7–12 Jul 2024
Aurum, the ‘Gabriele d’Annunzio’ University and ICRANet
Europe/Rome timezone

Modelling neutron star magnetic fields

12 Jul 2024, 15:30
30m
M6 (Palazzo Micara of the ‘Gabriele d’Annunzio’ University)

M6

Palazzo Micara of the ‘Gabriele d’Annunzio’ University

Viale Pindaro, 42, Pescara
Invited talk in a parallel session Galactic and extragalactic magnetars: recent observations and theoretical progress Galactic and extragalactic magnetars: recent observations and theoretical progress

Speaker

Brynmor Haskell (Nicolaus Copernicus Astronomical Center, PAS)

Description

The magnetic field of a neutron star plays a key role in its evolution and the dynamics of the emission, both electromagnetic and gravitational. Nevertheless the field configuration of these stars is still highly uncertain. In this talk I will review the main issues involved in modelling the magnetic field, and recent advances.

Primary author

Brynmor Haskell (Nicolaus Copernicus Astronomical Center, PAS)

Presentation materials