The Santa Barbara Cluster Comparison Project: A Comparison of Cosmological Hydrodynamics Solutions
Year: 1999
Type: article
Abstract: We have simulated the formation of an X-ray cluster in a cold dark matter universe using 12 different codes. The codes span the range of numerical techniques and implementations currently in use, including smoothed particle hydrodynamics (SPH) and grid methods with fixed, deformable, or multilevel meshes. The goal of this comparison is to assess the reliability of cosmological gasdynamical simulations of clusters in the simplest astrophysically relevant case, that in which the gas is assumed to be nonradiative. We compare images of the cluster at different epochs, global properties such as mass, temperature and X-ray luminosity, and radial profiles of various dynamical and thermodynamical quantities. On the whole, the agreement among the various simulations is gratifying, although a number of discrepancies exist. Agreement is best for properties of the dark matter and worst for the total X-ray luminosity. Even in this case, simulations that adequately resolve the core radius of the gas distribution predict total X-ray luminosities that agree to within a factor of 2. Other quantities are reproduced to much higher accuracy. For example, the temperature and gas mass fraction within the virial radius agree to within about 10%, and the ratio of specific dark matter kinetic to gas thermal energies agree to within about 5%. Various factors, including differences in the internal timing of the simulations, contribute to the spread in calculated cluster properties. Based on the overall consistency of results, we discuss a number of general properties of the cluster we have modeled.
Source: The Astrophysical Journal
DOI: 10.1086/307908
Authors: C. S. Frenk, S. D. M. White, P. Bode, J. R. Bond, G. L. Bryan, R. Cen, H. M. P. Couchman, A. E. Evrard, N. Gnedin, A. Jenkins, A. M. Khokhlov, A. Klypin, J. F. Navarro, M. L. Norman, J. P. Ostriker, J. M. Owen, F. R. Pearce, U.‐L. Pen, M. Steinmetz, P. A. Thomas, J. V. Villumsen, J. W. Wadsley, M. S. Warren, G. Xu, G. Yepes
Institutions: Durham University, Max Planck Institute for Astrophysics, University of Pennsylvania, University of Toronto, Canadian Institute for Theoretical Astrophysics, Massachusetts Institute of Technology, Princeton University, Western University, University of Michigan, University of California, Berkeley, United States Naval Research Laboratory, Naval Research Laboratory Laboratories for Computational Physics & Fluid Dynamics, New Mexico State University, University of Victoria, University of Illinois Urbana-Champaign, National Center for Supercomputing Applications, Lawrence Livermore National Laboratory, The Ohio State University, Center for Astrophysics Harvard & Smithsonian, University of Arizona, University of Sussex, Los Alamos National Laboratory, University of California, Santa Cruz, Universidad Autónoma de Madrid
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
OpenAlex ID: W2162725047