Determination of Alpha_s(1 GeV) from the charmonium fine structure

Abstract

The strong coupling constant ${\alpha }_s(\mu )$ is extracted from the fits to charmonium spectrum and fine structure splittings. The relativistic kinematics is taken into account and relativistic corrections are shown to increase the matrix elements defining spin effects up to 40%. The value of ${\alpha }_s(\mu )$ at low-energy scale $\mu =1.0\pm 0.2GeV$ was found to be ${\alpha }_s(\mu )=0.38\pm 0.03(exp.)+0.04(theor.)$ which is about 50% lower than standard perturbative two-loop approximation and is in good agreement with the freezing ${\alpha }_s$ behaviour.

Comments: RevTeX 8 pages, 1 figure in ps format