Nuclear pasta structures and the charge screening effect

Abstract

Non uniform structures of the nucleon matter at subnuclear densities are numerically studied by means of the density functional theory with relativistic mean-fields coupled with the electric field. A particular role of the charge screening effects is demonstrated.

11 pages, 9 figures, submitted to PRC

References in corpus (19)

• Phase separation in asymmetrical fermion superfluids
• The Minimal CFL-Nuclear Interface
• Neutrino-pasta scattering: the opacity of nonuniform neutron-rich matter
• First Order Kaon Condensate
• Charge Screening at First Order Phase Transitions and Hadron - Quark Mixed Phase
• Simulation of Transitions between "Pasta" Phases in Dense Matter
• Quantum Molecular Dynamics Approach to the Nuclear Matter Below the Saturation Density
• Kaon Condensation in Proto-Neutron Star Matter
• Thermodynamic properties of nuclear "pasta" in neutron star crusts
• Charge Screening at First Order Phase Transitions
• First Order Phase Transitions in Neutron star Matter: Droplets and Coherent Neutrino Scattering
• Phase Structure of 2-Flavor Quark Matter: Heterogeneous Superconductors
• Microscopic Study of Slablike and Rodlike Nuclei: Quantum Molecular Dynamics Approach
• Color Superconductivity in Asymmetric Matter
• Surface Tension between Kaon Condensate and Normal Nuclear Matter Phase
• First Order Kaon Condensation in Neutron Stars: Finite Size Effects in the Mixed Phase
• Electron screening in the liquid-gas mixed phases of nuclear matter
• Numerical study of the hadron-quark mixed phase
• Protoneutron Stars with Kaon Condensation and their Delayed Collapse

Cited by in corpus (145)

• Equations of state for supernovae and compact stars
• From hadrons to quarks in neutron stars: a review
• Physics of Neutron Star Crusts
• Skyrme Interaction and Nuclear Matter Constraints
• Statistical Model for a Complete Supernova Equation of State
• Constraints on the high-density nuclear equation of state from the phenomenology of compact stars and heavy-ion collisions
• Neutron star radii and crusts: uncertainties and unified equations of state
• Core-crust transition in neutron stars: predictivity of density developments
• Inner crust of neutron stars with mass-fitted Skyrme functionals
• Dynamical response of the nuclear pasta in neutron star crusts
• Unified treatment of sub-saturation stellar matter at zero and finite temperature
• Hadron-quark mixed phase in hyperon stars
• Nuclear Pasta Formation
• Equation of state and thickness of the inner crust of neutron stars
• Formation of Nuclear "Pasta" in Supernovae
• Solution of the Hyperon Puzzle within a Relativistic Mean-Field Model
• Finite-size effects at the hadron-quark transition and heavy hybrid stars
• Thermodynamics of isospin-asymmetric nuclear matter from chiral effective field theory
• The pasta phase within density dependent hadronic models
• The Vlasov formalism for extended relativistic mean field models: the crust-core transition and the stellar matter equation of state
• Semi-classical equation of state and specific heats for neutron-star inner crust with proton shell corrections
• Non-congruence of the nuclear liquid-gas and deconfinement phase transitions
• Nuclear symmetry energy and core-crust transition in neutron stars: a critical study
• Phase diagram of nuclear "pasta" and its uncertainties in supernova cores
• Warm pasta phase in the Thomas-Fermi approximation
• Neutron skins and neutron stars
• Low-energy collective excitations in the neutron star inner crust
• The neutron star inner crust and symmetry energy
• Delta isobars in relativistic mean-field models with $\sigma$-scaled hadron masses and couplings
• Statistical description of complex nuclear phases in supernovae and proto-neutron stars
• Nuclear Equation of state for Compact Stars and Supernovae
• Nuclear Waffles
• Effects of the symmetry energy on properties of neutron star crusts near the neutron drip density
• Conditions for Phase Equilibrium in Supernovae, Proto-Neutron and Neutron Stars
• Appearance of the Single Gyroid Network Phase in Nuclear Pasta Matter
• Relativistic Mean-Field Models with Scaled Hadron Masses and Couplings: Hyperons and Maximum Neutron Star Mass
• Finite size effects on kaonic pasta structures
• Nuclear "pasta" structures in low-density nuclear matter and neutron star crust
• Nuclear medium cooling scenario in the light of new Cas A cooling data and the 2 M_sun pulsar mass measurements
• Light clusters, pasta phases and phase transitions in core-collapse supernova matter
• Imprint of the symmetry energy on the inner crust and strangeness content of neutron stars
• Quantum Nuclear Pasta and Nuclear Symmetry Energy
• Building a realistic neutron star from holography
• Uncertainties in the pasta-phase properties of catalysed neutron stars
• Cluster formation in compact stars: relativistic versus Skyrme models
• Electronic phase separation: recent progress in the old problem
• Hybrid Stars using the Quark-Meson Coupling and Proper Time NJL Models
• Topological characterization of neutron star crusts
• Influence of the symmetry energy on nuclear pasta in neutron star crusts
• Three dimensional structure of low-density nuclear matter
• Impact of nuclear "pasta" on neutrino transport in collapsing stellar cores
• Hydrodynamical description of first-order phase transitions: Analytical treatment and numerical modeling
• Glitches in rotating supersolids
• A Neutron Star is born
• Unified neutron star EOSs and neutron star structures in RMF models
• Light clusters and the pasta phase
• Influence of the stiffness of the equation of state and in-medium effects on the cooling of compact stars
• Hot hadron-quark mixed phase including hyperons
• $\alpha$ particles and the pasta phase
• Anomalous thermodynamics and phase transitions of neutron-star matter
• Nuclear Pasta Matter for Different Proton Fractions
• Equation of State for Hot and Dense Matter: $\sigma$-$\omega$-$\rho$ Model with Scaled Hadron Masses and Couplings
• Fermi-to-Bose crossover in a trapped quasi-2D gas of fermionic atoms
• Liquid-gas coexistence vs. energy minimization with respect to the density profile in the inhomogeneous inner crust of neutron stars
• Full distribution of clusters with universal couplings and in-medium effects
• Magnetization of a neutron plasma with Skyrme and Gogny forces in the presence of a strong magnetic field
• Quantum Simulations of Nuclei and Nuclear Pasta with the Multi-resolution Adaptive Numerical Environment for Scientific Simulations
• Effect of strong magnetic fields on the crust-core transition and inner crust of neutron stars
• The pasta phase and its consequences on neutrino opacities
• Effect of Coulomb Screening Length on Nuclear Pasta Simulations
• Domains and defects in nuclear "pasta"
• Dense Matter in Neutron Stars with eXTP
• Chiral pasta
• Inference of neutron-star properties with unified crust-core equations of state for parameter estimation
• The effect of the energy functional on the pasta-phase properties of catalysed neutron stars
• Phase transitions in Core-Collapse Supernova Matter at sub-saturation densities
• Neutron Fermi Liquids under the presence of a strong magnetic field with effective nuclear forces
• Shear oscillations in the hadron-quark mixed phase
• Cooling of neutron stars in "nuclear medium cooling scenario" with stiff equation of state including hyperons
• Surface tension of the core-crust interface of neutron stars with global charge neutrality
• Proton fraction in the inner neutron-star crust
• Effect of Inner Crust EoS on Neutron star properties
• Pasta properties of the neutron star within effective relativistic mean-field model
• A new statistical method for the structure of the inner crust of neutron stars
• Nuclear pasta structures and symmetry energy
• Unified nuclear matter EOSs constrained by the in-medium balance in density-dependent covariant density functionals
• Curvature effect on nuclear pasta: Is it helpful for gyroid appearance?
• Ising analogue to compact-star matter
• Pasta phases within the QMC model
• Detectability of a phase transition in neutron star matter with third-generation gravitational wave interferometers
• Supercritically charged objects and electron-positron pair creation
• Interface effects of quark matter: Light-quark nuggets and compact stars
• Molecular Dynamics for Dense Matter
• Response of spin polarized neutron matter under the presence of a strong magnetic field with Skyrme interactions
• Structure formation during phase transitions in strongly interacting matter
• Pasta fluctuations in symmetric matter at finite temperature
• Quark-hadron pasta phase in neutron stars: the role of medium-dependent surface and curvature tensions
• Warm unstable asymmetric nuclear matter: critical properties and the density dependence of the symmetry energy
• Dynamical instabilities in density-dependent hadronic relativistic models
• The proto-neutron star inner crust in the liquid phase
• Self consistent calculation of the nuclear composition in hot and dense stellar matter
• Relativistic equation of state at subnuclear densities in the Thomas-Fermi approximation
• Scalar quanta in Fermi liquids: zero sounds, instabilities, Bose condensation, and a metastable state in dilute nuclear matter
• Nuclear pasta and symmetry energy in the relativistic point-coupling model
• The proto-neutron star inner crust in a multi-component plasma approach
• Effects of finite size and symmetry energy on the phase transition of stellar matter at subnuclear densities
• Application of superconducting-superfluid magnetohydrodynamics to nuclear "pasta" in neutron stars
• Strong magnetic fields and pasta phases revisited
• Generalized skyrmion crystals with applications to neutron stars
• Parametrization of the surface energy in the ETF approximation
• Neutrino diffusion in the pasta phase matter within the Thomas-Fermi approach
• Strong magnetic fields: neutron stars with an extended inner crust
• Fluctuations in the pasta phase
• Shell States of Neutron Rich Matter
• Charged Ising Model of Neutron Star Matter
• Bayesian inference of neutron star crust properties using an ab initio-benchmarked meta-model
• RMF models with $\sigma$-scaled hadron masses and couplings for description of heavy-ion collisions below 2A GeV
• Emergence of non-trivial minimizers for the three-dimensional Ohta-Kawasaki energy
• Nuclear pasta structures at high temperatures
• Light clusters in the liquid proto-neutron star inner crust
• Phase diagram of neutron-rich nuclear matter and its impact on astrophysics
• Pairing effects in nuclear pasta phase within the relativistic Thomas-Fermi formalism
• Effects of inner crusts on $g$-mode oscillations in neutron stars
• Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches
• The effects of medium on nuclear properties in multifragmentation
• Strongly interacting matter in extreme magnetic fields
• Do short range correlations inhibit the appearance of the nuclear pasta?
• Binding energies and modelling of nuclei in semiclassical simulations
• Nuclear collision in strong magnetic field
• Preliminary EoS for core-collapse supernova simulations with the QMC model
• The role of the electric Bond number in the stability of pasta phases
• Properties and microscopic structures of dense stellar matter in RMF models
• Liquid-gas mixed phase in nuclear matter at finite temperature
• Some aspects of the phase diagram of nuclear matter relevant to compact stars
• Pressure and chemical potentials in the inner crust of a cold neutron star within Hartree-Fock and extended Thomas-Fermi methods
• Unified treatment for in-medium light and heavy clusters with RMF models
• Inner crust equations of state for CompOSE
• Characterization of the inner edge of the neutron star crust
• Isospin-Asymmetry Dependence of the Thermodynamic Nuclear Equation of State in Many-Body Perturbation Theory
• Thermodynamics of compact-star matter within an ising approach
• Neutron-rich nuclei and the equation of state of stellar matter
• Finite temperature collective modes in a two phase coexistence region of asymmetric nuclear matter
• Non-Uniform Structure of Matter and the Equation of State
• Evolution of quasiperiodic structures in non-ideal hydrodynamic description of phase transitions
• The phases of QCD reached in terrestrial and cosmic colliders