Equation of state of hot dense matter

Details Equation of state of hot dense matter Equation of state of hot dense matter

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...183l...3l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 183, no. 1, Sept. 1987, p. L3-L6.

Statistics

Computation

43

Computational Astrophysics, Condensed Matter Physics, Equations Of State, Gravitational Collapse, Supernovae, Algorithms, Enthalpy, Stellar Cores

Scientific paper

With the Thomas-Fermi method, the authors determine the equation of state of hot dense matter at nuclear subsaturation densities. They investigate several geometries with nucleons organized in crystals structures of nuclei, rods, slabs, tubes and bubbles. They calculate the adiabatic index relevant for the first stage of the collapse of medium mass stars.

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