Effects Of Star Formation Models On The Cosmic Star Formation History

Mathematics – Logic

Scientific paper

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Scientific paper

We investigate the effects of star formation (SF) models on the cosmic SF history using cosmological smoothed particle hydrodynamics (SPH) simulations based on the cold dark matter (CDM) model. We test two new SF models: 1) the `Pressure' model based on the work by Schaye & Dalla Vecchia (2008), and 2) the `Blitz' model that takes the effect of molecular hydrogen formation into account, based on the work by Blitz & Rosolowsky (2006). Compared to the previous conventional SF model, the Pressure model reduces the SFR in low-density region and shows better agreement with the observations of the Kennicutt law. Our new model also suppresses the early star formation and shift the peak of the cosmic SF history toward low redshift, more consistently with the recent observational estimates of cosmic SFR density. The simulations with the new SF model also predict lower global stellar mass densities at high redshift, larger population of low-mass galaxies and high gas fraction in high-redshift galaxies. Our results suggest that there are still rooms left in the model uncertainties to reconcile the discrepancy that was found between the theory and observations of cosmic SF history and stellar mass density. Nevertheless, our simulations still predict higher stellar mass densities than most of the observational estimates.

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