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Properties of nuclear pastas
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June 1973 |
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A comparative study of Hartree-Fock iteration techniques
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April 1982 |
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Self-consistent study of triaxial deformations: Application to the isotopes of Kr, Sr, Zr and Mo
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Thermodynamic properties of nuclear “pasta” in neutron star crusts
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Band structure effects for dripped neutrons in neutron star crust
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Simulations of cold nuclear matter at sub-saturation densities
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Phase transitions and symmetry energy in nuclear pasta
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A highly resistive layer within the crust of X-ray pulsars limits their spin periods
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Equation of State and Neutron star Properties Constrained by Nuclear Physics and Observation
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A Survey of the Parameter Space of the Compressible Liquid drop Model as Applied to the Neutron star Inner Crust
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The Cooling of the Cassiopeia a Neutron star as a Probe of the Nuclear Symmetry Energy and Nuclear Pasta
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Bulk viscosity in a neutron star mantle
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Survey of nuclear pasta in the intermediate-density regime: Shapes and energies
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Elastic properties of phases with nonspherical nuclei in dense matter
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May 2020 |
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Survey of nuclear pasta in the intermediate-density regime: Structure functions for neutrino scattering
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May 2020 |
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Nuclear pasta in hot and dense matter and its influence on the equation of state for astrophysical simulations
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July 2020 |
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Fast neutrino cooling of nuclear pasta in neutron stars: Molecular dynamics simulations
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Proton superconductivity in pasta phases in neutron star crusts
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Thermal fluctuations in nuclear pasta
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Quantum molecular dynamics approach to the nuclear matter below the saturation density
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Structure of the inner crust of neutron stars: Crystal lattice or disordered phase?
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Neutrino-“pasta” scattering: The opacity of nonuniform neutron-rich matter
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Dynamical response of the nuclear “pasta” in neutron star crusts
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Fusion reactions in multicomponent dense matter
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Nuclear matter in the crust of neutron stars
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Nuclear matter in the crust of neutron stars derived from realistic NN interactions
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Phase diagram of nuclear “pasta” and its uncertainties in supernova cores
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Shear viscosity and thermal conductivity of nuclear “pasta”
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Modeling nuclear “pasta” and the transition to uniform nuclear matter with the 3D Skyrme-Hartree-Fock method at finite temperature: Core-collapse supernovae
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May 2009 |
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Simple analytic model for astrophysical S factors
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October 2010 |
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Curvature effect on nuclear “pasta”: Is it helpful for gyroid appearance?
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Topological characterization of neutron star crusts
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Time-dependent Hartree-Fock approach to nuclear “pasta” at finite temperature
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Nuclear “pasta” formation
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Nuclear “pasta matter” for different proton fractions
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Appearance of the single gyroid network phase in “nuclear pasta” matter
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Pasta nucleosynthesis: Molecular dynamics simulations of nuclear statistical equilibrium
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Twist-averaged boundary conditions for nuclear pasta Hartree-Fock calculations
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Quantum Monte Carlo calculations of neutron matter with chiral three-body forces
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Time-dependent density functional theory with twist-averaged boundary conditions
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Asymmetric nuclear matter based on chiral two- and three-nucleon interactions
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May 2016 |
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Quantum simulations of nuclei and nuclear pasta with the multiresolution adaptive numerical environment for scientific simulations
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May 2016 |
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Effect of topological defects on “nuclear pasta” observables
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Low-density nuclear matter with quantum molecular dynamics: The role of the symmetry energy
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August 2016 |
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“Parking-garage” structures in nuclear astrophysics and cellular biophysics
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Quantum nuclear pasta and nuclear symmetry energy
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Domains and defects in nuclear pasta
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Gyroid Phase in Nuclear Pasta
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Exploring the Nuclear Pasta Phase in Core-Collapse Supernova Matter
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Disordered Nuclear Pasta, Magnetic Field Decay, and Crust Cooling in Neutron Stars
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Colloquium : Astromaterial science and nuclear pasta
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Pycnonuclear burning of34Ne in accreting neutron stars
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Fictive Temperature and the Glassy State
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Superfluid Liquid Crystals: Pasta Phases in Neutron Star Crusts
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The equation of state of neutron matter, symmetry energy and neutron star structure
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Shape of Nuclei in the Crust of Neutron Star
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Further Study of the Nuclear Shape in High-Density Matter
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Transport Properties of the Nuclear Pasta Phase with Quantum Molecular Dynamics
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Prior Probability Distributions of Neutron Star Crust Models
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