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Actinide Crystallization and Fission Reactions in Cooling White Dwarf Stars

C. J. Horowitz*

M. E. Caplan†

  • Center for Exploration of Energy and Matter and Department of Physics, Indiana University, Bloomington, Indiana 47405, USA

  • Illinois State University, Department of Physics, Normal, Illinois 61790, USA

  • *horowit@indiana.edu
  • †mecapl1@ilstu.edu

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 Z5/3 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.

Physics Subject Headings (PhySH)

Focus

Fission Chain Reaction May Trigger Supernovae

Published 29 March, 2021

White dwarf explosions may be initiated by uranium in the stellar core detonating like a nuclear weapon.

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