The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.
Analytic approach to the perturbative expansion of nonlinear gravitational fluctuations in cosmological density and velocity fields
Abstract
Equations of self-gravitating systems in the Universe are solved by expanding as perturbation series in Fourier space. The formulas for the higher-order terms are given for density and velocity fields. We apply the formulas to several analytically integrable models whose linear density power spectra obey a single power law, and asymptotically approach the prediction of the cold-dark-matter scenario. We explicitly give the nonlinear gravitational evolution for the fields and its dependence on the initial spectrum.
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Citations
Cites
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
Cited by
Large-scale structure of the Universe and cosmological perturbation theory
Bernardeau, F., Colombi, S., Gaztañaga, E., & Scoccimarro, R. (2002) · Physics Reports · doi:10.1016/s0370-1573(02)00135-7 · Cited by 1,922
Desjacques, V., Jeong, D., & Schmidt, F. (2018) · Physics Reports · doi:10.1016/j.physrep.2017.12.002 · Cited by 817
The density and peculiar velocity fields of nearby galaxies
Strauss, M. A., & Willick, J. A. (1995) · Physics Reports · doi:10.1016/0370-1573(95)00013-7 · Cited by 567
Matsubara, T. (2008) · Physical Review D · doi:10.1103/physrevd.78.083519 · Cited by 255
Metadata
- Authors
- Makino, N., Sasaki, M., & Suto, Y.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 1992-07-15
- Volume
- 46
- Issue
- 2
- Pages
- 585-602
- ISSN
- 0556-2821 (ISSN-L)
- OpenAlex
- W1978879626
- Cited by
- 171
- References
- 1
- FWCI
- 1.97
- Type
- journal article
- Language
- en
- Open access
- closed
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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