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      Formation of excited systems with a wide range in\(N/Z\)

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          Statistical multifragmentation of nuclei

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            Systematics of complex fragment emission in niobium-induced reactions

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              Is Open Access

              Phase Transitions in Warm, Asymmetric Nuclear Matter

              A relativistic mean-field model of nuclear matter with arbitrary proton fraction is studied at finite temperature. An analysis is performed of the liquid-gas phase transition in a system with two conserved charges (baryon number and isospin) using the stability conditions on the free energy, the conservation laws, and Gibbs' criteria for phase equilibrium. For a binary system with two phases, the coexistence surface (binodal) is two-dimensional. The Maxwell construction through the phase-separation region is discussed, and it is shown that the stable configuration can be determined uniquely at every density. Moreover, because of the greater dimensionality of the binodal surface, the liquid-gas phase transition is continuous (second order by Ehrenfest's definition), rather than discontinuous (first order), as in familiar one-component systems. Using a mean-field equation of state calibrated to the properties of nuclear matter and finite nuclei, various phase-separation scenarios are considered. The model is then applied to the liquid-gas phase transition that may occur in the warm, dilute matter produced in energetic heavy-ion collisions. In asymmetric matter, instabilities that produce a liquid-gas phase separation arise from fluctuations in the proton concentration (chemical instability), rather than from fluctuations in the baryon density (mechanical instability).
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                Author and article information

                Journal
                PRVCAN
                Physical Review C
                Phys. Rev. C
                American Physical Society (APS)
                0556-2813
                1089-490X
                June 2003
                June 3 2003
                : 67
                : 6
                Article
                10.1103/PhysRevC.67.064602
                85633291-2444-47f0-bc63-94ab78f44e9b
                © 2003

                http://link.aps.org/licenses/aps-default-license

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