Speaker
Brynmor Haskell
(CAMK PAN)
Description
I will discuss the issues related with calculating the magnetic field structure in the interior of neutron stars, and how numerical simulations can be used to asses the stability and evolution of such configurations.
In particular I will focus on instabilities and on the development of turbulence. I will show new results in which the turbulence is resolved, and discuss it's impact on astrophysical observables.
Primary authors
Brynmor Haskell
(CAMK PAN)
RAJ KISHOR JOSHI
(Nicolaus Copernicus Astronomical Center)
William Cook
(Friedrich-Schiller-Universität Jena)
