Image Details
Caption: Figure 1.
Dimensionless diffusion coefficients ﹩{D}^{* }=D/{\omega }_{p}{a}_{i}^{2}﹩ for Yukawa plasmas at a typical screenings for neutron star crusts. Points that cross melting are from weakly superheated (supercooled) simulations.
© 2026. The Author(s). Published by the American Astronomical Society.