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Numerical simulations of the cosmic star formation history

Y. Ascasibar·G. Yepes·S. Gottloeber·V. Mueller
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Abstract

The cosmic star formation history in Cold Dark Matter dominated cosmological scenarios is studied by means of hydrodynamical numerical simulations. In particular, we explore a low density model with a Lambda-term and two high density models with different power spectra, all of them being spatially flat. Our simulations employ a fully nonlinear N-body and Eulerian hydrodynamics algorithm with a model for star formation and supernovae feedback that depends on two phenomenological parameters determined in agreement with previous papers. We find a nearly constant star formation rate beyond z=1, and we discuss which facts may determine the decrease in the SFR from z=1 to the present epoch. The Lambda-term cosmology with realistic parameters for star formation and feedback best reproduces the observed star formation history.

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Y. Ascasibar, G. Yepes, S. Gottloeber, V. Mueller. 2002-03-01. Numerical simulations of the cosmic star formation history. https://doi.org/10.1051/0004-6361%3A20020303

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