Magnetic Field Evolution for Keplerian and Sub-Keplerian Flows around Non Rotating Black Hole

The exact two-dimensional non-stationary solution for the evolution of the magnetic field during accretion with nearly spherical symmetry, using Newton's solution and considering both Keplerian and sub-Keplerian flows around the black hole (BH), has been derived using the Schwarzschild metric....

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	arXiv.org 2024-08
Hauptverfasser:	Gharghabi, Malihe Mousapour, Ghanbari, Jamshid, Moghaddas, Mahboobe Moeen
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Companion stars Interstellar matter Magnetic fields Schwarzschild metric Subsonic flow Two dimensional flow
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!