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From the 2 of 35 linked papers with an AI index.

activity
20242026
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35 papers

astro-ph.HE2026

Relativistic blob signatures in the M87 jet at sub-parsec scales

Donaldo Mora, Alejandro Cruz-Osorio, Erika Benítez +1

In this work, we present results from general-relativistic radiative-transfer calculations of black hole accretion and jet launching to reproduce the observed properties of the M\,…

astro-ph.HE2026

Effects of Ambient Medium Profiles on the Evolution of Relativistic Magnetized Jets

Xufan Hu, Yosuke Mizuno

Relativistic radio-galaxy jets are conventionally divided into two morphological classes: FR~I and FR~II. Among them, FR~I jets have relatively low radio luminosities and edge-dark…

astro-ph.HE2026

Inverse Transfer in Non-helical 2D Collisionless Magnetic Turbulence: Island-Merger Picture with Kinetic Effects

Yangyang Cai, Hongzhe Zhou, Yosuke Mizuno

The paper uses particle‑in‑cell simulations to study inverse transfer of magnetic energy in non‑helical, 2‑D collisionless plasma turbulence, finding that while a conserved quantit…

astro-ph.HE2026

Probing radiation micro-physics in M 87 I. Total intensity and broad-band spectra

Christian M. Fromm, Yosuke Mizuno, Ziri Younsi +6

The paper presents 3D general relativistic magnetohydrodynamic simulations of accretion onto a Kerr black hole in M87 and predicts how future high‑resolution VLBI observations can…

astro-ph.HE2026

Impacts of radiative cooling on the images of a black hole shadow and extended jets in two-temperature GRMHD simulations

Mingyuan Zhang, Yosuke Mizuno, Indu K. Dihingia +4

The recent 230 GHz observations from the Event Horizon Telescope collaboration have successfully imaged the supermassive black hole shadow of the M87 galaxy. However, the relativel…

astro-ph.HE2026

Polarization Architecture of Steady GRMHD Jets from the Horizon to Infinity

Zhenyu Zhang, Yehui Hou, Yu Song +2

We develop a semi-analytic framework for stationary, axisymmetric GRMHD jets that efficiently generates resolved polarized images from the near-horizon region out to $\sim 10^5\,r_…