2007
DOI: 10.1103/physrevd.75.074031
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Potential model calculations and predictions for heavy quarkonium

Abstract: We investigate the spectroscopy and decays of the charmonium and upsilon systems in a potential model consisting of a relativistic kinetic energy term, a linear confining term including its scalar and vector relativistic corrections and the complete perturbative one-loop quantum chromodynamic short distance potential. The masses and wave functions of the various states are obtained using a variational technique, which allows us to compare the results for both perturbative and nonperturbative treatments of the … Show more

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Cited by 157 publications
(163 citation statements)
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“…There exist a wide range of models for the scalar and vector potentials [29,30,74]. In this work we use the following effective potentials:…”
Section: Scalar Interactionmentioning
confidence: 99%
“…There exist a wide range of models for the scalar and vector potentials [29,30,74]. In this work we use the following effective potentials:…”
Section: Scalar Interactionmentioning
confidence: 99%
“…Given the set of parameters, we predict the masses of the forty two bb states shown in Table 1, where we compare the present theoretical predictions with those from the relativized extension of the nonrelativistic model [25] and a semirelativistic Hamiltonian under nonperturbative framework [22]. Fig.…”
Section: Mass Spectrummentioning
confidence: 99%
“…Therefore, both perturbation and nonperturbative treatments have been taken into account recently in Ref. [22], which indicates the most significant effect of different treatments on the wave functions. The nonperturbative treatment brings each state with its own wave function, while the perturbative treatment leads to the same angular momentum multiplets sharing the identical wave function.…”
Section: Introductionmentioning
confidence: 99%
“…By using, for the interaction, only central potentials, we shall not take into account the effects related to the spin-spin, spin-orbit and tensor interaction. These corrective contributions, that are extremely relevant for a detailed study of charmonium spectroscopy [5][6][7][8], can be introduced perturbatively carefully considering the Lorentz transformation properties of the interaction operators. The aim of the following analysis is only to demonstrate that our relativistic equation, with a local kinetic operator, can adequately reproduce the main structure of the charmonium spectrum for the low-lying resonances.…”
Section: A Numerical Application To the Charmonium Spectrummentioning
confidence: 99%
“…(1), is exactly consistent only for the zero component of a vector field. If a scalar (effective) field is considered, as it is usually done, in particular, for the study ¯ and ¯ spectra [5][6][7][8], one should add the corresponding scalar interaction operators to the constituent masses by means of the substitution that will be discussed in Section 3. However, these scalar interaction operators would appear in the square roots of the relativistic energies, giving rise to very serious difficulties for the calculations, unless an approximate Taylor expansion of the square roots is performed.…”
Section: Introductionmentioning
confidence: 99%