Solution for the relativistic magnetic field dynamics equation of neutron stars as magnetized, accreting, and rapidly rotating conductors in zero angular momentum observers (ZAMO) frame

Solution for the relativistic magnetic field dynamics equation of neutron stars as magnetized conductors has been formulated by assuming the magnetic field as magnetized, rapidly rotating conductor, and accreting in Zero Angular Momentum Observers (ZAMO) frame. The magnetic field in a neutron star i...

Ausführliche Beschreibung

Bibliographische Detailangaben

Hauptverfasser:	Yasrina, A., Andra, D., Widianingrum, N., Latifah, E., Pramono, N. A.
Format:	Tagungsbericht
Sprache:	eng
Schlagworte:	Angular momentum Conductors Deposition Differential equations Magnetic fields Maxwell's equations Neutron stars Neutrons Observers Relativistic effects Stellar magnetic fields Stellar rotation Tensors Time functions
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!