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Cited by 158

The DOI matches its Crossref record; 5 of the 5 references it cites were found in a registry or an index.

The Damping Tail of Cosmic Microwave Background Anisotropies

Open access
Hu, Wayne, White, Martin·1997·The Astrophysical Journal

Abstract

By decomposing the damping tail of cosmic microwave background (CMB) anisotropies into a series of transfer functions representing individual physical effects, we provide ingredients that will aid in the reconstruction of the cosmological model from small-scale CMB anisotropy data. We accurately calibrate the model-independent effects of diffusion and reionization damping, which provide potentially the most robust information on the background cosmology. Removing these effects, we uncover model-dependent processes, such as the acoustic peak modulation and gravitational enhancement, that can help distinguish between alternate models of structure formation and provide windows into the evolution of fluctuations at various stages in their growth.

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Metadata

Authors
Hu, W., & White, M.
Venue
The Astrophysical Journal
Published
1997-04-20
Volume
479
Issue
2
Pages
568-579
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2116034383
Cited by
158
References
5
FWCI
9.54
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: The Damping Tail of Cosmic Microwave Background Anisotropies. https://app.cochat.ai/papers/10.1086/303928
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Hu, W., & White, M. (1997). The Damping Tail of Cosmic Microwave Background Anisotropies. The Astrophysical Journal. https://doi.org/10.1086/303928

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