Formation of hot heavy nuclei in supernova explosions

Physics – Nuclear Physics – Nuclear Theory

Scientific paper

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6 pages with 4 figures

Scientific paper

10.1016/j.physletb.2004.01.064

We point out that during the supernova II type explosion the thermodynamical condition of stellar matter between the protoneutron star and the shock front corresponds to the nuclear liquid-gas phase coexistence region, which can be investigated in nuclear multifragmentation reactions. We have demonstrated, that neutron-rich hot heavy nuclei can be produced in this region. The production of these nuclei may influence dynamics of the explosion and contribute to the synthesis of heavy elements.

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