In this work, we focus on different length scales within the dynamics of nucleons in conditions according to the neutron star crust, with a semiclassical molecular dynamics model, studying isospin symmetric matter at subsaturation densities. While varying the temperature, we find that a solid-liquid phase transition exists, which can be also characterized with a morphology transition. For higher temperatures, above this phase transition, we study the neutrino opacity, and find that in the liquid phase, the scattering of low momenta neutrinos remain high, even though the morphology of the structures differ significatively from those of the traditional nuclear pasta.Fil: Alcain, Pablo Nicolás. Universidad de Buenos Aires. Facultad de Ciencias...
International audienceContext. The interior of a neutron star is expected to exhibit different state...
International audienceContext. The interior of a neutron star is expected to exhibit different state...
International audienceContext. The interior of a neutron star is expected to exhibit different state...
The study of neutron rich matter, present in neutron star, proto-neutron stars and core-collapse sup...
International audienceThe abundance of large clusters of nucleons in neutron-rich matter at subnucle...
International audienceThe abundance of large clusters of nucleons in neutron-rich matter at subnucle...
International audienceThe abundance of large clusters of nucleons in neutron-rich matter at subnucle...
A first order phase transition at high baryon density implies that a mixed phase can occupy a signif...
Ideal nuclear matter is expected to undergo a first order phase transition at the thermodynamic limi...
We investigate the structure attained by neutron star matter with proton to neutron ratios ranging f...
Cold and isospin-symmetric nuclear matter at sub-saturation densities is known to form the so-called...
International audienceDense matter as it can be found in core-collapse supernovae and neutron stars ...
International audienceDense matter as it can be found in core-collapse supernovae and neutron stars ...
International audienceContext. The interior of a neutron star is expected to exhibit different state...
Open AccessDense matter as it can be found in core-collapse supernovae and neutron stars is expected...
International audienceContext. The interior of a neutron star is expected to exhibit different state...
International audienceContext. The interior of a neutron star is expected to exhibit different state...
International audienceContext. The interior of a neutron star is expected to exhibit different state...
The study of neutron rich matter, present in neutron star, proto-neutron stars and core-collapse sup...
International audienceThe abundance of large clusters of nucleons in neutron-rich matter at subnucle...
International audienceThe abundance of large clusters of nucleons in neutron-rich matter at subnucle...
International audienceThe abundance of large clusters of nucleons in neutron-rich matter at subnucle...
A first order phase transition at high baryon density implies that a mixed phase can occupy a signif...
Ideal nuclear matter is expected to undergo a first order phase transition at the thermodynamic limi...
We investigate the structure attained by neutron star matter with proton to neutron ratios ranging f...
Cold and isospin-symmetric nuclear matter at sub-saturation densities is known to form the so-called...
International audienceDense matter as it can be found in core-collapse supernovae and neutron stars ...
International audienceDense matter as it can be found in core-collapse supernovae and neutron stars ...
International audienceContext. The interior of a neutron star is expected to exhibit different state...
Open AccessDense matter as it can be found in core-collapse supernovae and neutron stars is expected...
International audienceContext. The interior of a neutron star is expected to exhibit different state...
International audienceContext. The interior of a neutron star is expected to exhibit different state...
International audienceContext. The interior of a neutron star is expected to exhibit different state...