Numerical simulations of oscillating and differentially rotating neutron stars

Context. The remnants of binary neutron star mergers are expected to be massive, rapidly rotating stars whose oscillations produce gravitational waves in the kilohertz band. The degree of differential rotation and the rotation profiles strongly influence their structure, stability, and oscillation s...

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Principais autores:	Jaraba Santiago, Novak Jérôme, Oertel Micaela
Format:	Artigo
Jezik:	Inglês
Izdano:	EDP Sciences 2026-04-01
Serija:	Astronomy & Astrophysics
Teme:	gravitation gravitational waves hydrodynamics methods: numerical stars: neutron stars: oscillations (including pulsations)
Online dostop:	https://www.aanda.org/articles/aa/full_html/2026/04/aa58989-26/aa58989-26.html
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