Liquid-gas phase transition in strange hadronic matter with relativistic models
arXiv:1510.01381 · doi:10.1103/PhysRevC.93.024306
Abstract
Background: The advent of new dedicated experimental programs on hyperon physics is rapidly boosting the field, and the possibility of synthetizing multiple strange hypernuclei requires the addition of the strangeness degree of freedom to the models dedicated to nuclear structure and nuclear matter studies at low energy. Purpose: We want to settle the influence of strangeness on the nuclear liquid-gas phase transition. Because of the large uncertainties concerning the hyperon sector, we do not aim at a quantitative estimation of the phase diagram but rather at a qualitative description of the phenomenology, as model independent as possible. Method: We analyze the phase diagram of low density matter composed of neutrons, protons and hyperons using a Relativistic Mean Field (RMF) model. We largely explore the parameter space to pin down generic features of the phase transition, and compare the results to ab-initio quantum Monte Carlo calculations. Results: We show that the liquid-gas phase transition is only slightly quenched by the addition of hyperons. Strangeness is seen to be an order parameter of the phase transition, meaning that dilute strange matter is expected to be unstable with respect to the formation of hyper-clusters. Conclusions: More quantitative results within the RMF model need improved functionals at low density, possibly fitted to ab-initio calculations of nuclear and matter.
References in corpus (14)
- Hyperon Puzzle: Hints from Quantum Monte Carlo Calculations
- New Hyperon Equations of State for Supernovae and Neutron Stars in Density-dependent Hadron Field Theory
- Proto-Neutron and Neutron Stars in a Chiral SU(3) Model
- Hypernuclear Physics for Neutron Stars
- Constraining hypernuclear density functional with -hypernuclei and compact stars
- Equation of state of low--density neutron matter and the pairing gap
- Double- hypernuclei in the relativistic mean-field theory
- Cluster formation in compact stars: relativistic versus Skyrme models
- Behaviour of the and potential strengths in the He hypernucleus
- Spinodal instabilities and the distillation effect in nuclear matter under strong magnetic fields
- Latent heat of nuclear matter
- A relativistic mean field study of multi-strange system
- Ground states and excited states of hypernuclei in Relativistic Mean Field approach
- Liquid gas phase transition in hypernuclei
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- Critical parameters of consistent relativistic mean-field models
- Examination of strangeness instabilities and effects of strange meson couplings in dense strange hadronic matter and compact stars
- Correlations between critical parameters and bulk properties of nuclear matter
- A closer look at the Yukawa's interaction from a symmetry group perspective
- Critical behaviour of an effective relativistic mean field model in the presence of magnetic background and boundaries
- Strangeness thermodynamic instabilities in hot and dense nuclear matter
- Effect of hyperons on phase coexistence in strange matter
- The role of strangeness and isospin in low density expansions of hadronic matter