We investigate the scenario of homogeneous nucleation for a first order quark-hadron phase transition in a rapidly expanding background of quark gluon plasma. Using an improved preexponential factor for homogeneous nucleation rate, we solve a set of coupled equations to study the hadronization and the hydrodynamical evolution of the matter. It is found that significant supercooling is possible before hadronization begins. This study also suggests that spinodal decomposition competes with nucleation and may provide an alternative mechanism for phase conversion particularly if the transition is strong enough and the medium is nonviscous. For weak enough transition, the phase conversion may still proceed via homogeneous nucleation. PACS number(s): 12.38.Mh, 64.60.Qb
I. INTRODUCTIONThe hadronization of Quark Gluon Plasma (QGP) possibly produced in the early universe or expected to be formed in relativistic heavy-ion collisions [1] has been the focus of much attention during the past few years. The quark gluon plasma (QGP), if formed, would expand hydrodynamically and would cool down until it reaches a critical temperature T C where a phase transition from the quark matter to the hadron matter begins. Although the plasma has to hadronize, the mechanism of hadronization still remains an open question. The percolation model calculations are used in the case of a second order phase transition. In a first order scenario, the dynamics of the phase transition has been modeled in several ways. In the most idealized picture, the temperature of the plasma is held fixed at T = T C until the phase conversion is completely over. Assuming an isoentropic expansion in (1+1) dimension, the hadronization in the above picture gets completed at τ h = r τ C where r is the ratio of the degrees of freedom of QGP and hadronic phases and τ C is the proper time at which the QGP cools down to the temperature T C . In reality, a first order phase transition is characterized by a large nucleation barrier that separates the two phases at T = T C and the hadronization will not begin unless the matter supercools below T C . Alternatively, the theory of homogeneous nucleation has been invoked to study the first order phase transition which is more realistic than the above idealized adiabatic scenario and has been in use for quite some time in the cosmological context [2]. In this picture, the transition is initiated by the nucleation of critical-size hadron bubbles from a supercooled metastable QGP phase. These hadron bubbles can grow against surface tension, converting the QGP phase into the hadron phase as the temperature drops below the critical temperature, T C . For strong enough transition, the large amplitude fluctuations are suppressed so that the nucleation begins from a (nearly) homogeneous background of supercooled metastable phase. This has been the basis of homogeneous nucleation theory [3] based on which the QCD phase transition has been studied extensively [4][5][6][7][8][9]. However, for a weak enough transition, the matter may not ...