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oai:digital.library.adelaide.edu.au:2440/1225852026-06-12T08:09:54Zcom_2440_14759col_2440_14760

Thomas, Anthony Leinweber, Derek Husain, Wasif School of Physical Sciences : Physics 2019 http://hdl.handle.net/2440/122585 In this thesis a very comprehensive model of rotating neutron stars has been constructed, which is based on the Quark-Meson Coupling model (QMC model), using the method developed by Hartle for slowly rotating compact stars. To determine tidal Love number method suggested by ’Hinderer’ is adopted. In this thesis, neutron star properties are calculated at the rotation frequency of 500 Hz and compared for three EoSs which are based on pure nuclear matter, full baryon octet (both are constructed by taking nuclear structure into consideration) and finally strange quark matter (which is based on the MIT bag model) at the core in β equilibrium. Various universalities have been predicted among the neutron star properties such as dimensionless quadrupole moment vs compactness, dimensionless moment of inertia vs M/R, dimensionless moment of inertia vs dimensionless quadrupole moment and dimensionless moment of inertia vs dimensionless tidal deformability. The significance of the low energy density region and crust is also shown. Thesis (MPhil) -- University of Adelaide, School of Physical Sciences, 2019 en Neutron stars strange stars QMC model universalities Equation of state of rotating neutron stars Thesis This electronic version is made publicly available by the University of Adelaide in accordance with its open access policy for student theses. Copyright in this thesis remains with the author. This thesis may incorporate third party material which has been used by the author pursuant to Fair Dealing exceptions. If you are the owner of any included third party copyright material you wish to be removed from this electronic version, please complete the take down form located at: http://www.adelaide.edu.au/legalsopen.access