The DOI matches its Crossref record; 15 of the 15 references it cites were found in a registry or an index.
Galaxy formation theory
Open accessAbstract
We review the current theory of how galaxies form within the cosmological framework provided by the cold dark matter paradigm for structure formation. Beginning with the pre-galactic evolution of baryonic material we describe the analytical and numerical understanding of how baryons condense into galaxies, what determines the structure of those galaxies and how internal and external processes (including star formation, merging, active galactic nuclei, etc.) determine their gross properties and evolution. Throughout, we highlight successes and failures of current galaxy formation theory. We include a review of computational implementations of galaxy formation theory and assess their ability to provide reliable modeling of this complex phenomenon. We finish with a discussion of several “hot topics” in contemporary galaxy formation theory and assess future directions for this field.
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Citations
Cites
A Universal Density Profile from Hierarchical Clustering
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1997) · The Astrophysical Journal · doi:10.1086/304888 · Cited by 9,917
The Structure of Cold Dark Matter Halos
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1996) · The Astrophysical Journal · doi:10.1086/177173 · Cited by 8,544 · cited 1×
“…et al. 2004; Merritt et al. 2005; Prada et al. 2006) indicate that density profiles of dark matter halos have an approximately universal form in CDM cosmologies that is better described by the Einasto profile (Einasto 1965) than the Navarro-Frenk-White (NFW) profile (Navarro et al. 1996, 1997).”
BackgroundThe 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
Electromagnetic extraction of energy from Kerr black holes
Blandford, R. D., & Znajek, R. L. (1977) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/179.3.433 · Cited by 5,116
Particle dark matter: evidence, candidates and constraints
Bertone, G., Hooper, D., & Silk, J. (2005) · Physics Reports · doi:10.1016/j.physrep.2004.08.031 · Cited by 4,979
Core condensation in heavy halos: a two-stage theory for galaxy formation and clustering
White, S. D. M., & Rees, M. J. (1978) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/183.3.341 · Cited by 3,919
On the Gravitational Stability of a Disk of Stars
Toomre, A. (1964) · The Astrophysical Journal · doi:10.1086/147861 · Cited by 3,349
McKee, C. F., & Ostriker, J. P. (1977) · The Astrophysical Journal · doi:10.1086/155667 · Cited by 2,082 · cited 2×
“Our discussion below will mostly follow Efstathiou (2000; see also McKee and Ostriker 1977).”
BackgroundInfluentialThe origin of dwarf galaxies, cold dark matter, and biased galaxy formation
Dekel, A., & Silk, J. (1986) · The Astrophysical Journal · doi:10.1086/164050 · Cited by 1,919 · cited 1×
“As early as 1974 (Larson 1974; see also White and Rees 1978; Dekel and Silk 1986) it was realized that star formation could not proceed with 100% efficiency in all dark matter halos.”
BackgroundMaraston, C. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09270.x · Cited by 1,907 · cited 1×
“Several libraries exist which provideL(SSP)ν (t, Z, φ) for several different ages, metallicities and initial mass functions (Bruzual and Charlot 2003; Maraston 2005; Dotter et al. 2007; Conroy et al. 2008; Lee et al. 2009).”
BackgroundDunkley, J., Komatsu, E., Nolta, M. R., Spergel, D. N., Larson, D., Hinshaw, G., Page, L., Bennett, C. L., Gold, B., Jarosik, N., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/180/2/306 · Cited by 1,787
Lintott, C. J., Schawinski, K., Slosar, A., Land, K., Bamford, S., Thomas, D., Raddick, M. J., Nichol, R. C., Szalay, A., Andreescu, D., et al. (2008) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2008.13689.x · Cited by 1,488
Contraction of dark matter galactic halos due to baryonic infall
Blumenthal, G. R., Faber, S. M., Flores, R., & Primack, J. R. (1986) · The Astrophysical Journal · doi:10.1086/163867 · Cited by 1,213 · cited 1×
“The original formulation of this argument for galaxies was given by Blumenthal et al. (1986) and has been used extensively ever since.”
MethodHeating of galactic disks by mergers
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Cosmic ray confinement in fossil cluster bubbles: Cosmic rays in fossil cluster bubbles
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Cited by
Physical Models of Galaxy Formation in a Cosmological Framework
Somerville, R. S., & Davé, R. (2015) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082812-140951 · Cited by 1,442
Dusty star-forming galaxies at high redshift
Casey, C. M., Narayanan, D., & Cooray, A. (2014) · Physics Reports · doi:10.1016/j.physrep.2014.02.009 · Cited by 800
Davé, R., Finlator, K., & Oppenheimer, B. D. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.20148.x · Cited by 512
Bromm, V., & Yoshida, N. (2011) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081710-102608 · Cited by 512
A unified multiwavelength model of galaxy formation
Lacey, C. G., Baugh, C. M., Frenk, C. S., Benson, A. J., Bower, R. G., Cole, S., Gonzalez-Perez, V., Helly, J. C., Lagos, C. D. P., & Mitchell, P. D. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1888 · Cited by 422
Self-citation
Metadata
- Authors
- Benson, A. J.
- Venue
- Physics Reports
- Publisher
- Elsevier BV
- Published
- 2010-10
- Volume
- 495
- Issue
- 2-3
- Pages
- 33-86
- ISSN
- 0370-1573 (ISSN-L)
- OpenAlex
- W1993501365
- Cited by
- 343
- References
- 15
- FWCI
- 14.95
- Type
- journal article
- Language
- en
- Open access
- green
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
