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Galaxy Clustering and Galaxy Bias in a Lambda-CDM Universe
David H. Weinberg, Romeel Dav'e, Neal Katz +1
We investigate galaxy clustering and galaxy-mass correlations in the LCDM cosmological model using a large volume SPH simulation. For the most part, the predicted biases between ga…
An analytical model for the history of cosmic star formation
Lars Hernquist, Volker Springel
We use simple analytic reasoning to identify physical processes that drive the evolution of the cosmic star formation density in cold dark matter universes. Based on our analysis,…
The Nature of the Ionising Background at z=2.5-5
Aaron Sokasian, Tom Abel, Lars E. Hernquist
Using radiative transfer calculations and cosmological simulations of structure formation, we study constraints that can be placed on the nature of the cosmic ultraviolet (UV) back…
Cosmological SPH simulations: A hybrid multi-phase model for star formation
Volker Springel, Lars Hernquist
We present a model for star formation and supernova feedback that describes the multi-phase structure of star forming gas on scales that are typically not resolved in cosmological…
The history of star formation in a LCDM universe
Volker Springel, Lars Hernquist
Employing hydrodynamic simulations of structure formation in a LCDM cosmology, we study the history of cosmic star formation from the "dark ages" at redshift z~20 to the present. I…
Simulating the Sunyaev-Zel'dovich effect(s): including radiative cooling and energy injection by galactic winds
Martin White, Lars Hernquist, Volker Springel
We present results on the thermal and kinetic Sunyaev-Zel'dovich (SZ) effects from a sequence of high resolution hydrodynamic simulations of structure formation, including cooling,…