Thermodynamic properties of nuclear matter with three-body forces

Abstract

We calculate thermodynamic quantities in symmetric nuclear matter within the self-consistent Green's functions method including three-body forces. The thermodynamic potential is computed directly from a diagrammatic expansion, implemented with the CD-Bonn and Nijmegen nucleon-nucleon potentials and the Urbana three-body forces. We present results for entropy and pressure up to temperatures of 20 MeV and densities of 0.32 fm^-3. While the pressure is sensitive to the inclusion of three-body forces, the entropy is not. The unstable spinodal region is identified and the critical temperature associated to the liquid-gas phase transition is determined. When three-body forces are added we find a strong reduction of the critical temperature, obtaining T_c ~ 12 MeV.

arXiv comment5 pages, 6 figures

References in corpus (16)

• The high-precision, charge-dependent Bonn nucleon-nucleon potential (CD-Bonn)
• Construction of high-quality Nucleon-Nucleon potential models
• Caloric curves and critical behavior in nuclei
• Limiting temperatures and the Equation of State of Nuclear Matter
• A unique spinodal region in asymmetric nuclear matter
• In medium T-matrix for nuclear matter with three-body forces - binding energy and single particle properties
• Symmetric and asymmetric nuclear matter in the relativistic approach at finite temperatures
• Liquid-gas phase transition in nuclear matter from realistic many-body approaches
• Self-consistent solution of Galitskii-Feynman equations at finite temperature
• Thermodynamic consistency for nuclear matter calculations
• Variational Theory of Hot Nucleon Matter
• The entropy of a correlated system of nucleons
• Limiting temperature from microscopic equation of state
• Superfluidity with dressed nucleons
• Temperature dependence of single-particle properties in nuclear matter
• Diagrammatic calculation of thermodynamical quantities in nuclear matter

Cited by in corpus (22)

• Neutron matter from chiral two- and three-nucleon calculations up to N${}^3$LO
• Ab-initio self-consistent Gorkov-Green's function calculations of semi-magic nuclei - I. Formalism at second order with a two-nucleon interaction
• Self-consistent Green's functions formalism with three-body interactions
• Symmetric nuclear matter with chiral three-nucleon forces in the self-consistent Green's functions approach
• Correlated density-dependent chiral forces for infinite matter calculations within the Green's function approach
• Nuclear chiral dynamics and thermodynamics
• Non-congruence of the nuclear liquid-gas and deconfinement phase transitions
• Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter
• Self-consistent Green's function theory for atomic nuclei
• $Abinitio$ constraints on thermal effects of the nuclear equation of state
• A comparative study of statistical models for nuclear equation of state of stellar matter
• Chiral thermodynamics of nuclear matter
• Ab initio nuclear thermodynamics
• BEC-BCS Crossover and the Liquid-Gas Phase Transition in Hot and Dense Nuclear Matter
• Microscopic predictions of the nuclear matter liquid-gas phase transition
• Effective interaction dependence of the liquid-gas phase transition in symmetric nuclear matter
• Structure Factors for Hot Neutron Matter from Ab Initio Lattice Simulations with High-Fidelity Chiral Interactions
• Setting nonperturbative uncertainties on finite-temperature properties of neutron matter
• Nuclear matter at finite temperature and static properties of proto-neutron star
• Latent heat of nuclear matter
• Many-body Propagator Theory with Three-Body Interactions: a Path to Exotic Open Shell Isotopes
• Self-consistent Green's functions with three-body forces