfeld7, J. Laiho13,14, L. Levkova5, P. B. Mackenzie7, E. T. Neil7,15,16, M. B. Oktay5, Si-Wei Qiu5, J. N. Simone7, R. Sugar17, D. Toussaint12, R. S. Van de Water7, and Ran Zhou10,7 (Fermilab Lattice and MILC Collaborations)

  • 1Physics Department, Brookhaven National Laboratory, Upton, New York 11973, USA
  • 2Department of Physics and Astronomy, University of Iowa, Iowa 52242, USA
  • 3Department of Physics, Washington University, St. Louis, Missouri 63130, USA
  • 4Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
  • 5Physics Department, University of Utah, Salt Lake City, Utah 84112, USA
  • 6Physics Department, University of Illinois, Urbana, Illinois 61801, USA
  • 7Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
  • 8Liberal Arts Department, School of the Art Institute of Chicago, Chicago, Illinois 60603, USA
  • 9CAFPE and Departamento de Física Teórica y del Cosmos, Universidad de Granada, E-18071 Granada, Spain
  • 10Department of Physics, Indiana University, Bloomington, Indiana 47405, USA
  • 11American Physical Society, Ridge, New York 11961, USA
  • 12Department of Physics, University of Arizona, Tucson, Arizona 85721, USA
  • 13SUPA, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom
  • 14Department of Physics, Syracuse University, Syracuse, New York 13244, USA
  • 15Department of Physics, University of Colorado, Boulder, Colorado 80309, USA
  • 16RIKEN-BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973, USA
  • 17Department of Physics, University of California, Santa Barbara, California 93106, USA

  • *megamiz@ugr.es

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Vol. 112, Iss. 11 — 21 March 2014

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