Spin-polarized low-density neutron matter
arXiv:1012.4464 · doi:10.1103/PhysRevC.83.065801
Abstract
Low-density neutron matter is relevant to the study of neutron-rich nuclei and neutron star crusts. Unpolarized neutron matter has been studied extensively over a number of decades, while experimental guidance has recently started to emerge from the field of ultracold atomic gases. In this work, we study population-imbalanced neutron matter (possibly relevant to magnetars and to density functionals of nuclei) applying a Quantum Monte Carlo method that has proven successful in the field of cold atoms. We report on the first ab initio simulations of superfluid low-density polarized neutron matter. For systems with small imbalances, we find a linear dependence of the energy on the polarization, the proportionality coefficient being dependent on the density. We also present results for the momentum and pair distributions of the two fermionic components.
8 pages, 3 figures, 1 table; v2 corresponds to the published version
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Cited by in corpus (7)
- Quantum Monte Carlo Calculations with Chiral Effective Field Theory Interactions
- Resummation of in-medium ladder diagrams: s-wave effective range and p-wave interaction
- Path integral contour deformations for noisy observables
- The neutron polaron as a constraint on nuclear density functionals
- Phase separation in low-density neutron matter
- Fermi polaron in low-density spin-polarized neutron matter
- Ab initio study of the neutron and Fermi polarons on the lattice