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Actinide Crystallization and Fission Reactions in Cooling White Dwarf Stars
Phys. Rev. Lett. 126, 131101 – Published 29 March, 2021
DOI: https://doi.org/10.1103/PhysRevLett.126.131101
Abstract
The first solids that form as a cooling white dwarf (WD) starts to crystallize are expected to be greatly enriched in actinides. This is because the melting points of WD matter scale as and actinides have the largest charge . We estimate that the solids may be so enriched in actinides that they could support a fission chain reaction. This reaction could ignite carbon burning and lead to the explosion of an isolated WD in a thermonuclear supernova (SN Ia). Our mechanism could potentially explain SN Ia with sub-Chandrasekhar ejecta masses and short delay times.
Physics Subject Headings (PhySH)
Focus
Fission Chain Reaction May Trigger Supernovae
White dwarf explosions may be initiated by uranium in the stellar core detonating like a nuclear weapon.
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