The MassiveBlack-II Simulation: The Evolution of Halos and Galaxies to z~0

Abstract

(Abridged for arXiv)We investigate the properties of halos, galaxies and blackholes to z=0 in the high resolution hydrodynamical simulation MassiveBlack-II (MBII) which evolves a LCDM cosmology in a comoving volume Vbox=100(Mpc/h)^3. MBII is the highest resolution simulation of this size which includes a self-consistent model for star formation, black hole accretion and associated feedback. We provide a simulation browser web application which enables interactive search and tagging of halos, subhalos and their properties and publicly release our galaxy catalogs. Our analysis of the halo mass function (MF) in MBII reveals that baryons have strong effects, with changes in the halo abundance of 20-35% below the knee of the MF (Mhalo < 10^13.2 Msun/h at z=0) when compared to fits based on dark matter only simulations. We provide a fitting function for the halo MF out to redshift z=11 and discuss how the onset of non-universality in the MF limits the accuracy of our fit. We study the halo occupation distribution and clustering of galaxies, in particular the evolution and scale dependence of stochasticity and bias finding reasonable agreement with observational data. The shape of the cosmic spectral energy distribution predicted by MBII is consistent with observations, but lower in amplitude. The Galaxy Stellar Mass Function (GSMF) function is broadly consistent with observations at z>=2. At z<2, the population of passive low mass (for M*<10^9 Msun) galaxies in MBII makes the GSMF too steep compared to observations whereas at the high mass end (M*>10^11 Msun) galaxies hosting bright AGNs make significant contributions to the GSMF. The quasar bolometric luminosity function is also largely consistent with observations. We note however that more efficient AGN feedback (beyond simple thermal coupling used here) is likely necessary for the largest, rarest objects/clusters at low redshifts.

26 pages, 25 figures. Submitted to MNRAS. High-resolution version and MBII galaxy catalogs can be found at http://mbii.phys.cmu.edu/data/

References in corpus (30)

• The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
• Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
• Properties of galaxies reproduced by a hydrodynamic simulation
• An Observational Determination of the Bolometric Quasar Luminosity Function
• Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
• A unified model for AGN feedback in cosmological simulations of structure formation
• Formation of Supermassive Black Holes by Direct Collapse in Pregalactic Halos
• Cosmological Simulations of Intergalactic Medium Enrichment from Galactic Outflows
• The stellar mass assembly of galaxies from z=0 to z=4. Analysis of a sample selected in the rest-frame near-infrared with Spitzer
• Forming Disk Galaxies in Lambda CDM Simulations
• Direct cosmological simulations of the growth of black holes and galaxies
• A primer on hierarchical galaxy formation: the semi-analytical approach
• Effects of Baryons and Dissipation on the Matter Power Spectrum
• The halo mass function from the dark ages through the present day
• Formation of z ~ 6 quasars from hierarchical galaxy mergers
• The Halo Mass Function: High-Redshift Evolution and Universality
• Quasars at z=6: the survival of the fittest
• A refined sub-grid model for black hole accretion and AGN feedback in large cosmological simulations
• The abundance of (not just) dark matter haloes
• The baryon fraction of LambdaCDM haloes
• The effect of AGN feedback on the halo mass function
• Simulation techniques for cosmological simulations
• The Structure of Halos: Implications for Group and Cluster Cosmology
• The Effect of Gas Physics on the Halo Mass Function
• Strong clustering of underdense regions and the environmental dependence of clustering from Gaussian initial conditions
• Comments on the size of the simulation box in cosmological N-Body simulations
• Supermassive Black Holes and Their Environments
• Median statistics cosmological parameter values
• The Cosmological Parameters (2023)
• Cosmological Perturbation Theory as a Tool for Estimating Box-Scale Effects in N-body Simulations

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