44 citations · 137 across the 12 of their papers we have counts for
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Cosmological Simulations with Scale-Free Initial Conditions II: Radiative Cooling
J. Michael Owen, David H. Weinberg, Jens V. Villumsen
The growth of structure from scale-free initial conditions is one of the most important tests of cosmological simulation methods, providing a realistically complex problem in which…
Cosmological Simulations with Scale-Free Initial Conditions I: Adiabatic Hydrodynamics
J. Michael Owen, David H. Weinberg, August E. Evrard +2
We analyze hierarchical structure formation based on scale-free initial conditions in an Einstein-de Sitter universe, including a baryonic component. We present three independent,…
Baryons, Dark Matter, and the Jeans Mass in Simulations of Cosmological Structure Formation
J. Michael Owen, Jens V. Villumsen
We investigate the properties of hybrid gravitational/hydrodynamical simulations, examining both the numerics and the general physical properties of gravitationally driven, hierarc…