The DOI matches its Crossref record; 3 of the 3 references it cites were found in a registry or an index.
Cosmic Complementarity: Joint Parameter Estimation from Cosmic Microwave Background Experiments and Redshift Surveys
Open accessAbstract
We study the ability of future cosmic microwave background anisotropy experiments and redshift surveys to constrain a 13-dimensional parameterization of the adiabatic cold dark matter model. Each alone is unable to determine all parameters to high accuracy. However, considered together, one data set resolves the difficulties of the other, allowing certain degenerate parameters to be determined with far greater precision. We treat in detail the degeneracies involving the classical cosmological parameters, massive neutrinos, tensor-scalar ratio, bias, and reionization optical depth as well as how redshift surveys can resolve them. We discuss the opportunities for internal and external consistency checks on these measurements. Previous papers on parameter estimation have generally treated smaller parameter spaces; in direct comparisons to these works, we tend to find weaker constraints and suggest numerical explanations for the discrepancies.
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Cites
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
Riess, A. G., Filippenko, A. V., Challis, P., Clocchiatti, A., Diercks, A., Garnavich, P. M., Gilliland, R. L., Hogan, C. J., Jha, S., Kirshner, R. P., et al. (1998) · The Astronomical Journal · doi:10.1086/300499 · Cited by 19,704
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
Big-bang nucleosynthesis enters the precision era
Schramm, D. N., & Turner, M. S. (1998) · Reviews of Modern Physics · doi:10.1103/revmodphys.70.303 · Cited by 353 · cited 1×
“We also allow the primordial helium fraction to vary but assume that the information from direct abundance measurements can be represented by a Gaussian prior (1 p) (Bond et al. 1997 ;Y p \ 0.24 ^ 0.02 Schramm & Turner 1998).”
MethodInfluential
Cited by
Cosmic Microwave Background Anisotropies
Hu, W., & Dodelson, S. (2002) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.40.060401.093926 · Cited by 745
Self-citationIntrinsic alignment-lensing interference as a contaminant of cosmic shear
Hirata, C. M., & Seljak, U. (2004) · Physical Review D · doi:10.1103/physrevd.70.063526 · Cited by 586
What does inflation really predict?
Tegmark, M. (2005) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2005/04/001 · Cited by 216
Self-citationCosmic tomographies: baryon acoustic oscillations and weak lensing
Zhan, H. (2006) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2006/08/008 · Cited by 60
Can a galaxy redshift survey measure dark energy clustering?
Takada, M. (2006) · Physical Review D · doi:10.1103/physrevd.74.043505 · Cited by 59
Metadata
- Authors
- Eisenstein, D. J., Hu, W., & Tegmark, M.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1999-06-10
- Volume
- 518
- Issue
- 1
- Pages
- 2-23
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W1498004781
- Cited by
- 338
- References
- 3
- FWCI
- 29.51
- Type
- journal article
- Language
- en
- Open access
- green
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