On the accuracy of the IWM-CFC approximation in differentially rotating relativistic stars

DOI10.1007/S10714-014-1800-5zbMath1305.83030arXiv1406.7375OpenAlexW3099396464WikidataQ63410490 ScholiaQ63410490MaRDI QIDQ481736

Nikolaos Stergioulas, Panagiotis Iosif

Publication date: 12 December 2014

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1406.7375

zbMATH Keywords

neutron starsdifferential rotationconformal flatnessnumerical relativity

Mathematics Subject Classification ID

Applications of differential geometry to physics (53Z05) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15) Computational methods for problems pertaining to relativity and gravitational theory (83-08)

Cites Work

• Unnamed Item
• Unnamed Item
• Unnamed Item
• Rapidly rotating general relativistic stars - II. Differentially rotating polytropes
• WAVELESS APPROXIMATION THEORIES OF GRAVITY
• A new general relativistic magnetohydrodynamics code for dynamical spacetimes
• Rapidly rotating general relativistic stars - I. Numerical method and its application to uniformly rotating polytropes
• The Cotton tensor in Riemannian spacetimes
• Rotating collapse of stellar iron cores in general relativity

This page was built for publication: On the accuracy of the IWM-CFC approximation in differentially rotating relativistic stars