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Hydrodynamic Simulations of the Growth of Cosmological Structure: Summary and Comparisons among Scenarios
1996
Astrophysical Journal
We compute, including a current state-of-the-art treatment of hydrodynamical processes, heating and cooling, a variety of cosmological models into the extreme nonlinear phase to enable comparisons with observations. First, we note the common, model independent results. All have a mean (z=0) temperature of 10^4.5-10^5.5, set essentially by photoheating processes. Most gas is in one of two components: either at the photoheating floor 10^4.5 and primarily in low density regions or else shock
doi:10.1086/177297
fatcat:ndgekmiunvdu5fe4rm35sbxmce