The ratio of decay widths of X(3872) to $ \psi^{\prime}\gamma $ and $ J/\psi\gamma$ as a test of the X(3872) dynamical structure
A. M. Badalian, V. D. Orlovsky, Yu. A. Simonov (Institute of, Theoretical, Experimental Physics, Moscow, Russia), B. L. G. Bakker, (Dept.of Physics, Astronomy, Vrije Universiteit, Amsterdam, The, Netherlands)

TL;DR
This paper investigates the radiative decay ratios of X(3872) using a coupled-channel approach, revealing that the dynamical structure significantly influences decay rates and can distinguish between different models of X(3872).
Contribution
It introduces a coupled-channel method combining relativistic string Hamiltonian and string breaking to analyze X(3872)'s structure and decay ratios, providing new insights into its composition.
Findings
The decay ratio R is significantly reduced from 5 to about 0.8 due to wave function admixture.
The model reproduces the X(3872) mass and decay properties consistent with experimental data.
Wave function admixture enhances the transition rate to J/ψγ by 50-70 keV.
Abstract
Radiative decays of X(3872) with are studied in the coupled-channel approach, where the states are described by relativistic string Hamiltonian, while for the decay channels a string breaking mechanism is used. Within this method a sharp peak and correct mass shift of the charmonium state just to the threshold was already obtained for a prescribed channel coupling to the decay channels. For the same value of coupling the normalized wave function (w.f.) of X(3872) acquires admixture of the component with the w.f. fraction ), which increases the transition rate up to 50-70 keV, making the ratio significantly smaller, as…
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