T Enoto, S Kisaka, S Shibata - Reports on Progress in Physics, 2019 - iopscience.iop.org
Young and rotation-powered neutron stars (NSs) are commonly observed as rapidly- spinning pulsars. They dissipate their rotational energy by emitting pulsar wind with …
D De Grandis, R Turolla, TS Wood, S Zane… - The Astrophysical …, 2020 - iopscience.iop.org
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 …
X Li, Y Levin, AM Beloborodov - The Astrophysical Journal, 2016 - iopscience.iop.org
We explore the interaction between Hall waves and mechanical failures inside a magnetar crust, using detailed one-dimensional models that consider temperature-sensitive plastic …
D Skiathas, KN Gourgouliatos - Monthly Notices of the Royal …, 2024 - academic.oup.com
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 …