Multifragmentation reactions and properties of hot stellar matter at subnuclear densities

Details Multifragmentation reactions and properties of hot stellar matter at subnuclear densities Multifragmentation reactions and properties of hot stellar matter at subnuclear densities

2005-06-20

arxiv.org/abs/nucl-th/0506061v1

Phys.Rev. C72 (2005) 048801

Physics

Nuclear Physics

Nuclear Theory

10 pages, 3 figures

Scientific paper

10.1103/PhysRevC.72.048801

We point out similarity of thermodynamic conditions reached in intermediate energy nuclear collisions and in supernova explosions. We show that a statistical approach, which has been previously applied for nuclear multifragmentation reactions, can be very useful for description of electro-neutral stellar matter. Then properties of hot unstable nuclei extracted from analysis of multifragmentation data can be used for construction of a realistic equation of state of supernova matter.

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