The DOI matches its Crossref record; 5 of the 5 references it cites were found in a registry or an index.
Halo models of large scale structure
Open accessAbstract
Abstract We review the formalism and applications of the halo-based description of non-linear gravitational clustering. In this approach, all mass is associated with virialized dark matter halos; models of the number and spatial distribution of the halos, and the distribution of dark matter within each halo, are used to provide estimates of how the statistical properties of large scale density and velocity fields evolve as a result of non-linear gravitational clustering. We first describe the model, and demonstrate its accuracy by comparing its predictions with exact results from numerical simulations of non-linear gravitational clustering. We then present several astrophysical applications of the halo model: these include models of the spatial distribution of galaxies, the non-linear velocity, momentum and pressure fields, descriptions of weak gravitational lensing, and estimates of secondary contributions to temperature fluctuations in the cosmic microwave background.
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Cites
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
The statistics of peaks of Gaussian random fields
Bardeen, J. M., Bond, J. R., Kaiser, N., & Szalay, A. S. (1986) · The Astrophysical Journal · doi:10.1086/164143 · Cited by 3,270
Gauge-invariant cosmological perturbations
Bardeen, J. M. (1980) · Physical Review D · doi:10.1103/physrevd.22.1882 · Cited by 2,393
Perturbations of a Cosmological Model and Angular Variations of the Microwave Background
Sachs, R. K., & Wolfe, A. M. (1967) · The Astrophysical Journal · doi:10.1086/148982 · Cited by 1,815
Primeval Adiabatic Perturbation in an Expanding Universe
Peebles, P. J. E., & Yu, J. T. (1970) · The Astrophysical Journal · doi:10.1086/150713 · Cited by 1,230
Cited by
The EAGLE project: simulating the evolution and assembly of galaxies and their environments
Schaye, J., Crain, R. A., Bower, R. G., Furlong, M., Schaller, M., Theuns, T., Dalla Vecchia, C., Frenk, C. S., McCarthy, I. G., Helly, J. C., et al. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu2058 · Cited by 3,601
Cole, S., Percival, W. J., Peacock, J. A., Norberg, P., Baugh, C. M., Frenk, C. S., Baldry, I., Bland-Hawthorn, J., Bridges, T., Cannon, R., et al. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09318.x · Cited by 2,094
What Shapes the Luminosity Function of Galaxies?
Benson, A. J., Bower, R. G., Frenk, C. S., Lacey, C. G., Baugh, C. M., & Cole, S. (2003) · The Astrophysical Journal · doi:10.1086/379160 · Cited by 893
Mandelbaum, R., Seljak, U., Kauffmann, G., Hirata, C. M., & Brinkmann, J. (2006) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2006.10156.x · Cited by 728
The Dependence of Halo Clustering on Halo Formation History, Concentration, and Occupation
Wechsler, R. H., Zentner, A. R., Bullock, J. S., Kravtsov, A. V., & Allgood, B. (2006) · The Astrophysical Journal · doi:10.1086/507120 · Cited by 567
Metadata
- Authors
- COORAY, A., & SHETH, R.
- Venue
- Physics Reports
- Publisher
- Elsevier BV
- Published
- 2002-12
- Volume
- 372
- Issue
- 1
- Pages
- 1-129
- ISSN
- 0370-1573 (ISSN-L)
- OpenAlex
- W2018719255
- Cited by
- 2,042
- References
- 5
- FWCI
- 31.74
- Type
- journal article
- Language
- en
- Open access
- green
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