Physics
Scientific paper
Oct 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....90...70h&link_type=abstract
Astronomy and Astrophysics, vol. 90, no. 1-2, Oct. 1980, p. 70-72. Research supported by the U.S.-Maria Sklodowska-Curie Fund.
Physics
Compressibility, Fermi Liquids, Matter (Physics), Neutron Stars, Stellar Structure, Elementary Excitations, Nucleon-Nucleon Interactions, Pressure Effects
Scientific paper
The properties of cold catalyzed matter (CCM) of density near and above the density characteristic of the central region of heavy atomic nuclei are of fundamental importance for the physics of neutron stars. In this paper the compression modulus of CCM (an electrically neutral, spatially homogeneous mixture of electrons, neutrons, and protons at a temperature of 0 K) is studied for nucleon number density in the range 0.15-0.4 per cu fm. To a very good approximation the compression modulus is given by the nucleon contribution calculated at a fixed composition of the matter.
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