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In this work, we focus on different length scales within the dynamics ofnucleons in conditions according to the neutron star crust, with asemiclassical molecular dynamics model, studying isospin symmetric matter atsubsaturation densities. While varying the temperature, we find that asolid-liquid phase transition exists, that can be also characterized with amorphology transition. For higher temperatures, above this phase transition, westudy the neutrino opacity, and find that in the liquid phase, the scatteringof low momenta neutrinos remain high, even though the morphology of thestructures differ significatively from those of the traditional nuclear pasta.

Beyond Nuclear Pasta: Phase Transitions and Neutrino Opacity of Non-Traditional Pasta