Phase diagram for the asymmetric nuclear matter in the multifragmentation model
arXiv:0908.1521 · doi:10.1103/PhysRevC.80.044609
Abstract
We assume that, in equilibrium, nuclear matter at reduced density and moderate finite temperature, breaks up into many fragments. A strong support to this assumption is provided by date accumulated from intermediate energy heavy ion collisions. The break-up of hot and expanded nuclear matter according to rules of equilibrium statistical mechanics is the multifragmentation model. The model gives a first order phase transition. This is studied in detail here. Phase-equilibrium lines for different degrees of asymmetry are computed.
22 pages, 10 figures
References in corpus (8)
- Phase Transitions in Warm, Asymmetric Nuclear Matter
- Cluster Formation and The Virial Equation of State of Low-Density Nuclear Matter
- The Thermodynamic Model for Nuclear Multifragmentation
- Role of isospin in the nuclear liquid-gas phase transition
- Exactly Soluble Model for Nuclear Liquid-Gas Phase Transition
- Comparison of Statistical Multifragmentation Model simulations with Canonical Thermodynamical Model results: a few representative cases
- A Model for Phase Transition based on Statistical Disassembly of Nuclei at Intermediate Energies
- Nuclear condensation and the equation of state of nuclear matter
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- Conditions for equivalence of Statistical Ensembles in Nuclear Multifragmentation
- Liquid gas phase transition in hypernuclei
- Common Approaches in Description of Ordinary Liquids and Hadronic Matter