Critical temperature for the nuclear liquid-gas phase transition (from multifragmentation and fission)

Abstract

Critical temperature Tc for the nuclear liquid-gas phase transition is stimated both from the multifragmentation and fission data. In the first case,the critical temperature is obtained by analysis of the IMF yields in p(8.1 GeV)+Au collisions within the statistical model of multifragmentation (SMM). In the second case, the experimental fission probability for excited 188Os is compared with the calculated one with Tc as a free parameter. It is concluded for both cases that the critical temperature is higher than 16 MeV.

15 pages, 8 figures

References in corpus (7)

• The liquid to vapor phase transition in excited nuclei
• Thermodynamical features of multifragmentation in peripheral Au + Au Collisions at 35 A.MeV
• Microscopic model approaches to fragmentation of nuclei and phase transitions in nuclear matter
• Critical Temperature for the Nuclear Liquid-Gas Phase Transition
• Critical Exponents of the Statistical Multifragmentation Model
• Multifragmentation and nuclear phase transitions (liquid-fog and liquid-gas)
• Nuclear multifragmentation and fission: similarity and differences

Cited by in corpus (23)

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• Nuclear Equation of state for Compact Stars and Supernovae
• Functional renormalization group studies of nuclear and neutron matter
• From asymmetric nuclear matter to neutron stars: a functional renormalization group study
• Chiral thermodynamics of nuclear matter
• Thermodynamic phases and mesonic fluctuations in a chiral nucleon-meson model
• Microscopic predictions of the nuclear matter liquid-gas phase transition
• Thermal Properties of Asymmetric Nuclear Matter
• The Flow Constraint Influence on the Properties of Nuclear Matter Critical Endpoint
• Critical parameters of consistent relativistic mean-field models
• Correlations between critical parameters and bulk properties of nuclear matter
• Nuclear matter at finite temperature and static properties of proto-neutron star
• Hot and dense matter beyond relativistic mean field theory
• Warm unstable asymmetric nuclear matter: critical properties and the density dependence of the symmetry energy
• Modern nuclear and astrophysical constraints of dense matter in a renormalized chiral approach
• Critical Properties of Symmetric Nuclear Matter in Low-Density Regime Using Effective-Relativistic Mean Field Formalism
• Critical properties of calibrated relativistic mean-field models for the transition to warm, non-homogeneous nuclear matter
• Dense nucleonic matter and the renormalization group
• Analysis of critical parameters for nonrelativistic models in symmetric nuclear matter