activity
20042008
most citedThe Density Probability Distribution in Compressible Isothermal Turbulence: Solenoidal versus Compressive Forcing

514 citations · 758 across the 4 of their papers we have counts for

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astro-ph2008514 cited

The Density Probability Distribution in Compressible Isothermal Turbulence: Solenoidal versus Compressive Forcing

Christoph Federrath, Ralf S. Klessen, Wolfram Schmidt

The probability density function (PDF) of the gas density in turbulent supersonic flows is investigated with high-resolution numerical simulations. In a systematic study, we compar…

astro-ph2006118 cited

A localised subgrid scale model for fluid dynamical simulations in astrophysics II: Application to type Ia supernovae

W. Schmidt, J. C. Niemeyer, W. Hillebrandt +1

The dynamics of the explosive burning process is highly sensitive to the flame speed model in numerical simulations of type Ia supernovae. Based upon the hypothesis that the effect…

astro-ph2006125 cited

A localised subgrid scale model for fluid dynamical simulations in astrophysics I: Theory and numerical tests

W. Schmidt, J. C. Niemeyer, W. Hillebrandt

We present a one-equation subgrid scale model that evolves the turbulence energy corresponding to unresolved velocity fluctuations in large eddy simulations. The model is derived i…

astro-ph2005

Thermonuclear supernova simulations with stochastic ignition

W. Schmidt, J. C. Niemeyer

We apply an ad hoc model for dynamical ignition in three-dimensional numerical simulations of thermonuclear supernovae assuming pure deflagrations. The model makes use of the stati…

astro-ph20041 cited

Simulations of Turbulent Thermonuclear Burning in Type Ia Supernovae

W. Hillebrandt, M. Reinecke, W. Schmidt +3

Type Ia supernovae have recently received considerable attention because it appears that they can be used as "standard candles" to measure cosmic distances out to billions of light…