PIC methods in astrophysics: simulations of relativistic jets and kinetic physics in astrophysical systems

K Nishikawa, I Duţan, C Köhn, Y Mizuno - Living Reviews in …, 2021 - Springer
Abstract The Particle-In-Cell (PIC) method has been developed by Oscar Buneman, Charles
Birdsall, Roger W. Hockney, and John Dawson in the 1950s and, with the advances of …

Precession-induced Variability in AGN Jets and OJ 287

S Britzen, M Zajaček, C Fendt, E Kun… - The Astrophysical …, 2023 - iopscience.iop.org
The combined study of the flaring of active galactic nuclei (AGNs) at radio wavelengths and
parsec-scale jet kinematics with Very Long Baseline Interferometry has led to the view that …

The role of magnetic field geometry in the evolution of neutron star merger accretion discs

IM Christie, A Lalakos, A Tchekhovskoy… - Monthly Notices of …, 2019 - academic.oup.com
Neutron star mergers are unique laboratories of accretion, ejection, and r-process
nucleosynthesis. We used 3D general relativistic magnetohydrodynamic simulations to …

Spontaneous magnetic reconnection: Collisionless reconnection and its potential astrophysical relevance

RA Treumann, W Baumjohann - The Astronomy and Astrophysics Review, 2015 - Springer
The present review concerns the relevance of collisionless reconnection in the astrophysical
context. Emphasis is put on recent developments in theory obtained from collisionless …

Light-curve models of black hole–neutron star mergers: steps towards a multi-messenger parameter estimation

C Barbieri, OS Salafia, A Perego, M Colpi… - Astronomy & …, 2019 - aanda.org
In the new era of gravitational wave (GW) and multi-messenger astrophysics, the detection
of a GW signal from the coalescence of a black hole–neutron star (BHNS) binary remains a …

The MIXR sample: AGN activity versus star formation across the cross-correlation of WISE, 3XMM, and FIRST/NVSS

B Mingo, MG Watson, SR Rosen… - Monthly Notices of …, 2016 - academic.oup.com
We cross-correlate the largest available mid-infrared (Wide-field Infrared Survey Explorer–
WISE), X-ray (3XMM) and radio (Faint Images of the Radio Sky at Twenty centimetres+ …

Electromagnetic counterparts of black hole–neutron star mergers: dependence on the neutron star properties

C Barbieri, OS Salafia, A Perego, M Colpi… - The European Physical …, 2020 - Springer
Detections of gravitational waves (GWs) may soon uncover the signal from the coalescence
of a black hole–neutron star (BHNS) binary, which is expected to be accompanied by an …

Jet launching in resistive GR-MHD black hole–accretion disk systems

Q Qian, C Fendt, C Vourellis - The Astrophysical Journal, 2018 - iopscience.iop.org
We investigate the launching mechanism of relativistic jets from black hole sources, in
particular the strong winds from the surrounding accretion disk. Numerical investigations of …

Magnetically driven jets and winds from weakly magnetized accretion discs

J Jacquemin-Ide, J Ferreira… - Monthly Notices of the …, 2019 - academic.oup.com
Semi-analytical models of disc outflows have successfully described magnetically driven,
self-confined super-Alfvénic jets from near-Keplerian accretion discs. These jet-emitting …

Kink instability: evolution and energy dissipation in relativistic force-free nonrotating jets

O Bromberg, CB Singh, J Davelaar… - The Astrophysical …, 2019 - iopscience.iop.org
We study the evolution of kink instability in a force-free, nonrotating plasma column of high
magnetization. The main dissipation mechanism is identified as reconnection of magnetic …