A review of Type Ia supernovae covering their physics, observational diversity, progenitor scenarios, and open questions, with no new research results.
Actinide crystallization and fission reactions in cooling white dwarf stars
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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 $Z^{5/3}$ and actinides have the largest charge $Z$. 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.
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2024 1verdicts
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Type Ia supernovae
A review of Type Ia supernovae covering their physics, observational diversity, progenitor scenarios, and open questions, with no new research results.