TY - JOUR
T1 - Relations among the light-cone quark models with the invariant meson mass scheme and the model prediction of the [Formula presented] mixing angle
AU - Choi, Ho Meoyng
AU - Ji, Chueng Ryong
PY - 1997
Y1 - 1997
N2 - We analyze the relations among the light-cone quark models which are based on the invariant meson mass scheme. We find that the difference from the Jacobi factor in model wave functions is substantially reduced in the numerical predictions for the physical observables once the best fit parameters are chosen. The difference in the choice of radial wave function [e.g., harmonic oscillator (HO) wave function versus power-law wave function] is, however, still appreciable even though the best fit parameters are used. We also observe an excellent agreement between the HO model predictions and the experimental data on the radiative decays of pseudoscalar [Formula presented] and vector [Formula presented] mesons and [Formula presented] processes, if we use the constraint obtained by the axial anomaly plus partial conservation of axial-vector current relations and choose the [Formula presented] mixing angle [Formula presented] [Formula presented]
AB - We analyze the relations among the light-cone quark models which are based on the invariant meson mass scheme. We find that the difference from the Jacobi factor in model wave functions is substantially reduced in the numerical predictions for the physical observables once the best fit parameters are chosen. The difference in the choice of radial wave function [e.g., harmonic oscillator (HO) wave function versus power-law wave function] is, however, still appreciable even though the best fit parameters are used. We also observe an excellent agreement between the HO model predictions and the experimental data on the radiative decays of pseudoscalar [Formula presented] and vector [Formula presented] mesons and [Formula presented] processes, if we use the constraint obtained by the axial anomaly plus partial conservation of axial-vector current relations and choose the [Formula presented] mixing angle [Formula presented] [Formula presented]
UR - https://www.scopus.com/pages/publications/0000790916
U2 - 10.1103/PhysRevD.56.6010
DO - 10.1103/PhysRevD.56.6010
M3 - Article
AN - SCOPUS:0000790916
SN - 1550-7998
VL - 56
SP - 6010
EP - 6013
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
IS - 9
ER -