The study deals with a scenario in which quark confinement within hadrons occurs as a first order phase transition and bubbles of the flow temperature phase are nucleated as a result of thermal fluctuations after the quark-gluon plasma has become slightly supercooled. The early stages of bubble growth are discussed and numerical results obtained for the case of a single spherical hadronic bubble are presented.

Structure of the Hydrodynamical Flow During the Cosmological Quark-Hadron Transition

PANTANO, ORNELLA;
1989

Abstract

The study deals with a scenario in which quark confinement within hadrons occurs as a first order phase transition and bubbles of the flow temperature phase are nucleated as a result of thermal fluctuations after the quark-gluon plasma has become slightly supercooled. The early stages of bubble growth are discussed and numerical results obtained for the case of a single spherical hadronic bubble are presented.
1989
Italian Conference on General Relativity and Gravitational Physics
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11577/174568
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