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Achieving Extreme Resolution in Numerical Cosmology Using Adaptive Mesh Refinement: Resolving Primordial Star Formation
Greg L. Bryan, Tom Abel, Michael L. Norman
As an entry for the 2001 Gordon Bell Award in the "special" category, we describe our 3-d, hybrid, adaptive mesh refinement (AMR) code, Enzo, designed for high-resolution, multiphy…
Thermal Instability-Induced Interstellar Turbulence
Alexei G. Kritsuk, Michael L. Norman
We study the dynamics of phase transitions in the interstellar medium by means of three-dimensional hydrodynamic numerical simulations. We use a realistic cooling function and gene…
Cosmological Hydrogen Reionization with Three Dimensional Radiative Transfer
Alexei O. Razoumov, Michael L. Norman, Tom Abel +1
We present new calculations of the inhomogeneous process of cosmological reionization by carefully following the radiative transfer in pre-computed hydrodynamical simulations of ga…
Magnetic Field Diagnostics Based on Far-Infrared Polarimetry: Tests Using Numerical Simulations
F. Heitsch, E. G. Zweibel, M. -M. Mac Low +2
The dynamical state of star-forming molecular clouds cannot be understood without determining the structure and strength of their magnetic fields. Measurements of polarized far-inf…