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Cosmic Complementarity: [ITAL]H[/ITAL][TINF]0[/TINF] and Ω[TINF][CLC][ITAL]m[/ITAL][/CLC][/TINF] from Combining Cosmic Microwave Background Experiments and Redshift Surveys

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Eisenstein, Daniel J., Hu, Wayne, Tegmark, Max·1998·The Astrophysical Journal

Abstract

We show that the detection of acoustic oscillations in both upcoming cosmic microwave background (CMB) satellite experiments and large-redshift surveys can yield 5% determinations of H 0 and Ω m , an order-of-magnitude improvement over CMB data alone. CMB anisotropies provide the sound horizon at recombination as a standard ruler. For reasonable baryon fractions, this scale is imprinted on the galaxy power spectrum as a series of spectral features. Measuring these features in redshift space determines the Hubble constant, which in turn yields Ω m once combined with CMB data. Since the oscillations in both power spectra are frozen-in at recombination, this test is insensitive to low-redshift cosmology.

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Metadata

Authors
Eisenstein, D. J., Hu, W., & Tegmark, M.
Venue
The Astrophysical Journal
Published
1998-09-10
Volume
504
Issue
2
Pages
L57-L60
ISSN
0004-637X (ISSN-L)
OpenAlex
W2114310261
Cited by
250
References
0
FWCI
7.14
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Cosmic Complementarity: [ITAL]H[/ITAL][TINF]0[/TINF] and Ω[TINF][CLC][ITAL]m[/ITAL][/CLC][/TINF] from Combining Cosmic Microwave Background Experiments and Redshift Surveys. https://app.cochat.ai/papers/10.1086/311582
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Eisenstein, D. J., Hu, W., & Tegmark, M. (1998). Cosmic Complementarity: [ITAL]H[/ITAL][TINF]0[/TINF] and Ω[TINF][CLC][ITAL]m[/ITAL][/CLC][/TINF] from Combining Cosmic Microwave Background Experiments and Redshift Surveys. The Astrophysical Journal. https://doi.org/10.1086/311582

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