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Neutron Star Matter

<p> An expression is obtained for the energy per particle
in neutron star matter. The energy per particle is expressed
as a function of, y, the ratio of protons to the total number
of nucleons in the system. Minimizing the energy with respect
to y gives the optimum proton ratio at a given density. Using
an effective nuclear force, the results were extrapolated to
a density of p = 6pNM. The proton ratio is rather sensitive
to the force used, but all forces used indicated a peak in the
proton concentration at p (approximately equal to) 2pNM. The expression for the
energy as a function of y was also used to interpolate the
energy per particle between the nuclear matter and neutron
. gas limits. The form of this interpolation is important in
determining the stability of neutron-rich nuclei. </p> / Thesis / Master of Science (MSc)

Identiferoai:union.ndltd.org:mcmaster.ca/oai:macsphere.mcmaster.ca:11375/17699
Date10 1900
CreatorsEllis, Dale D.
ContributorsSprung, D. W. L., Physics
Source SetsMcMaster University
LanguageEnglish
Detected LanguageEnglish
TypeThesis

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