2024/10/17 by D. A. Baiko, Baiko, D. A.
Materials Science · Physics and Astronomy · #Crystal Structures and Properties #FOS: Physical sciences #Solar and Stellar Astrophysics (astro-ph.SR) #Solid-state spectroscopy and crystallography #Stellar, planetary, and galactic studies
paper · pdf · doi:10.48550/arxiv.2410.13745
openalex publication_date 2024/10/17 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Thermal evolution of the central region of a 0.9 M_\odot C/O white dwarf at the initial stage of the ion mixture crystallization is studied by numerically solving the heat equation on a fine spatial and temporal grid and by including a detailed treatment of the latent heat release. Formation of two spherical shells is observed. The outer one surrounds a region where crystallization has begun. The inner one bounds a fully solidified core which has exhausted its latent heat. The region between the shells is partially liquid and partially solid. It gradually emits the latent heat of crystallization and also it releases light elements (carbon) in the process of element redistribution, accompanying the mixture solidification. Assuming that all released light elements cross the outer shell, we have estimated their flux induced by the mixture crystallization. The resulting flux is not divergent and is much smaller than an estimate derived from the growth rate of the fully crystallized core.