Towards order-by-order calculations of the nuclear and neutron matter equations of state in chiral effective field theory
arXiv:1411.0136 · doi:10.1103/PhysRevC.91.054311
Abstract
We calculate the nuclear and neutron matter equations of state from microscopic nuclear forces at different orders in chiral effective field theory and with varying momentum-space cutoff scales. We focus attention on how the order-by-order convergence depends on the choice of resolution scale and the implications for theoretical uncertainty estimates on the isospin asymmetry energy. Specifically we study the equations of state using consistent NLO and N2LO (next-to-next-to-leading order) chiral potentials where the low-energy constants cD and cE associated with contact vertices in the N2LO chiral three-nucleon force are fitted to reproduce the binding energies of 3H and 3He as well as the beta-decay lifetime of 3H. At these low orders in the chiral expansion there is little sign of convergence, while an exploratory study employing the N3LO two-nucleon force together with the N2LO three-nucleon force give first indications for (slow) convergence with low-cutoff potentials and poor convergence with higher-cutoff potentials. The consistent NLO and N2LO potentials described in the present work provide the basis for estimating theoretical uncertainties associated with the order-by-order convergence of nuclear many-body calculations in chiral effective field theory.
arXiv comment9 pages, 6 figures. Accepted for publication in Physical Review C
References in corpus (41)
- Chiral effective field theory and nuclear forces
- Accurate Charge-Dependent Nucleon-Nucleon Potential at Fourth Order of Chiral Perturbation Theory
- A New Expansion for Nucleon-Nucleon Interactions
- Constraints on the symmetry energy and neutron skins from experiments and theory
- Two-Nucleon Systems from Effective Field Theory
- Improved nuclear matter calculations from chiral low-momentum interactions
- Chiral three-nucleon forces and neutron matter
- Neutron matter at next-to-next-to-next-to-leading order in chiral effective field theory
- Renormalization of One-Pion Exchange and Power Counting
- Nucleon-Nucleon Scattering from Effective Field Theory
- Quantum Monte Carlo Calculations with Chiral Effective Field Theory Interactions
- Three-Nucleon Low-Energy Constants from the Consistency of Interactions and Currents in Chiral Effective Field Theory
- Subleading contributions to the chiral three-nucleon force I: long-range terms
- Neutron matter from chiral effective field theory interactions
- Is nuclear matter perturbative with low-momentum interactions?
- Subleading contributions to the chiral three-nucleon force II: Short-range terms and relativistic corrections
- Coupled-cluster calculations of nucleonic matter
- Density-dependent effective nucleon-nucleon interaction from chiral three-nucleon forces
- The nuclear matter equation of state with consistent two- and three-body perturbative chiral interactions
- Microscopic calculations and energy expansions for neutron-rich matter
- A recipe for EFT uncertainty quantification in nuclear physics
- Reduced regulator dependence of neutron-matter predictions with chiral interactions
- Chiral effective field theory predictions for muon capture on deuteron and 3He
- Electromagnetic structure of A=2 and 3 nuclei in chiral effective field theory
- Microscopic calculations in asymmetric nuclear matter
- Correlated density-dependent chiral forces for infinite matter calculations within the Green's function approach
- Two-pion exchange three-nucleon potential: O(q^4) chiral expansion
- 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
- Efficient calculation of chiral three-nucleon forces up to N3LO for ab initio studies
- Nuclear thermodynamics from chiral low-momentum interactions
- How low-energy weak reactions can constrain three-nucleon forces and the neutron-neutron scattering length
- Chiral three-nucleon interaction and the carbon-14 dating beta decay
- Four-nucleon force using the method of unitary transformation
- Effect of three-nucleon interaction in p-3He elastic scattering
- The proton-proton weak capture in chiral effective field theory
- Nonperturbative renormalization of the chiral nucleon-nucleon interaction up to next-to-next-to-leading order
- Coupled-cluster studies of infinite nuclear matter
- Dirac-Brueckner-Hartree-Fock versus chiral effective field theory
- A chiral effective field theory study of hadronic parity violation in few-nucleon systems
- Exact calculation of three-body contact interaction to second order
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- Nuclear saturation in lowest-order Brueckner theory with two- and three-nucleon forces in view of chiral effective field theory
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- Reconciling light nuclei and nuclear matter: relativistic calculations
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- Impact of the neutron matter equation of state on neutron skin and neutron drip lines in chiral effective field theory
- Isoscalar Giant Monopole Resonance in Spherical Nuclei as a Nuclear Matter Incompressibility Indicator
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- Constraining gravity with hadron physics: neutron stars, modified gravity and gravitational waves
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- Isospin-Asymmetry Dependence of the Thermodynamic Nuclear Equation of State in Many-Body Perturbation Theory
- Properties of hyperons in nuclear matter from chiral hyperon-nucleon interactions at next-to-next-to-leading order
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- An overview of symmetric nuclear matter properties from chiral interactions up to fourth order of the chiral expansion