Beyond Nuclear Pasta: Phase Transitions and Neutrino Opacity of Non-Traditional Pasta
arXiv:1406.1550 · doi:10.1103/PhysRevC.90.065803
Abstract
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, that 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.
12 pages, 10 figures
References in corpus (1)
Cited by in corpus (7)
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- Proton superconductivity in pasta phases in neutron star crusts
- The role of the electric Bond number in the stability of pasta phases