Relating the Kick Velocities of Young Pulsars with Magnetic Field Growth Timescales Inferred From Braking Indices

A nascent neutron star may be exposed to fallback accretion soon after the proto-neutron star stage. This high accretion episode can submerge the magnetic field deep in the crust. The diffusion of the magnetic field back to the surface will take hundreds to millions of years depending on the amount...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	arXiv.org 2012-12
Hauptverfasser:	Güneydaş, A, Ekşi, K Y
Format:	Artikel
Sprache:	eng
Schlagworte:	Braking Deposition Magnetic fields Neutron stars Neutrons Physics - High Energy Astrophysical Phenomena Pulsars Velocity
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!