collaborators

7 papers

astro-ph.HE2026

Resonant Inverse Compton Scattering and Hard X-ray Emission in Magnetar Magnetospheres

Kun Hu, Nicholas Rackers, Alexander Y. Chen

Magnetars are a subclass of neutron stars with ultra-strong surface magnetic fields. Some magnetars exhibit persistent hard X-ray emission, characterized by power-law tails with ph…

astro-ph.HE2026

Collisionless Accretion of Finite-Angular-Momentum Plasma onto a Spinning Black Hole

John M. Mehlhaff, Alexander Y. Chen, Martin Luepker +1

In low-luminosity active galactic nuclei like M87* and Sgr A*, the accretion disk around the central supermassive black hole is tenuous and collisionless. As a result, the usual id…

astro-ph.HE2025

Global Kinetic Simulations of Monster Shocks and Their Emission

Dominic Bernardi, Yajie Yuan, Alexander Y. Chen

Fast magnetosonic waves are one of the two low-frequency plasma modes that can exist in a neutron star magnetosphere. It was recently realized that these waves may become nonlinear…

astro-ph.HE2025

Stable Collisionless Tori Around Kerr Black Holes

Martin Luepker, Yajie Yuan, Alexander Y. Chen

In low-luminosity active galactic nuclei like M87 and Sgr A, the accretion flow in the vicinity of the black hole is in the collisionless regime, meaning that the col…

astro-ph.HE2025

Alfvén Wave Conversion to Low Frequency Fast Magnetosonic Waves in Magnetar Magnetospheres

Dominic Bernardi, Yajie Yuan, Alexander Y. Chen

Rapid shear motion of magnetar crust can launch Alfvén waves into the magnetosphere. The dissipation of the Alfvén waves has been theorized to power the X-ray bursts characterist…

astro-ph.HE2025

Physics of Pair Producing Gaps in Black Hole Magnetospheres: Two Dimensional General Relativistic Particle-in-cell Simulations

Yajie Yuan, Alexander Y. Chen, Martin Luepker

Black holes can launch powerful jets through the Blandford-Znajek process. This relies on enough plasma in the jet funnel to conduct the necessary current. However, in some low lum…