Non-perturbative Extraction of the Effective Mass in Neutron Matter
arXiv:1901.00870 · doi:10.1103/PhysRevLett.122.152701
Abstract
We carry out non-perturbative calculations of the single-particle excitation spectrum in strongly interacting neutron matter. These are microscopic quantum Monte Carlo computations of many-neutron energies at different densities as well as several distinct excited states. As input, we employ both phenomenological and chiral two- and three-nucleon interactions. We use the single-particle spectrum to extract the effective mass in neutron matter. With a view to systematizing the error involved in this extraction, we carefully assess the impact of finite-size effects on the quasiparticle dispersion relation. We find an effective-mass ratio that drops from 1 as the density is increased. We conclude by connecting our results with the physics of ultracold gases as well as with energy-density functional theories of nuclei and neutron-star matter.
arXiv comment5+ pages, 3 figures; v2 corresponds to published version
References in corpus (53)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- The equation of state for nucleon matter and neutron star structure
- Quantum Monte Carlo calculations of nuclei with A \leq 7
- Revealing the Superfluid Lambda Transition in the Universal Thermodynamics of a Unitary Fermi Gas
- The maximum mass and radius of neutron stars and the nuclear symmetry energy
- Chiral three-nucleon forces and neutron matter
- Relativistic effective interaction for nuclei, giant resonances, and neutron stars
- A critical examination of constraints on the equation of state of dense matter obtained from GW170817
- Evolution of Nuclear Spectra with Nuclear Forces
- Quantum Monte Carlo Calculations with Chiral Effective Field Theory Interactions
- Asymmetric Two-component Fermion Systems in Strong Coupling
- Normal state of a polarized Fermi gas at unitarity
- Local chiral effective field theory interactions and quantum Monte Carlo applications
- Low-density neutron matter
- Strongly paired fermions: Cold atoms and neutron matter
- Nucleon Effective Masses in Neutron-Rich Matter
- Renormalization group approach to neutron matter: quasiparticle interactions, superfluid gaps and the equation of state
- Coupled-cluster calculations of nucleonic matter
- Leading chiral three-nucleon forces along isotope chains in the calcium region
- Quantum Monte Carlo calculation of the equation of state of neutron matter
- Quantum Monte Carlo Calculations of Neutron Matter
- Quantum Monte Carlo calculations of neutron matter with chiral three-body forces
- Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. IX: Constraint of pairing force to neutron-matter gap
- Resonant Fermi gases with a large effective range
- Light-nuclei spectra from chiral dynamics
- Neutron Matter from Low to High Density
- Microscopic calculations and energy expansions for neutron-rich matter
- Reduced regulator dependence of neutron-matter predictions with chiral interactions
- Cold neutrons trapped in external fields
- Correlated density-dependent chiral forces for infinite matter calculations within the Green's function approach
- Properties of nuclei up to using local chiral interactions
- Quantum Monte Carlo calculations of neutron matter with non-local chiral interactions
- Auxiliary-Field Quantum Monte Carlo Simulations of Neutron Matter in Chiral Effective Field Theory
- Comparative study of neutron and nuclear matter with simplified Argonne nucleon-nucleon potentials
- Ground state energy of dilute neutron matter at next-to-leading order in lattice chiral effective field theory
- Neutron Drops and Skyrme Energy-Density Functionals
- Linear response theory and neutrino mean free path using Brussels-Montreal Skyrme functionals
- Linear response of homogeneous nuclear matter with energy density functionals
- Generic Constraints on the Relativistic Mean-Field and Skyrme-Hartree-Fock Models from the Pure Neutron Matter Equation of State
- Constraints on Skyrme Equations of State from Properties of Doubly Magic Nuclei and Ab-Initio Calculations of Low-Density Neutron Matter
- Static Response of Neutron Matter
- Auxiliary Field Diffusion Monte Carlo calculation of ground state properties of neutron drops
- Microscopically constrained mean field models from chiral nuclear thermodynamics
- Resummation of in-medium ladder diagrams: s-wave effective range and p-wave interaction
- Ab Initio study of neutron drops with chiral Hamiltonians
- Ab initio and phenomenological studies of the static response of neutron matter
- Constraining the nuclear energy density functional with quantum Monte Carlo calculations
- The neutron polaron as a constraint on nuclear density functionals
- Energy-density functionals inspired by effective-field theories: Applications to neutron drops
- Di-neutrons in neutron matter within Brueckner-Hartree-Fock approach
- Effect of three-body forces on response functions in infinite neutron matter
- Static response, collective frequencies and ground state thermodynamical properties of spin saturated two-component cold atoms and neutron matter
- Beyond--mean--field effective masses in the nuclear Fermi liquid from axial breathing modes
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- New equations of state constrained by nuclear physics, observations, and QCD calculations of high-density nuclear matter
- constraints on thermal effects of the nuclear equation of state
- Benchmark calculations of infinite neutron matter with realistic two- and three-nucleon potentials
- Neutron Star Matter as a Relativistic Fermi Liquid
- 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
- Model nuclear energy density functionals derived from ab initio calculations
- Pairing in pure neutron matter
- Machine-learning approach to finite-size effects in systems with strongly interacting fermions
- Approximate self-energy for Fermi systems with large s-wave scattering length: a step towards density functional theory
- Satisfying the compressibility sum rule in neutron matter
- Polaronic Proton and Diproton Clustering in Neutron-Rich Matter
- BCS-BEC Crossover Effects and Pseudogap in Neutron Matter
- Finite-temperature infinite matter with effective-field-theory-inspired energy-density functionals
- Skyrme-based extrapolation for the static response of neutron matter
- Properties of fermionic systems with the Path-integral ground state method
- Neutron matter at the interface(s): static response and effective mass