arXiv · hep-ph/0103230
Calculation of the K^0-\bar{K}^0 mixing parameter via the QCD sum rules at finite energies
Abstract
The QCD finite energy sum rules method is used to show that the parameter of the K^0-\bar{K}_0 mixing \hat{B} is mainly determined by the value of g m_s< \bar{d} G_{μν} σ_{μν} d > and the vacuum expectation values of four-quark operators. Assuming the hypothesis of vacuum dominance and/or unitarity symmetry to estimate latter, it is found that \hat{B}=1.2\pm 0.1. (The updated (March 2001) prediction reads \hat{B} = 1.0 +- 0.1 (for more details, see Comments after the main text).
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K. G. Chetyrkin, A. L. Kataev, A. B. Krasulin, A. A. Pivovarov. 2001-03-21. Calculation of the K^0-\bar{K}^0 mixing parameter via the QCD sum rules at finite energies. https://doi.org/10.1016/0370-2693(86)91137-8
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