Glassy quantum nuclear pasta in neutron star crusts
William G. Newton, Mark Alexander Kaltenborn, Sarah Cantu, Shuxi Wang,, Amber Stinson, Jirina Rikovska Stone

TL;DR
This study uses 3D Hartree-Fock+BCS calculations to explore nuclear pasta phases in neutron star crusts, revealing a glassy, disordered state with multiple coexisting configurations affecting the crust's transport properties.
Contribution
It provides the first detailed survey of nuclear pasta shapes and their energy landscapes, supporting the glassy nature and domain formation in neutron star crusts.
Findings
Nuclear pasta phases occupy large regions of the crust.
Multiple pasta configurations coexist at given depths.
Protons become delocalized in bi-continuous phases.
Abstract
We investigate the nuclear pasta phases in neutron star crusts by conducting a large number of three-dimensional Hartree-Fock+BCS calculations at densities leading to the crust-core transition. We survey the shape parameter space of pasta at constant pressure. Spaghetti, waffles, lasagna, bi-continuous phases and cylindrical holes occupy local minima in the resulting Gibbs energy surfaces. The bi-continuous phase, in which both the neutron gas and nuclear matter extend continuously in all dimensions and therefore protons are delocalized, appears over a large range of depths. Our results support the idea that nuclear pasta is a glassy system. Multiple pasta configurations coexist in a given layer of the crust. At a characteristic temperature, of order -K, different phases become frozen into domains whose sizes we estimate to be 1-50 times the lattice spacing and over which…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
