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arXiv · 0803.1388

From nuclear multifragmentation reactions to supernova explosions

Igor N. Mishustin
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Abstract

In this talk I discuss properties of hot stellar matter at sub-nuclear densities which is formed in supernova explosions. I emphasize that thermodynamic conditions there are rather similar to those created in the laboratory by intermediate-energy heavy-ion collisions. Theoretical methods developed for the description of multi-fragment final states in such reactions can be used also for description of the stellar matter. I present main steps of the statistical approach to the equation of state and nuclear composition, dealing with an ensemble of nuclear species instead of one "average" nucleus.

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Igor N. Mishustin. 2008-03-10. From nuclear multifragmentation reactions to supernova explosions. https://arxiv.org/abs/0803.1388

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