The Complete |Delta S|=2 Hamiltonian in the Next-To-Leading Order
arXiv:hep-ph/9604330 · doi:10.1016/0550-3213(96)00324-0
Abstract
We present the complete next-to-leading order short-distance QCD corrections to the effective \dstwo -hamiltonian in the Standard Model. The calculation of the coefficient is described in great detail. It involves the two-loop mixing of bilocal structures composed of two \dsone\ operators into \dstwo\ operators. The next-to-leading order corrections enhance by 27\% to $η_3=0.47 \errorpm{+0.03}{-0.04}$ thereby affecting the phenomenology of sizeably. depends on the physical input parameters , and $\laMSb$ only weakly. The quoted error stems from renormalization scale dependences, which have reduced compared to the old leading log result. The known calculation of and is repeated in order to compare the structure of the three QCD coefficients. We further discuss some field theoretical aspects of the calculation such as the renormalization group equation for Green's functions with two operator insertions and the renormalization scheme dependence caused by the presence of evanescent operators.
68 pages, requires LaTeX2e and the standard LaTeX-packages epsf.sty, rotate.sty, a4.sty, subeqn.sty, cite.sty, array.sty, dcolumn.sty; Figures are submitted as a seperate tar.gz-file. A complete PostScript version may be obtained from ftp://feynman.t30.physik.tu-muenchen.de/pub/preprints/tum-86-96.ps.gz or ftp://feynman.t30.physik.tu-muenchen.de/pub/preprints/tum-86-96.ps2.gz (scaled down and rotated version to print two pages on one sheet of paper). Source available at ftp://feynman.t30.physik.tu-muenchen.de/pub/preprints/tum-86-96.tar.gz
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