Renormalization group evolution of the CKM matrix

Details Renormalization group evolution of the CKM matrix Renormalization group evolution of the CKM matrix

2003-01-14

arxiv.org/abs/hep-ph/0301098v1

AIP Conf.Proc.670:81-86,2003

Physics

High Energy Physics

High Energy Physics - Phenomenology

Talk given in the X Mexican School of Particles and Fields, Playa del Carmen, Mexico, 2002. 6 pages, LaTeX, needs aipproc.cls

Scientific paper

10.1063/1.1594322

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 $\lambda ^{4}$, where $\lambda \sim 0.22$ 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).

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