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Biennial Report 2005-2007 - Saha Institute of Nuclear Physics

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Theoretical <strong>Physics</strong> 151.4 Relativistic Heavy Ion Collisions, Quantum Chromodynamics,Hadrodynamics and Quark-Gluon Plasma1.4.1.1 Energy Loss <strong>of</strong> Charm Quarks in the Quark-Gluon Plasma: Collisional vsRadiativeConsidering the collisional energy loss rates <strong>of</strong> heavy quarks from hard light parton interactions thetotal energy loss <strong>of</strong> a charm quark for a static medium has been computed. For the energy range E ∼(5−10) GeV <strong>of</strong> charm quark, it is found to be almost same order as that <strong>of</strong> radiative ones estimatedto a first order opacity expansion. The collisional energy loss will become much more important forlower energy charm quarks and this feature could be very interesting for phenomenology <strong>of</strong> hadronsspectra.Munshi Golam MustafaTheo1.4.1.2 Dynamical Screening in a Quark-Gluon PlasmaWe calculate the wake potential <strong>of</strong> a fast parton moving through a quark gluon plasma usingthe framework <strong>of</strong> the Boltzmann-Vlasov equation. We found an anisotropic potential showing aminimum in the direction <strong>of</strong> the parton velocity. Possible consequences <strong>of</strong> this potential on binarystates in a quark-gluon plasma are discussed.Purnendu Chakraborty, Munshi Golam Mustafa, Markus H Thoma†Theo1.4.1.3 Some Applications <strong>of</strong> Thermal Field Theory to Quark-Gluon PlasmaIn this review we briefly introduce the thermal field theory within imaginary time formalism, thehard thermal loop perturbation theory and some <strong>of</strong> its applications to the physics <strong>of</strong> the quarkgluonplasma, possibly created in relativistic heavy-ion collisions.Munshi Golam MustafaTheo1.4.1.4 Susceptibilities and Speed <strong>of</strong> Sound from the Polyakov-Nambu-Jona-LasinioModelWe present the Taylor expansion coefficients <strong>of</strong> the pressure in quark number chemical potentialµ 0 = µ B /3 = µ u = µ d , for the strongly interacting matter as described by the PNJL model for twolight degenerate flavours <strong>of</strong> quarks u and d. The expansion has been done upto eighth order in µ 0 ,and the results are consistent with recent estimates from Lattice. We have further obtained thespecific heat C V , squared speed <strong>of</strong> sound v 2 s and the conformal measure ∆ C.Sanjay K Ghosh†, Tamal K Mukherjee†, Rajarshi Ray, Munshi G MustafaTheo

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