2004
DOI: 10.1134/1.1777292
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The pole heavy-quark masses in the Hamiltonian approach

Abstract: From the fact that the nonperturbative self-energy contribution CSE to the heavy meson mass is small: CSE(bb) = 0; CSE(cc) ∼ = −40 MeV

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Cited by 19 publications
(32 citation statements)
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References 45 publications
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“…This result is also consistent with Dyson-Schwinger equation studies of the physical gluon propagator [28,29]. The relationship of these results to the infrared-finite coupling for the vector interaction defined in the quarkonium potential has recently been discussed by Badalian and Veselov [37].…”
Section: The Infrared Behavior Of Effective Qcd Couplingssupporting
confidence: 86%
“…This result is also consistent with Dyson-Schwinger equation studies of the physical gluon propagator [28,29]. The relationship of these results to the infrared-finite coupling for the vector interaction defined in the quarkonium potential has recently been discussed by Badalian and Veselov [37].…”
Section: The Infrared Behavior Of Effective Qcd Couplingssupporting
confidence: 86%
“…For the potential taken from [15], 3. To demonstrate the sensitivity of the leptonic widths to the behavior of the confining potential at large distances we consider the "modified" potential, 10) where the flattening effect is taken into account and the string tension σ(r) is taken as for light mesons [6] while the vector coupling α B (r) is the same as in the potential Eq.…”
Section: Tionmentioning
confidence: 99%
“…For this simple asymptotic potential V asym (large r) = rσ(r) the constituent masses ω n (QQ) and σ(r) nS can be calculated easily from the solutions of the spinless Salpeter equation [15]. For the Υ(6S) and Υ(7S), using (σ 0 = 0.…”
Section: Leptonic Widths Of Highly Excited Resonancesmentioning
confidence: 99%
“…One must also take into account the NP self-energy correction to the quark masses [17], however, in bottomonium the NP self-energy contribution to H R appears to be compatible with zero (∼ 3 MeV) and can be neglected [18]. For the linear potential the splitting ∆ 1 between the orbital excitations 1D and 1P turns out to be ∼ 160 ÷ 170 MeV, i.e., much smaller then the experimental value (1.1).…”
Section: Hamiltonian For Spinless Quark and Antiquarkmentioning
confidence: 99%