The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.
Power Spectra for Cold Dark Matter and Its Variants
Open accessAbstract
The bulk of recent cosmological research has focused on the adiabatic cold dark matter model and its simple extensions. Here we present an accurate fitting formula that describes the matter transfer functions of all common variants, including mixed dark matter models. The result is a function of wavenumber, time, and six cosmological parameters: the massive neutrino density, number of neutrino species degenerate in mass, baryon density, Hubble constant, cosmological constant, and spatial curvature. We show how observational constraints—e.g., the shape of the power spectrum, the abundance of clusters and damped Lyα systems, and the properties of the Lyα forest—can be extended to a wide range of cosmologies, which includes variations in the neutrino and baryon fractions in both high-density and low-density universes.
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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
The Cosmic Microwave Background Spectrum from the Full COBE FIRAS Data Set
Fixsen, D. J., Cheng, E. S., Gales, J. M., Mather, J. C., Shafer, R. A., & Wright, E. L. (1996) · The Astrophysical Journal · doi:10.1086/178173 · Cited by 1,780 · cited 1×
“The CMB temperature isH0\ 100given by K; the best determination to dateTCMB\ 2.7#2.7is 2.728^ 0.004 K (Fixsen et al. 1996 ; 95% conÐdence interval), at which it is Ðxed for most of our expressions.”
MethodInfluential
Cited by
Cosmological parameters from CMB and other data: A Monte Carlo approach
Lewis, A., & Bridle, S. (2002) · Physical Review D · doi:10.1103/physrevd.66.103511 · Cited by 3,495
Carroll, S. M. (2001) · Living Reviews in Relativity · doi:10.12942/lrr-2001-1 · Cited by 2,650
Cosmology and Fundamental Physics with the Euclid Satellite
The Euclid Theory Working Group, Amendola, L., Appleby, S., Bacon, D., Baker, T., Baldi, M., Bartolo, N., Blanchard, A., Bonvin, C., Borgani, S., et al. (2013) · Living Reviews in Relativity · doi:10.12942/lrr-2013-6 · Cited by 899
Dalal, N., Doré, O., Huterer, D., & Shirokov, A. (2008) · Physical Review D · doi:10.1103/physrevd.77.123514 · Cited by 830
The Evolution of X-Ray Clusters of Galaxies
Rosati, P., Borgani, S., & Norman, C. (2002) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.40.120401.150547 · Cited by 482
Metadata
- Authors
- Eisenstein, D. J., & Hu, W.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1999-01-20
- Volume
- 511
- Issue
- 1
- Pages
- 5-15
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2134287871
- Cited by
- 910
- References
- 2
- FWCI
- 21.24
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Eisenstein, D. J., & Hu, W. (1999). Power Spectra for Cold Dark Matter and Its Variants. The Astrophysical Journal. https://doi.org/10.1086/306640
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