activity
20092024
most citedMagnetic fields in axisymmetric neutron stars

169 citations · 1.2k across the 28 of their papers we have counts for

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16 papers · 1 filter

astro-ph.HE2024

The Meissner effect in neutron stars

S. K. Lander

We present the first model aimed at understanding how the Meissner effect in a young neutron star affects its macroscopic magnetic field. In this model, field expulsion occurs on a…

astro-ph.HE2024★ 3 cited

Signatures of magnetic flux expulsion from neutron star cores

S. K. Lander, K. N. Gourgouliatos, Z. Wadiasingh +1

Shortly after a neutron star is born, the protons in its core begin to form a superconductor. In terrestrial materials, the hallmark of superconductivity is an associated expulsion…

astro-ph.HE2023

Twisted magnetar magnetospheres

D. Ntotsikas, K. N. Gourgouliatos, I. Contopoulos +1

Magnetar magnetospheres are strongly twisted, and are able to power sudden energetic events through the rapid release of stored electromagnetic energy. In this paper, we investigat…

astro-ph.HE2022★ 25 cited

The game of life on a magnetar crust: from -ray flares to FRBs

S. K. Lander

This paper presents a model to unify the diverse range of magnetar activity, through the building and release of elastic stress from the crust. A cellular automaton drives both loc…

astro-ph.HE2022★ 28 cited

Pulse Peak Migration during the Outburst Decay of the Magnetar SGR 1830-0645: Crustal Motion and Magnetospheric Untwisting

G. Younes, S. K. Lander, M. G. Baring +12

Magnetars, isolated neutron stars with magnetic field strengths typically ~G, exhibit distinctive months-long outburst epochs during which strong evolution of soft…

astro-ph.HE2021★ 36 cited

Axisymmetric magneto-plastic evolution of neutron-star crusts

Konstantinos N. Gourgouliatos, Samuel K. Lander

Magnetic field evolution in neutron-star crusts is driven by the Hall effect and Ohmic dissipation, for as long as the crust is sufficiently strong to absorb Maxwell stresses exert…