Cavitation and bubble collapse in hot asymmetric nuclear matter

Physics – Nuclear Physics – Nuclear Theory

Scientific paper

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Revtex file (10 pages) and 3 figures

Scientific paper

10.1103/PhysRevC.70.044321

The dynamics of embryonic bubbles in overheated, viscous and non-Markovian nuclear matter is studied. It is shown that the memory and the Fermi surface distortions significantly affect the hinderance of bubble collapse and determine a characteristic oscillations of the bubble radius. These oscillations occur due to the additional elastic force induced by the memory integral.

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