PIC methods in astrophysics: simulations of relativistic jets and kinetic physics in astrophysical systems
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 …
Birdsall, Roger W. Hockney, and John Dawson in the 1950s and, with the advances of …
Precession-induced Variability in AGN Jets and OJ 287
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 …
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 …
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 …
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 …
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+ …
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 …
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 …
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 …
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
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 …
magnetization. The main dissipation mechanism is identified as reconnection of magnetic …