Structure of Matter below Nuclear Saturation Density

Details Structure of Matter below Nuclear Saturation Density Structure of Matter below Nuclear Saturation Density

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983phrvl..50.2066r&link_type=abstract

Physical Review Letters, Volume 50, Issue 26, June 27, 1983, pp.2066-2069

Physics

219

Nuclear Matter, Phase Transitions: General Studies, Late Stages Of Stellar Evolution

Scientific paper

It is found that just below nuclear saturation density more stable forms of dense matter exist than the near-spherical nuclei or bubbles customarily assumed. Because of the large effect of the Coulomb lattice energy, cylindrical and planar geometries can occur, both as nuclei and as bubbles. It is suggested that in order to approximate more complicated kinds of short-range order, the dimensionality should be regarded as a continuous variable ranging from d=3 (spheres) to d=1 (planes). The dependence of d on density is illustrated, and its dependence on nuclear models discussed.

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