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Cavitation and bubble collapse in hot asymmetric nuclear matter

V. M. Kolomietz
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Abstract

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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V. M. Kolomietz. 2004-06-19. Cavitation and bubble collapse in hot asymmetric nuclear matter. https://doi.org/10.1103/physrevc.70.044321

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