Neutron stars are natural physical laboratories allowing us to study a plethora of
phenomena in extreme conditions. In particular, these compact objects can have very strong …

Young and rotation-powered neutron stars (NSs) are commonly observed as rapidly-
spinning pulsars. They dissipate their rotational energy by emitting pulsar wind with …

Neutron stars harbor extremely strong magnetic fields within their solid outer crust. The
topology of this field strongly influences the surface temperature distribution and, hence, the …

Current models of magnetars require extremely strong magnetic fields to explain their
observed quiescent and bursting emission, implying that the field strength within the star's …

We study dynamics of relativistic coronal mass ejections (CMEs), from launching by
shearing of foot-points (either slowly–the 'Solar flare'paradigm, or suddenly–the 'star …

We present the first fully self-consistent three dimensional model of a neutron star's magnetic
field, generated by electric currents in the star's crust via the Hall effect. We find that the …

We explore the interaction between Hall waves and mechanical failures inside a magnetar
crust, using detailed one-dimensional models that consider temperature-sensitive plastic …

Neutron star magnetic field evolution is mediated through the Hall effect and Ohmic
dissipation in the crust while ambipolar diffusion is taking place in the core. These effects …

We explore magnetic field configurations that lead to the formation of magnetic spots on the
surface of neutron stars and the displacement of the magnetic dipole axis. We find that a …

Neutron stars host the strongest magnetic fields that we know of in the Universe. Their
magnetic fields are the main means of generating their radiation, either magnetospheric or …