Renormalization group evolution of the CKM matrix
High Energy Physics - Phenomenology
2010-11-23 v1
Abstract
We present here the most important ideas, equations and solutions for the running of all the quark Yukawa couplings and all the elements of the Cabibbo-Kobayashi-Maskawa matrix, in the approximation of one loop, and up to order , where is the sine of the Cabibbo angle. Our purpose is to determine what the evolution of these parameters may indicate for the physics of the standard model (SM), the minimal supersymmetric standard model (MSSM) and for the Double Higgs Model (DHM).
Cite
@article{arxiv.hep-ph/0301098,
title = {Renormalization group evolution of the CKM matrix},
author = {P. Kielanowski and S. R. Juarez W},
journal= {arXiv preprint arXiv:hep-ph/0301098},
year = {2010}
}
Comments
Talk given in the X Mexican School of Particles and Fields, Playa del Carmen, Mexico, 2002. 6 pages, LaTeX, needs aipproc.cls style