Spin-orbit induced backflow in neutron matter with auxiliary field diffusion Monte Carlo
arXiv:nucl-th/0304042 · doi:10.1103/PhysRevC.67.065806
Abstract
The energy per particle of zero-temperature neutron matter is investigated, with particular emphasis on the role of the interaction. An analysis of the importance of explicit spin--orbit correlations in the description of the system is carried out by the auxiliary field diffusion Monte Carlo method. The improved nodal structure of the guiding function, constructed by explicitly considering these correlations, lowers the energy. The proposed spin--backflow orbitals can conveniently be used also in Green's Function Monte Carlo calculations of light nuclei.
4 pages, 1 figure
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Cited by in corpus (13)
- Quantum Monte Carlo calculation of the equation of state of neutron matter
- Nuclear and neutron-star matter from local chiral interactions
- Neutron matter at zero temperature with auxiliary field diffusion Monte Carlo
- Benchmark calculations of pure neutron matter with realistic nucleon-nucleon interactions
- superfluid phase--transition in neutron matter with realistic nuclear potentials and modern many--body theories
- Auxiliary Field Diffusion Monte Carlo calculation of ground state properties of neutron drops
- Benchmark calculations of infinite neutron matter with realistic two- and three-nucleon potentials
- Spin-orbit and tensor interactions in homogeneous matter of nucleons: accuracy of modern many-body theories
- Mg impurity in helium droplets
- Quantum Monte Carlo study of dilute neutron matter at finite temperatures
- Spin-orbit correlation energy in neutron matter
- The Auxiliary Field Diffusion Monte Carlo Method for Nuclear Physics and Nuclear Astrophysics
- Quantum Monte Carlo method applied to strongly correlated dilute fermi gases with finite effective range