English

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 λ4\lambda ^{4}, where λ0.22\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).

Keywords

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

R2 v1 2026-07-22T13:46:01.350Z