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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 1996 · astro-phShow all

6 papers · 2 filters

astro-ph1996★ 1 cited

Numerical Simulations Of Advective Flows Around Black Holes

Sandip K. Chakrabarti, D. Ryu, D. Molteni +3

We present fully time-dependent solutions of accretion processes on black holes and compare them with analytical solutions. We use Smoothed Particle Hydrodynamics and Total Variati…

astro-ph1996★ 18 cited

Accreting Matter around Clusters of Galaxies: One-Dimensional Considerations

Dongsu Ryu, Hyesung Kang

During the formation of the large scale structure of the Universe, matter accretes onto high density peaks. Accreting collisionless dark matter (DM) forms caustics around them, whi…

astro-ph1996★ 456 cited

The Protogalactic Origin for Cosmic Magnetic Fields

Russell M. Kulsrud, Renyue Cen, Jeremiah P. Ostriker +1

It is demonstrated that strong magnetic fields are produced from a zero initial magnetic field during the pregalactic era, when galaxies are first forming. Their development procee…

astro-ph1996★ 131 cited

Zero Energy Rotating Accretion Flows near a Black Hole

Dongsu Ryu, Sandip K. Chakrabarti, Diego Molteni

We characterize the nature of thin, axisymmetric, inviscid, accretion flows of cold adiabatic gas with zero specific energy in the vicinity of a black hole by the specific angular…

astro-ph1996★ 104 cited

The Magnetohydrodynamics of Supersonic Gas Clouds: MHD Cosmic Bullets and Wind-Swept Clumps

T. W. Jones, Dongsu Ryu, I. L. Tregillis

We report an extensive set of two-dimensional MHD simulations exploring the role and evolution of magnetic fields in the dynamics of supersonic plasma clumps. We examine the influe…

astro-ph1996★ 106 cited

Numerical Simulations of Standing Shocks in Accretion Flows around Black Holes: A Comparative Study

Diego Molteni, Dongsu Ryu, Sandip K. Chakrabarti

We compare the results of numerical simulations of thin and quasi-spherical (thick) accretion flows with existing analytical solutions. We use a Lagrangian code based on the Smooth…