Heavy quarkonia description from a generalized screened potential model

2016 ◽  
Author(s):  
P. González
1983 ◽  
Vol 28 (7) ◽  
pp. 1716-1720 ◽  
Author(s):  
Suraj N. Gupta ◽  
Stanley F. Radford ◽  
Wayne W. Repko

2006 ◽  
Vol 21 (17) ◽  
pp. 1383-1391 ◽  
Author(s):  
D. U. MATRASULOV ◽  
F. C. KHANNA ◽  
KH. T. BUTANOV ◽  
KH. YU. RAKHIMOV

Finite-temperature spectra of heavy quarkonia are calculated by combining potential model and thermofield dynamics formalisms. The mass spectra of the heavy quarkonia with various quark contents are calculated. It is found that binding mass of the quarkonium decreases as temperature increases.


1989 ◽  
Vol 04 (13) ◽  
pp. 1277-1285 ◽  
Author(s):  
S. GHOSH ◽  
S. MUKHERJEE

The adequacy of using the Breit-Fermi type of interactions for describing the fine hyperfine splittings of heavy quarkonia has been examined critically. A potential model which just about accommodates the trend of the recent data on 1P1 states has been studied. The possibility of including the spin-dependent contributions of a pseudoscalar exchange potential is also considered. It is shown that the choice of the Breit-Fermi form for the spin-dependent interactions severely constrains the generally accepted non-relativistic potential and do not allow enough freedom to fit the recent data on 1P1 levels.


1986 ◽  
Vol 34 (1) ◽  
pp. 201-206 ◽  
Author(s):  
Suraj N. Gupta ◽  
Stanley F. Radford ◽  
Wayne W. Repko

2019 ◽  
Vol 34 (37) ◽  
pp. 1950307 ◽  
Author(s):  
Ahmed Al-Jamel

Heavy [Formula: see text] and [Formula: see text] quarkonia are considered as systems confined within a hard-wall potential shaped after a linear combination of a cotangent — with a square co-secant function. Wave functions and energy spectra are then obtained in closed forms in solving by the Nikiforov–Uvarov method the associated radial Schrödinger equation in the presence of a centrifugal term. The interest in this potential is that in one parametrization, it can account for a conformal symmetry of the strong interaction, and in another for its perturbation, a reason for which we here employ it to study status of conformal symmetry in the heavy flavor sector. The resulting predictions on heavy quarkonia mass spectra and root mean square radii are compared with the available experimental data, as well as with predictions by other theoretical approaches. We observe that a relatively small conformal symmetry perturbing term in the potential suffices to achieve good agreement with data.


1989 ◽  
Vol 39 (3) ◽  
pp. 974-977 ◽  
Author(s):  
Suraj N. Gupta ◽  
Wayne W. Repko ◽  
Casimir J. SuchytaIII

2005 ◽  
Vol 43 (1-4) ◽  
pp. 77-80 ◽  
Author(s):  
Á Mócsy ◽  
P. Petreczky

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