The DOI matches its Crossref record; 116 of the 116 references it cites were found in a registry or an index.
Direct Cosmological Simulations of the Growth of Black Holes and Galaxies
Open accessAbstract
We investigate the coupled formation and evolution of galaxies and their embedded supermassive black holes using state-of-the-art hydrodynamic simulations of cosmological structure formation. For the first time, we self-consistently follow the dark matter dynamics, radiative gas cooling, and star formation, as well as BH growth and associated feedback processes, starting directly from initial conditions appropriate for the ΛCDM cosmology. Our modeling of the black hole physics is based on an approach that we have developed in simulations of isolated galaxy mergers. Here we examine (1) the predicted global history of BH mass assembly, (2) the evolution of the local black hole-host mass correlations, and (3) the conditions that allow rapid growth of the first quasars, and the properties of their hosts and descendants today. We find a total BH mass density in good agreement with observational estimates. The BH accretion rate density peaks at lower redshift and evolves more strongly at high redshift than the star formation rate density, but the ratio of black hole to stellar mass density shows only a moderate evolution at low redshifts. We find strong correlations between BH masses and properties of the stellar systems, agreeing well with the measured local M BH -σ and M BH - M * relationships, but also suggesting (dependent on the mass range) a weak evolution with redshift in the normalization and the slope. Our simulations also produce massive black holes at high redshift, due to extended periods of exponential growth in regions that collapse early and exhibit strong gas inflows. These first supermassive BH systems, however, are not necessarily the most massive ones today, since they are often overtaken in growth by quasars that form later.
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Three‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Implications for Cosmology
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The cosmological simulation code gadget-2
Springel, V. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09655.x · Cited by 6,368
Self-citationThe Global Schmidt Law in Star‐forming Galaxies
Kennicutt, Jr. (1998) · The Astrophysical Journal · doi:10.1086/305588 · Cited by 5,202
Simulations of the formation, evolution and clustering of galaxies and quasars
Springel, V., White, S. D. M., Jenkins, A., Frenk, C. S., Yoshida, N., Gao, L., Navarro, J., Thacker, R., Croton, D., Helly, J., et al. (2005) · Nature · doi:10.1038/nature03597 · Cited by 5,067
Self-citationSmoothed Particle Hydrodynamics
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A Fundamental Relation between Supermassive Black Holes and Their Host Galaxies
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The Demography of Massive Dark Objects in Galaxy Centers
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The cosmological simulation code GADGET-2
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Self-citationCroton, D. J., Springel, V., White, S. D. M., De Lucia, G., Frenk, C. S., Gao, L., Jenkins, A., Kauffmann, G., Navarro, J. F., & Yoshida, N. (2006) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09675.x · Cited by 3,685
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Cited by
Simulating galaxy formation with black hole driven thermal and kinetic feedback
Weinberger, R., Springel, V., Hernquist, L., Pillepich, A., Marinacci, F., Pakmor, R., Nelson, D., Genel, S., Vogelsberger, M., Naiman, J., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2944 · Cited by 1,258
Self-citationTumlinson, J., Peeples, M. S., & Werk, J. K. (2017) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-091916-055240 · Cited by 1,147
The Assembly of the First Massive Black Holes
Inayoshi, K., Visbal, E., & Haiman, Z. (2020) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-120419-014455 · Cited by 665
THE MAJOR AND MINOR GALAXY MERGER RATES AT z < 1.5
Lotz, J. M., Jonsson, P., Cox, T. J., Croton, D., Primack, J. R., Somerville, R. S., & Stewart, K. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/742/2/103 · Cited by 450
Cosmological Simulations of Quasar Fueling to Subparsec Scales Using Lagrangian Hyper-refinement
Anglés-Alcázar, D., Quataert, E., Hopkins, P. F., Somerville, R. S., Hayward, C. C., Faucher-Giguère, C.-A., Bryan, G. L., Kereš, D., Hernquist, L., & Stone, J. M. (2021) · The Astrophysical Journal · doi:10.3847/1538-4357/ac09e8 · Cited by 118
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Metadata
- Authors
- Di Matteo, T., Colberg, J., Springel, V., Hernquist, L., & Sijacki, D.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2008-03-20
- Volume
- 676
- Issue
- 1
- Pages
- 33-53
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2070803987
- Cited by
- 555
- References
- 116
- FWCI
- 28.30
- Type
- journal article
- Language
- en
- Open access
- green
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