Composition and equation of state of cold catalyzed matter below neutron drip

Details Composition and equation of state of cold catalyzed matter below neutron drip Composition and equation of state of cold catalyzed matter below neutron drip

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...222..353h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 222, no. 1-2, Sept. 1989, p. 353-357.

Astronomy and Astrophysics

Astrophysics

48

Equations Of State, Hartree Approximation, Neutron Stars, Nucleon-Nucleon Interactions, Stellar Interiors, Stellar Structure, Interstellar Matter, Pulsars, Stellar Temperature

Scientific paper

The composition and equation of state of cold catalyzed matter below neutron drip is calculated. The binding energies of nuclei are calculated using the Hartree-Fock-Bogolyubov scheme with an effective nucleon-nucleon interaction. The effect of neutron shells in very neutron-rich nuclei turns out to be much weaker than that obtained using semiempirical mass formulas.

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