2015
DOI: 10.1142/s021773231550162x
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Quarkonia disintegration due to time dependence of the qq̄ potential in relativistic heavy-ion collisions

Abstract: Rapid thermalization in ultra-relativistic heavy-ion collisions leads to fast changing potential between a heavy quark and antiquark from zero temperature potential to the finite temperature one. Time dependent perturbation theory can then be used to calculate the survival probability of the initial quarkonium state. In view of very short time scales of thermalization at RHIC and LHC energies, we calculate the survival probability of J/ψ and Υ using sudden approximation. Our results show that quarkonium decay … Show more

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Cited by 6 publications
(2 citation statements)
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“…Moreover, lattice studies have also shown that the potential may have a sizable imaginary part [22]. There are, however, other processes that may cause the depopulation of the resonance states either through the transition from ground state to the excited states during the nonadiabatic evolution of quarkonia [23] or through the swelling or shrinking of states due to the Brownian motion of QQ states in the parton plasma [24]. Very recently the change in the properties of heavy quarkonia immersed in a weakly coupled thermal QCD medium has been described by hard thermal loop (HTL) permittivity [25].…”
Section: Introductionmentioning
confidence: 99%
“…Moreover, lattice studies have also shown that the potential may have a sizable imaginary part [22]. There are, however, other processes that may cause the depopulation of the resonance states either through the transition from ground state to the excited states during the nonadiabatic evolution of quarkonia [23] or through the swelling or shrinking of states due to the Brownian motion of QQ states in the parton plasma [24]. Very recently the change in the properties of heavy quarkonia immersed in a weakly coupled thermal QCD medium has been described by hard thermal loop (HTL) permittivity [25].…”
Section: Introductionmentioning
confidence: 99%
“…We have investigated the time evolution of spatial wave functions of quarkonia and therefore have not considered the spin-magnetic field interaction into account for the current article. The non-adiabatic evolution previously has been addressed in the context of evolving QGP [17] and also in the context of rapid thermalisation [18].…”
mentioning
confidence: 99%