3 papers
astro-ph.EP2026
The evolution and internal structure of Neptunes and sub-Neptunes II. Convective mixing and thermal conductivity
Mark Eberlein, Ravit Helled
Sub-Neptunes and Neptunes are often modeled with distinct, fully convective layers. Yet, there are several arguments for compositions gradients that can inhibit convection. In thes…
astro-ph.EP2026
The Evolution and Internal Structure of Neptunes and Sub-Neptunes: The importance of thermal conductivity in non-convective regions
Mark Eberlein, Ravit Helled
Neptunes and sub-Neptunes are typically modeled under the assumption that the interior is adiabatic and consists of distinct layers. However, formation models indicate that composi…
astro-ph.GA2025
Dark Matter Particle Flux in a Dynamically Self-consistent Milky Way Model
Lucijana Stanic, Mark Eberlein, Stanislav Linchakovskyy +5
We extend a recently developed dynamically self-consistent model of the Milky Way constrained by observations from the Gaia observatory to include a radially anisotropic component…