Using gravitational-wave data to constrain dynamical tides in neutron star binaries

We discuss the role of dynamical tidal effects for inspiraling neutron star binaries, focusing on features that may be considered “unmodeled” in gravitational-wave searches. In order to cover the range of possibilities, we consider (i) individual oscillation modes becoming resonant with the tide, (i...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Physical review. D 2018-01, Vol.97 (2), Article 023016
Hauptverfasser:	Andersson, Nils, Ho, Wynn C. G.
Format:	Artikel
Sprache:	eng
Schlagworte:	Binary stars Energy dissipation Gravitation Gravitational waves Neutron stars Neutrons Oscillation modes Stability Tidal effects
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!