The MassiveBlack-II simulation: The evolution of haloes and galaxies to z ~ 0
Abstract
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 Vbox = (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 (Mhalo 1013.2 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.
- Authors:
-
- Brookhaven National Lab. (BNL), Upton, NY (United States)
- Carnegie Mellon Univ., Pittsburgh, PA (United States)
- Univ. of Sussex, Brighton (United Kingdom)
- The Hebrew Univ., Jerusalem (Israel)
- Publication Date:
- Research Org.:
- Brookhaven National Laboratory (BNL), Upton, NY (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1214100
- Report Number(s):
- BNL-108322-2015-JA
Journal ID: ISSN 0035-8711; KA2301020
- Grant/Contract Number:
- SC00112704
- Resource Type:
- 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
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; methods: numerical - cosmology: theory - cosmology: large-scale structure of Universe - galaxies; formation - galaxies: evolution - quasars: general
Citation Formats
Khandai, Nishikanta, Di Matteo, Tiziana, Croft, Rupert, Wilkins, Stephen, Feng, Yu, Tucker, Evan, DeGraf, Colin, and Liu, Mao -Sheng. The MassiveBlack-II simulation: The evolution of haloes and galaxies to z ~ 0. United States: N. p., 2015.
Web. doi:10.1093/mnras/stv627.
Khandai, Nishikanta, Di Matteo, Tiziana, Croft, Rupert, Wilkins, Stephen, Feng, Yu, Tucker, Evan, DeGraf, Colin, & Liu, Mao -Sheng. The MassiveBlack-II simulation: The evolution of haloes and galaxies to z ~ 0. United States. https://doi.org/10.1093/mnras/stv627
Khandai, Nishikanta, Di Matteo, Tiziana, Croft, Rupert, Wilkins, Stephen, Feng, Yu, Tucker, Evan, DeGraf, Colin, and Liu, Mao -Sheng. Fri .
"The MassiveBlack-II simulation: The evolution of haloes and galaxies to z ~ 0". United States. https://doi.org/10.1093/mnras/stv627. https://www.osti.gov/servlets/purl/1214100.
@article{osti_1214100,
title = {The MassiveBlack-II simulation: The evolution of haloes and galaxies to z ~ 0},
author = {Khandai, Nishikanta and Di Matteo, Tiziana and Croft, Rupert and Wilkins, Stephen and Feng, Yu and Tucker, Evan and DeGraf, Colin and Liu, Mao -Sheng},
abstractNote = {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 Vbox = (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 (Mhalo 1013.2 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.},
doi = {10.1093/mnras/stv627},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 2,
volume = 450,
place = {United States},
year = {Fri Apr 24 00:00:00 EDT 2015},
month = {Fri Apr 24 00:00:00 EDT 2015}
}
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