Clustering and phase transitions in hot, dense stellar matter

Details Clustering and phase transitions in hot, dense stellar matter Clustering and phase transitions in hot, dense stellar matter

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...245l.109b&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 245, May 1, 1981, p. L109-L112.

Physics

Nuclear Physics

6

Astrophysics, Neutron Stars, Nuclei (Nuclear Physics), Phase Transformations, Thomas-Fermi Model, Dense Plasmas, Equations Of State, Nucleons, Supernovae

Scientific paper

The nuclear Thomas-Fermi model is applied to the study of the clustering
of nucleons in hot, dense matter. The several phase transitions which
occur are discussed: (1) from the clustered to the homogeneous phase,
(2) between the Coulomb fluid and the Coulomb crystal and, finally, (3)
the transition from nuclei to nucleon bubbles.

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