Origin of galactic and extragalactic magnetic fields
LM Widrow - Reviews of Modern Physics, 2002 - APS
A variety of observations suggest that magnetic fields are present in all galaxies and galaxy
clusters. These fields are characterized by a modest strength (10− 7–10− 5 G) and huge …
clusters. These fields are characterized by a modest strength (10− 7–10− 5 G) and huge …
On the origin of cosmic magnetic fields
RM Kulsrud, EG Zweibel - Reports on progress in physics, 2008 - iopscience.iop.org
We review the extensive and controversial literature concerning how the cosmic magnetic
fields pervading nearly all galaxies and clusters of galaxies actually got started. Some …
fields pervading nearly all galaxies and clusters of galaxies actually got started. Some …
A new class of accurate, mesh-free hydrodynamic simulation methods
PF Hopkins - Monthly Notices of the Royal Astronomical Society, 2015 - academic.oup.com
We present two new Lagrangian methods for hydrodynamics, in a systematic comparison
with moving-mesh, smoothed particle hydrodynamics (SPH), and stationary (non-moving) …
with moving-mesh, smoothed particle hydrodynamics (SPH), and stationary (non-moving) …
Enzo: An adaptive mesh refinement code for astrophysics
This paper describes the open-source code Enzo, which uses block-structured adaptive
mesh refinement to provide high spatial and temporal resolution for modeling astrophysical …
mesh refinement to provide high spatial and temporal resolution for modeling astrophysical …
E pur si muove: Galilean-invariant cosmological hydrodynamical simulations on a moving mesh
V Springel - Monthly Notices of the Royal Astronomical Society, 2010 - academic.oup.com
Hydrodynamic cosmological simulations at present usually employ either the Lagrangian
smoothed particle hydrodynamics (SPH) technique or Eulerian hydrodynamics on a …
smoothed particle hydrodynamics (SPH) technique or Eulerian hydrodynamics on a …
Cosmological hydrodynamics with adaptive mesh refinement-a new high resolution code called ramses
R Teyssier - Astronomy & Astrophysics, 2002 - aanda.org
A new N-body and hydrodynamical code, called RAMSES, is presented. It has been
designed to study structure formation in the universe with high spatial resolution. The code is …
designed to study structure formation in the universe with high spatial resolution. The code is …
Statistical properties of x-ray clusters: Analytic and numerical comparisons
We compare the results of Eulerian hydrodynamic simulations of cluster formation against
virial scaling relations between four bulk quantities: the cluster mass, the dark matter velocity …
virial scaling relations between four bulk quantities: the cluster mass, the dark matter velocity …
Baryons in the warm-hot intergalactic medium
ABSTRACT Approximately 30%–40% of all baryons in the present-day universe reside in a
warm-hot intergalactic medium (WHIM), with temperatures in the range 10 5< T< 10 7 K. This …
warm-hot intergalactic medium (WHIM), with temperatures in the range 10 5< T< 10 7 K. This …
A primer on hierarchical galaxy formation: the semi-analytical approach
CM Baugh - Reports on Progress in Physics, 2006 - iopscience.iop.org
Recent observational and theoretical breakthroughs make this an exciting time to be
working towards understanding the physics of galaxy formation. The goal of this review is to …
working towards understanding the physics of galaxy formation. The goal of this review is to …
FARGO3D: a new GPU-oriented MHD code
P Benítez-Llambay, FS Masset - The Astrophysical Journal …, 2016 - iopscience.iop.org
We present the FARGO3D code, recently publicly released. It is a magnetohydrodynamics
code developed with special emphasis on the physics of protoplanetary disks and planet …
code developed with special emphasis on the physics of protoplanetary disks and planet …