Restudy on the wave functions of {Upsilon}(nS) states in the light-front quark model and the radiative decays of {Upsilon}(nS){yields}{eta}{sub b}+{gamma}
The light-front quark model has been applied to calculate the transition matrix elements of heavy hadron decays. However, it is noted that using the traditional wave functions of the light-front quark model given in the literature, the theoretically determined decay constants of the {Upsilon}(nS) obviously contradict the data. This implies that the wave functions must be modified. Keeping the orthogonality among the nS states and fitting their decay constants, we obtain a series of the wave functions for {Upsilon}(nS). Based on these wave functions and by analogy with the hydrogen atom, we suggest a modified analytical form for the {Upsilon}(nS) wave functions. Using the modified wave functions, the obtained decay constants are close to the experimental data. Then we calculate the rates of radiative decays of {Upsilon}(nS){yields}{eta}{sub b}+{gamma}. Our predictions are consistent with the experimental data on decays {Upsilon}(3S){yields}{eta}{sub b}+{gamma} within the theoretical and experimental errors.