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19942023
most citedThe Protogalactic Origin for Cosmic Magnetic Fields

456 citations · 8.7k across the 154 of their papers we have counts for

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Showing 2011 · astro-ph.COShow all

7 papers · 2 filters

astro-ph.CO2011★ 151 cited

Magnetic fields in the Large-Scale Structure of the Universe

Dongsu Ryu, Dominik R. G. Schleicher, Rudolf A. Treumann +2

Magnetic fields appear to be ubiquitous in astrophysical environments. Their existence in the intracluster medium is established through observations of synchrotron emission and Fa…

astro-ph.CO2011★ 207 cited

The First Magnetic Fields

Lawrence M. Widrow, Dongsu Ryu, Dominik Schleicher +3

We review current ideas on the origin of galactic and extragalactic magnetic fields. We begin by summarizing observations of magnetic fields at cosmological redshifts and on cosmol…

astro-ph.CO2011★ 2 cited

MHD Turbulence Simulation in a Cosmic Structure Context

T. W. Jones, D. H. Porter, D. Ryu +1

The gaseous media of galaxy clusters and cosmic filaments, which constitute most of the baryonic matter in the universe, is highly dynamic. It is also probably turbulent, although…

astro-ph.CO2011★ 69 cited

Faraday Rotation Measure due to the Intergalactic Magnetic Field II: the Cosmological Contribution

Takuya Akahori, Dongsu Ryu

We investigate the Faraday rotation measure (RM) due to the intergalactic magnetic field (IGMF) through the cosmic web up to cosmological distances, using a model IGMF based on tur…

astro-ph.CO2011★ 102 cited

A Comparison of Cosmological Codes: Properties of Thermal Gas and Shock Waves in Large Scale Structures

F. Vazza, K. Dolag, D. Ryu +4

[...] We present results for the statistics of thermal gas and the shock wave properties for a large volume simulated with three different cosmological numerical codes: the Euleria…

astro-ph.CO2011★ 119 cited

Re-acceleration of Nonthermal Particles at Weak Cosmological Shock Waves

Hyesung Kang, Dongsu Ryu

We examine diffusive shock acceleration (DSA) of the pre-exisiting as well as freshly injected populations of nonthermal, cosmic-ray (CR) particles at weak cosmological shocks. Ass…

astro-ph.CO2011★ 1 cited

Cluster Turbulence: Simulation Insights

T. W. Jones, David H. Porter, Dongsu Ryu +1

Cluster media are dynamical, not static; observational evidence suggests they are turbulent. High-resolution simulations of the intracluster media (ICMs) and of idealized, similar…