For differentially rotating, strongly magnetized neutron stars on constant angular-momentum sequences, the normalized moment of inertia remains quasi-universal across equations of state when the Breu-Rezzolla fit is extended with magnetic and differential-rotation coefficients.
With the help ofxnscode utilizing 10 different EoSs, we have obtained equilibrium configurations of NSs
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Structural quasi-universality in highly magnetized differentially rotating neutron stars
For differentially rotating, strongly magnetized neutron stars on constant angular-momentum sequences, the normalized moment of inertia remains quasi-universal across equations of state when the Breu-Rezzolla fit is extended with magnetic and differential-rotation coefficients.