Properties of nuclear pastas
In this review we study the nuclear pastas as they are expected to be formed in neutron star
crusts. We start with a study of the pastas formed in nuclear matter (composed of protons …
crusts. We start with a study of the pastas formed in nuclear matter (composed of protons …
Unified equations of state for cold nonaccreting neutron stars with Brussels-Montreal functionals. II. Pasta phases in semiclassical approximation
JM Pearson, N Chamel, AY Potekhin - Physical Review C, 2020 - APS
We generalize our earlier work on neutron stars, which assumed spherical Wigner-Seitz
cells in the inner crust, to admit the possibility of pasta phases, ie, nonspherical cell shapes …
cells in the inner crust, to admit the possibility of pasta phases, ie, nonspherical cell shapes …
Skyrme-Hartree-Fock-Bogoliubov mass models on a 3D mesh: effect of triaxial shape
The modelling of nuclear reactions and radioactive decays in astrophysical or earth-based
conditions requires detailed knowledge of the masses of essentially all nuclei. Microscopic …
conditions requires detailed knowledge of the masses of essentially all nuclei. Microscopic …
A neutron star is born
DP Menezes - Universe, 2021 - mdpi.com
A neutron star was first detected as a pulsar in 1967. It is one of the most mysterious
compact objects in the universe, with a radius of the order of 10 km and masses that can …
compact objects in the universe, with a radius of the order of 10 km and masses that can …
Unified neutron star EOSs and neutron star structures in RMF models
CJ **a, T Maruyama, A Li, BY Sun… - Communications in …, 2022 - iopscience.iop.org
In the framework of the Thomas-Fermi approximation, we systematically study the EOSs and
microscopic structures of neutron star matter in a vast density range with nb≈ 10− 10-2 fm …
microscopic structures of neutron star matter in a vast density range with nb≈ 10− 10-2 fm …
Dark particle mass effects on neutron star properties from a short-range correlated hadronic model
In this work we study a relativistic mean-field (RMF) hadronic model, with nucleonic short-
range correlations (SRC) included, coupled to dark matter (DM) through the Higgs boson …
range correlations (SRC) included, coupled to dark matter (DM) through the Higgs boson …
Impact of the neutron-star deformability on equation of state parameters
We use a Bayesian inference analysis to explore the sensitivity of Taylor expansion
parameters of the nuclear equation of state (EOS) to the neutron star dimensionless tidal …
parameters of the nuclear equation of state (EOS) to the neutron star dimensionless tidal …
Analytic multi-Baryonic solutions in the SU (N)-Skyrme model at finite density
A bstract We construct explicit analytic solutions of the SU (N)-Skyrme model (for generic N)
suitable to describe different phases of nuclear pasta at finite volume in (3+ 1) dimensions …
suitable to describe different phases of nuclear pasta at finite volume in (3+ 1) dimensions …
Unified nuclear matter equations of state constrained by the in-medium balance in density-dependent covariant density functionals
Considering the effects of charge screening, we propose a new numerical recipe within the
framework of the Thomas-Fermi approximation, where the properties of nuclear matter …
framework of the Thomas-Fermi approximation, where the properties of nuclear matter …
Structure and composition of the inner crust of neutron stars from Gogny interactions
The detailed knowledge of the inner crust properties of neutron stars might be important to
explain different phenomena such as pulsar glitches or the possibility of an r-process site in …
explain different phenomena such as pulsar glitches or the possibility of an r-process site in …