Effect of Compressibility on Nuclear Matter in a Neutron Star Crust

Details Effect of Compressibility on Nuclear Matter in a Neutron Star Crust Effect of Compressibility on Nuclear Matter in a Neutron Star Crust

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...283..867d&link_type=abstract

Astronomy and Astrophysics, Vol. 283, NO. 3/MAR(III), P. 867, 1994

Astronomy and Astrophysics

Astrophysics

Dense Matter - Equation Of State - Stars: Neutron

Scientific paper

The role of bulk compressibility in evaluating the surface energy term
in nuclear matter at the neutron star crust is studied. The distribution
of proton fraction in nuclei is found to decrease as the density
increases. The maximum Z for nuclei on the neutron star crust are found
to be (20, 25) and (29, 36) for the models considered in this paper.

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