activity
20032026
most citedResonant Cyclotron Scattering in Three Dimensions and the Quiescent Non-thermal X-ray Emission of Magnetars

123 citations · 277 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2026

Global Magnetohydrodynamic Simulations of Monster Shocks in Neutron Star Magnetospheres

Michael P. Grehan, Bart Ripperda, Andrei M. Beloborodov +2

Waves launched from the neutron star surface or inner magnetosphere propagate through the magnetosphere as small perturbations, but can grow relative to the background magnetic fie…

astro-ph.HE2025

Magnetized Accretion onto Neutron Stars: from Photon-trapped to Neutrino-cooled Flows

Luciano Combi, Christopher Thompson, Daniel M. Siegel +2

When a neutron star (NS) intercepts gas from a non-degenerate star, e.g., in a tidal disruption event, a common-envelope phase, or the collapsing core of a massive star, photons be…

astro-ph2008★ 71 cited

Stability of a Spherical Accretion Shock with Nuclear Dissociation

Rodrigo Fernández, Christopher Thompson

We examine the stability of a standing shock wave within a spherical accretion flow onto a gravitating star, in the context of core-collapse supernova explosions. Our focus is on t…

astro-ph2006

Efficient approximations of neutrino physics for three-dimensional simulations of stellar core collapse

M. Liebendoerfer, U. -L. Pen, C. Thompson

Neutrino transport in spherically symmetric models of stellar core collapse and bounce has achieved a technically complete level, rewarded by the agreement among independent groups…

astro-ph2006★ 123 cited

Resonant Cyclotron Scattering in Three Dimensions and the Quiescent Non-thermal X-ray Emission of Magnetars

Rodrigo Fernandez, Christopher Thompson

Although the surface of a magnetar is a source of bright thermal X-rays, its spectrum contains substantial non-thermal components. The X-ray emission is pulsed, with pulsed fractio…

astro-ph2005★ 83 cited

Magnetospheric Eclipses in the Binary Pulsar J0737-3039

Maxim Lyutikov, Christopher Thompson

(Abridged) In the binary radio pulsar system J0737-3039, the faster pulsar A is eclipsed once per orbit. We construct a simple geometric model which successfully reproduces the ecl…