Maximum mass, moment of inertia and compactness of relativistic stars

A number of recent works have highlighted that it is possible to express the properties of general-relativistic stellar equilibrium configurations in terms of functions that do not depend on the specific equation of state employed to describe matter at nuclear densities. These functions are normally...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	arXiv.org 2016-04
Hauptverfasser:	Breu, Cosima, Rezzolla, Luciano
Format:	Artikel
Sprache:	eng
Schlagworte:	Angular momentum Binary stars Configurations Equations of state Inertia Moments of inertia Nuclear matter Parameterization Physics - General Relativity and Quantum Cosmology Physics - High Energy Astrophysical Phenomena Relativism Relativistic effects
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!