Pressure inequalities for nuclear and neutron matter
arXiv:nucl-th/0407101 · doi:10.1103/PhysRevC.71.044001
Abstract
We prove several inequalities using lowest-order effective field theory for nucleons which give an upper bound on the pressure of asymmetric nuclear matter and neutron matter. We prove two types of inequalities, one based on convexity and another derived from shifting an auxiliary field.
16 pages, published journal version - includes inequalities for spin polarized systems
References in corpus (12)
- Observation of a Strongly-Interacting Degenerate Fermi Gas of Atoms
- Measurement of interaction energy near a Feshbach resonance in a 6Li Fermi gas
- Measurement of positive and negative scattering lengths in a Fermi gas of atoms
- Radio-Frequency Spectroscopy of Ultracold Fermions
- Mechanical Stability of a Strongly-Interacting Fermi Gas of Atoms
- Nuclear Lattice Simulations with Chiral Effective Field Theory
- A lattice theory for low energy fermions at finite chemical potential
- Inequalities for Light Nuclei in the Wigner Symmetry Limit
- QCD inequalities for the nucleon mass and the free energy of baryonic matter
- Inequalities for low-energy symmetric nuclear matter
- Mean Field Calculation of Thermal Properties of Simple Nucleon Matter on a Lattice
- Nonlinear Realization of Chiral Symmetry on the Lattice
Cited by in corpus (7)
- Lattice Simulations for Light Nuclei: Chiral Effective Field Theory at Leading Order
- Ground state energy of dilute neutron matter at next-to-leading order in lattice chiral effective field theory
- Lattice calculations for A=3,4,6,12 nuclei using chiral effective field theory
- Spectral convexity for attractive SU(2N) fermions
- Dilute neutron matter on the lattice at next-to-leading order in chiral effective field theory
- Lattice Effective Field Theory Simulations of Nuclei
- Chiral Effective Field Theory after Thirty Years: Nuclear Lattice Simulations