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19962002
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astro-ph2002

Structure Shocks as a Source of Cosmic Rays in Clusters

T. W. Jones, Francesco Miniati, Dongsu Ryu +2

Shocks are a ubiquitous consequence of cosmic structure formation, and they play an essential role in heating galaxy cluster media. Virtually all of the gas in clusters has been pr…

astro-ph2000

3-D MHD Numerical Simulations of Cloud-Wind Interactions

G. Gregori, Francesco Miniati, Dongsu Ryu +1

We present results from three-dimensional (3-D) numerical simulations investigating the magnetohydrodynamics of cloud-wind interactions. The initial cloud is spherical while the ma…

astro-ph2000

Acceleration of CR at Large Scale Shocks and Their Cosmological Role for Structure Formation in the Universe

Francesco Miniati, Dongsu Ryu, T. W. Jones +1

We investigate the dynamical importance of a newly recognized possible source of significant feedback generated during structure formation; namely cosmic ray (CR) pressure. We pres…

astro-ph1999

Three-Dimensional Simulations of the Parker Instability in a Uniformly-rotating Disk

Jongsoo Kim, Dongsu Ryu, T. W. Jones

We investigate the nonlinear effects of uniform rotation on the Parker instability in an exponentially-stratified disk through high-resolution simulations. During the linear stage,…

astro-ph1999

Cosmic Rays and Their Radiative Processes in Numerical Cosmology

Dongsu Ryu, Francesco Miniati, Tom W. Jones +1

A cosmological hydrodynamic code is described, which includes a routine to compute cosmic ray acceleration and transport in a simplified way. The routine was designed to follow exp…

astro-ph1999

The First Magnetic Fields

George Davies, Lawrence M. Widrow

We demonstrate that the Biermann battery mechanism for the creation of large scale magnetic fields can arise in a simple model protogalaxy. Analytic calculations and numerical simu…