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Title: The MassiveBlack-II simulation: The evolution of haloes and galaxies to z ~ 0

We investigate the properties and clustering of halos, galaxies and blackholes to z = 0 in the high resolution hydrodynamical simulation MassiveBlack-II (MBII). MBII evolves a ΛCDM cosmology in a cubical comoving volume V box = (100Mpc/h)³. It 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 the halos, subhalos and their properties and publicly release our galaxy catalogs to the scientific community. Our analysis of the halo mass function in MBII reveals that baryons have strong effects with changes in the halo abundance of 20–35% below the knee of the mass function (M halo 10 13.2 M h at z = 0) when compared to dark-matter-only simulations. We provide a fitting function for the halo MF out to redshift z = 11 and discuss its limitations.
 [1] ;  [2] ;  [2] ;  [3] ;  [2] ;  [2] ;  [4] ;  [2]
  1. Brookhaven National Lab. (BNL), Upton, NY (United States)
  2. Carnegie Mellon Univ., Pittsburgh, PA (United States)
  3. Univ. of Sussex, Brighton (United Kingdom)
  4. The Hebrew Univ., Jerusalem (Israel)
Publication Date:
Report Number(s):
Journal ID: ISSN 0035-8711; KA2301020
Grant/Contract Number:
Accepted Manuscript
Journal Name:
Monthly Notices of the Royal Astronomical Society
Additional Journal Information:
Journal Volume: 450; Journal Issue: 2; Journal ID: ISSN 0035-8711
Royal Astronomical Society
Research Org:
Brookhaven National Laboratory (BNL), Upton, NY (United States)
Sponsoring Org:
USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
Country of Publication:
United States
79 ASTRONOMY AND ASTROPHYSICS; methods: numerical - cosmology: theory - cosmology: large-scale structure of Universe - galaxies; formation - galaxies: evolution - quasars: general
OSTI Identifier: