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.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.HE 1years
2026 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
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.