Joule heating in high magnetic field pulsars

2008/03/19 by V. Urpin, D. Konenkov · 1 citation
Earth and Planetary Sciences · Mathematics · Physics and Astronomy · #Astrophysics #Field (mathematics) #High-pressure geophysics and materials #Joule (programming language) #Joule heating #Magnetic field #Mathematics #Neutron star #Physics #Pulsar #Pulsars and Gravitational Waves Research #Quantum, superfluid, helium dynamics #Stars #Thermodynamics #astro-ph

paper · pdf · doi:10.1051/0004-6361:20078553

8 pages, 5 figures; accepted by Astronomy and Astrophysics

openalex publication_date 2008/03/19 · arxiv created 2008/04/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims. We study the efficiency of Joule heating in the crustal layers of young neutron stars.

Citations

• Population synthesis of pulsars: Magnetic field effects
• Chandra X-Ray Detection of the High Magnetic Field Radio Pulsar PSR J1718-3718
• Evolution of Crustal Magnetic Fields in Isolated Neutron Stars: Combined Effects of Cooling and Curvature of Spacetime
• The magnetic structure of neutron stars and their surface-to-core temperature relation
• Spot-like structures of neutron star surface magnetic fields
• Magnetic Field Evolution in Neutron Star Crusts Due to the Hall Effect and Ohmic Decay
• Non–linear magnetic field decay in neutron stars

Cited by

• The neutron star in Cassiopeia A: equation of state, superfluidity, and Joule heating