Abstract

Using HISQ $N_f=2+1+1$ MILC ensembles with five different values of the lattice spacing, including four ensembles with physical quark masses, we have performed the most precise computation to date of the $K\to\pi\ell\nu$ vector form factor at zero momentum transfer, $f_+^{K^0\pi^-}(0)=0.9696(15)_\text{stat}(12)_\text{syst}$. 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 matrix element $|V_{us}|=0.22333(44)_{f_+(0)}(42)_\text{exp}$, 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 $f_{K^+}/f_{\pi^+}$, which uses $|V_{ud}|$ as input. Our value of $|V_{us}|$ is in tension at the 2--$2.6\sigma$ 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 $|V_{ud}|$, although a recent determination of the nucleus-independent radiative corrections to superallowed nuclear $\beta$ decays could reduce the $|V_{ud}|^2$ uncertainty nearly to that of $|V_{us}|^2$. 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. As part of our analysis, we calculated the correction to $f_+^{K\pi}(0)$ 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 $[C_{12}^r+C_{34}^r-(L_5^r)^2](M_\rho)=(2.92\pm0.31)\cdot10^{-6}$.

Highlights

  • High-precision tests of the unitarity of the CabibboKobayashi-Maskawa (CKM) matrix, as predicted by the Standard Model (SM), are at the forefront of the current flavor physics program

  • As we were finishing this work, a paper appeared with a new calculation of the nucleus-independent electroweak radiative corrections involved in the extraction of jVudj from superallowed β decays with a new approach based on dispersion relations [17]

  • Isospin-breaking corrections accounting for the difference between the up- and down-quark masses can be calculated in the chiral perturbation theory (ChPT) framework and written as a chiral expansion starting at next-to-leading order (NLO) for neutral kaons fKþπ;isospin limitð0Þ

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Summary

INTRODUCTION

High-precision tests of the unitarity of the CabibboKobayashi-Maskawa (CKM) matrix, as predicted by the Standard Model (SM), are at the forefront of the current flavor physics program. Determinations of jVusj from leptonic kaon and pion decays (Kl2 and πl2), combined with fK=fπ from lattice QCD, currently have somewhat smaller errors than those from Kl3. As we were finishing this work, a paper appeared with a new calculation of the nucleus-independent electroweak radiative corrections involved in the extraction of jVudj from superallowed β decays with a new approach based on dispersion relations [17] If this calculation is confirmed, the resulting value of jVudj would increase the present tension with unitarity. Inclusive hadronic τ decays have, in the past, yielded values of jVusj smaller than the semileptonic kaon determination and, were in even more disagreement with unitarity [34].

LATTICE SETUP AND ANALYSIS
Fit methods and statistical analysis
FORM-FACTOR CORRECTIONS
Finite volume
Nonequilibrated topological charge
Fit results
SYSTEMATIC ERROR ANALYSIS
Inputs for the fixed parameters in the chiral function
Lattice scale
Partial-quenching effects in ms at NNLO
Higher-order finite-volume corrections
Method
Isospin-breaking corrections
RESULTS
Determination of jVusj
Tests of CKM unitarity
Ratio of leptonic and semileptonic decays
Implications of the new extraction of jVudj
VIII. CONCLUSIONS AND OUTLOOK

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