Crystallization onset in white dwarfs

\nWe studied the thermal evolution of the central region of a 0.9 M⊙ C/O white dwarf at the initial stage of ion mixture crystallization by numerically solving the heat equation on a fine spatial and temporal grid and by including a detailed treatment of the latent heat release. The 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 that has exhausted its latent heat. The region between the shells is partially liquid and partially solid. It gradually emits the latent heat generated by crystallization and also releases light elements (carbon) in the process of element redistribution, which accompanies the mixture solidification. Assuming that all released light elements cross the outer shell, we estimated the flux induced by the mixture crystallization. The resulting flux is not divergent and is much lower than the estimate derived from the growth rate of the fully crystallized core.\n

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Publication Details

Journal
Springer Link (Chiba Institute of Technology)
Published
2024-11-18
DOI
https://doi.org/10.1051/0004-6361/202452021/pdf
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
0.00

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article

Crystallization onset in white dwarfs

Springer Link (Chiba Institute of Technology)
Stellar, planetary, and galactic studies
article

Crystallization onset in white dwarfs

article en

Abstract

\nWe studied the thermal evolution of the central region of a 0.9 M⊙ C/O white dwarf at the initial stage of ion mixture crystallization by numerically solving the heat equation on a fine spatial and temporal grid and by including a detailed treatment of the latent heat release. The 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 that has exhausted its latent heat. The region between the shells is partially liquid and partially solid. It gradually emits the latent heat generated by crystallization and also releases light elements (carbon) in the process of element redistribution, which accompanies the mixture solidification. Assuming that all released light elements cross the outer shell, we estimated the flux induced by the mixture crystallization. The resulting flux is not divergent and is much lower than the estimate derived from the growth rate of the fully crystallized core.\n

Springer Link (Chiba Institute of Technology)
Ioffe Institute (RU)
Russian Science Foundation
Openalex Percentile: Top 78%
Stellar, planetary, and galactic studies
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