TY - JOUR
T1 - Mixing angles and electromagnetic properties of ground state pseudoscalar and vector meson nonets in the light-cone quark model
AU - Choi, Ho Meoyng
AU - Ji, Chueng Ryong
PY - 1999/3/5
Y1 - 1999/3/5
N2 - Both the mass spectra and the wave functions of the light pseudoscalar (Formula presented) and vector(Formula presented) mesons are analyzed within the framework of the light-cone constituent quark model. A Gaussian radial wave function is used as a trial function of the variational principle for a QCD-motivated Hamiltonian which includes not only the Coulomb plus confining potential but also the hyperfine interaction to obtain the correct (Formula presented)-(Formula presented) splitting. For the confining potential, we use the (1) harmonic oscillator potential and (2) linear potential and compare the numerical results for these two cases. The mixing angles of (Formula presented)-(Formula presented) and (Formula presented)-(Formula presented) are predicted and various physical observables such as decay constants, charge radii, and radiative decay rates, etc., are calculated. Our numerical results in the two cases (1) and (2) are overall not much different from each other and are in good agreement with the available experimental data.
AB - Both the mass spectra and the wave functions of the light pseudoscalar (Formula presented) and vector(Formula presented) mesons are analyzed within the framework of the light-cone constituent quark model. A Gaussian radial wave function is used as a trial function of the variational principle for a QCD-motivated Hamiltonian which includes not only the Coulomb plus confining potential but also the hyperfine interaction to obtain the correct (Formula presented)-(Formula presented) splitting. For the confining potential, we use the (1) harmonic oscillator potential and (2) linear potential and compare the numerical results for these two cases. The mixing angles of (Formula presented)-(Formula presented) and (Formula presented)-(Formula presented) are predicted and various physical observables such as decay constants, charge radii, and radiative decay rates, etc., are calculated. Our numerical results in the two cases (1) and (2) are overall not much different from each other and are in good agreement with the available experimental data.
UR - http://www.scopus.com/inward/record.url?scp=85037883722&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.59.074015
DO - 10.1103/PhysRevD.59.074015
M3 - Article
AN - SCOPUS:85037883722
SN - 1550-7998
VL - 59
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
IS - 7
ER -