Abstract
We have used a self-consistent time dependent Thomas-Fermi model at finite temperature to calculate the dynamical evolution of hot and compressed nuclei. It has been found that nuclei can accomodate more thermal energy than compressional energy before they break.
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References
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Nemeth, J., Barranco, M., Ngô, C. et al. Spherical time dependent Thomas-Fermi calculation of the dynamical evolution of hot and compressed nuclei. Z Physik A 320, 691–692 (1985). https://doi.org/10.1007/BF01411873
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DOI: https://doi.org/10.1007/BF01411873