Supermassive black hole spin-flip during the inspiral

During post-Newtonian evolution of a compact binary, a mass ratio different from 1 provides a second small parameter, which can lead to unexpected results. We present a statistics of supermassive black hole candidates, which enables us first to derive their mass distribution, then to establish a log...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	arXiv.org 2010-07
Hauptverfasser:	Gergely, László Á, Biermann, Peter L, Caramete, Laurenţiu I
Format:	Artikel
Sprache:	eng
Schlagworte:	Angular momentum Mass distribution Mass ratios Physics - Cosmology and Nongalactic Astrophysics Physics - General Relativity and Quantum Cosmology Radio galaxies Supermassive black holes
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!