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@ARTICLE{Aoki:15718,
author = {Aoki, Y. and Arthur, R. and Blum, T. and Boyle, P.A. and
Brömmel, D. and Christ, N.H. and Dawson, C. and Izubuchi,
T. and Jung, C. and Kelly, C. and Kenway, R.D. and Lightman,
M. and Mawhinney, R.D. and Ohta, S. and Sachrajda, C.T. and
Scholz, E.E. and Soni, A. and Sturm, C. and Wennekers, J.
and Zhou, R.},
title = {{C}ontinuum {L}imit of ${B}_{K}$ from 2+1 {F}lavor {D}omain
{W}all {QCD}},
journal = {Physical review / D},
volume = {84},
number = {1},
issn = {1550-7998},
address = {[S.l.]},
publisher = {Soc.},
reportid = {PreJuSER-15718},
pages = {014503},
year = {2011},
note = {The calculations reported here were performed on the QCDOC
computers [65-68] at Columbia University, Edinburgh
University, and at Brookhaven National Laboratory (BNL), and
Argonne Leadership Class Facility (ALCF) BlueGene/P
resources at Argonne National Laboratory (ANL). At BNL, the
QCDOC computers of the RIKEN-BNL Research Center and the
USQCD Collaboration were used. The very large scale
capability of the ALCF was critical for carrying out the
challenging calculations reported here. The Edinburgh QCDOC
system was funded by PPARC JIF Grant No. PPA/J/S/1998/00756
and operated through support from the Universities of
Edinburgh, Southampton, and Wales Swansea, and from STFC
Grant No. PP/E006965/1. Computations for this work were
carried out in part on facilities of the USQCD
Collaboration, which are funded by the Office of Science of
the U.S. Department of Energy. We thank ANL, RIKEN, BNL, and
the U.S. DOE, the University of Edinburgh and STFC for
providing the facilities essential for the completion of
this work. The software used includes: the CPS QCD codes
(http://qcdoc.phys.columbia.edu/cps.html), supported in part
by the U.S. DOE SciDAC program; the BAGEL [69] assembler
kernel generator for many of the high-performance optimized
kernels; and the UKHadron codes. The work of the Edinburgh
authors was supported by PPARC Grants No. PP/D000238/1 and
No. PP/C503154/1. P. A. B. acknowledges support from RCUK.
T. B. and R. Z. were supported by the U.S. DOE under Grant
No. DE-FG02-92ER40716. T. I. was supported in part by the
Grant-in-Aid of the Japanese Ministry of Education (Grants
No. 22540301, No. 20105002, and No. 20025010). C.J., T. I.,
C.St., and A. S. (BNL) were partially supported by the U.S.
DOE under Contract No. DE-AC02-98CH10886. E. E. S is partly
supported by DFG SFB/TR 55 and by the Research Executive
Agency of the European Union under Grant No.
PITN-GA-2009-238353 (ITN STRONGnet). N.C. and R. M.
(Columbia University) were partially supported by the U.S.
DOE under Contract No. DE-FG02-92ER40699. D. B. and C. T. S.
(University of Southampton) were partially supported by U.K.
STFC Grant No. PP/D000211/1 and by EU Contract No.
MRTN-CT-2006-035482 (Flavianet). Y.A. is partially supported
by JSPS KAKENHI 21540289. We thank Andrzej Buras for useful
conversations.},
abstract = {We determine the neutral kaon mixing matrix element B-K in
the continuum limit with 2 + 1 flavors of domain wall
fermions, using the Iwasaki gauge action at two different
lattice spacings. These lattice fermions have near exact
chiral symmetry and therefore avoid artificial lattice
operator mixing. We introduce a significant improvement to
the conventional nonperturbative renormalization (NPR)
method in which the bare matrix elements are renormalized
nonperturbatively in the regularization invariant momentum
scheme (RI-MOM) and are then converted into the (MS) over
bar scheme using continuum perturbation theory. In addition
to RI-MOM, we introduce and implement four nonexceptional
intermediate momentum schemes that suppress infrared
nonperturbative uncertainties in the renormalization
procedure. We compute the conversion factors relating the
matrix elements in this family of regularization invariant
symmetric momentum schemes (RI-SMOM) and (MS) over bar at
one-loop order. Comparison of the results obtained using
these different intermediate schemes allows for a more
reliable estimate of the unknown higher-order contributions
and hence for a correspondingly more robust estimate of the
systematic error. We also apply a recently proposed approach
in which twisted boundary conditions are used to control the
Symanzik expansion for off-shell vertex functions leading to
a better control of the renormalization in the continuum
limit. We control chiral extrapolation errors by considering
both the next-to-leading order SU(2) chiral effective
theory, and an analytic mass expansion. We obtain B-K((MS)
over bar)(3 GeV) = 0.529(5)(stat)(15)(chi)(2)(FV)(11)(NPR).
This corresponds to (B) over cap ((RGI ) over bar)(K) =
0.749(7)(stat)(21)(chi)(3)(FV)(15)(NPR). Adding all sources
of error in quadrature, we obtain (B) over cap ((RGI ) over
bar)(K)0.749(27)(combined), with an overall combined error
of $3.6\%.$},
keywords = {J (WoSType)},
cin = {JSC},
ddc = {530},
cid = {I:(DE-Juel1)JSC-20090406},
pnm = {Scientific Computing (FUEK411) / 411 - Computational
Science and Mathematical Methods (POF2-411)},
pid = {G:(DE-Juel1)FUEK411 / G:(DE-HGF)POF2-411},
shelfmark = {Astronomy $\&$ Astrophysics / Physics, Particles $\&$
Fields},
typ = {PUB:(DE-HGF)16},
UT = {WOS:000292514400009},
doi = {10.1103/PhysRevD.84.014503},
url = {https://juser.fz-juelich.de/record/15718},
}