Abstract
We analyze the transitions between hadronic and quark-gluon phases of QCD using an effective low-energy lagrangian for chiral and scale invariance, which embodies quark and gluon condensation. We argue that the quark condensation and deconfinement transitions take place at the same temperature, T q, and that gluon condensation and confinement occur at a common temperature T g. The requirement that scale invariance be spontaneously broken before quarks condense imposes T q ⩽ T q. The gluon transition is in general first order, whereas the quark transition may be second order if T q < T g, or first order if T q = T g, which is favoured for large N c. We argue on general grounds and demonstrate with several model calculations that massive hadrons play a key role in driving the gluon transition, and suggest that T g is below the Hagedorn temperature. We also estimate the surface tension for hadronic bubbles forming in a quark-gluon plasma, finding it to be somewhat too small for inhomogeneities to affect the standard calculations of cosmological nucleosynthesis.
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