Magnetic field evolution in neutron stars: one-dimensional multi-fluid model

2008/01/31 by J. Hoyos, A. Reisenegger, J. A. Valdivia · 56 citations
Physics and Astronomy · #Astrophysical Phenomena and Observations #Dust and Plasma Wave Phenomena #Field (mathematics) #Magnetic field #Neutron #Neutron star #Pulsars and Gravitational Waves Research #Series (stratigraphy) #Stellar evolution #Stellar magnetic field #astro-ph

paper · pdf · doi:10.1051/0004-6361:200809466

published in Astronomy and Astrophysics 487(3), 789-803 (EDP Sciences) · Paper Accepted in Astronomy & Astrophysics: 24 April 2008, Paper Reference Number: AA/2008/09466. Paper contains 8 Figures. In this version the section: Summary and Conclusions has been expanded

openalex publication_date 2008/06/24 · arxiv created 2008/07/31 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. This paper is the first in a series that aims to understand the long-term evolution of neutron star magnetic fields.

Citations

• Magnetars: Time Evolution, Superfluid Properties, and the Mechanism of Magnetic Field Decay
• A fossil origin for the magnetic field in A stars and white dwarfs
• On non-axisymmetric magnetic equilibria in stars
• Magnetic Field Evolution in Neutron Star Crusts Due to the Hall Effect and Ohmic Decay
• The occurrence of the Hall instability in crusts of isolated neutron stars
• Magnetic fields in neutron stars: A theoretical perspective
• Non–linear magnetic field decay in neutron stars