Abstract
We study the radiative decays of the D13(1515), S11(1525), F15(1690), and Y0*(1520) resonances within the framework of the symmetric quark model with harmonic-oscillator wave functions. We point out that if it is assumed that the quarks have large anomalous magnetic moments, then it becomes necessary to consider the so-called "spin-orbit" term in the nonrelativistic electromagnetic interaction Hamiltonian. Including the effect of this term, we show that it is possible to understand the vanishing contribution of the D13(1515) resonance to backward or forward pion photoproduction in terms of a cancellation between electric and magnetic multipoles. Requiring such a cancellation gives a value of the oscillator range parameter, α=105 MeV. Using this value and assuming that the quark scale magnetic moment μ is equal to the proton moment, we calculate the multipole amplitudes involved in the decays of interest, and compare the results for the D15(1515) and S11(1525) resonances with the recent phenomenological multipole analysis by Chau, Dombey, and Moorhouse of pion photoproduction in the second resonance region. Agreement is reasonably good. For the Y0*(1520) we obtain a radiative width Γγ=0.051 MeV to be compared with a recent experimental result Γγ=0.15±0.03 MeV, and an angular distribution compatible with experimen t. We comment on the contribution of the F15(1690) resonance to pion photoproduction.