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Efficient Computation of Cosmic Microwave Background Anisotropies in Closed Friedmann‐Robertson‐Walker Models

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Lewis, Antony, Challinor, Anthony, Lasenby, Anthony·2000·The Astrophysical Journal

DOI 10.1086/309179

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Abstract

We implement the efficient line-of-sight method to calculate the anisotropy and polarization of the cosmic microwave background for scalar and tensor modes in almost Friedmann-Robertson-Walker models with positive spatial curvature. We present new results for the polarization power spectra in such models.

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Challinor, A. D. 1999a, Gen. Relativ. Gravitation, in press (preprint astro-ph/9903283) · arXiv
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Authors: Lewis, A., Challinor, A., & Lasenby, A.
Affiliations: University of Cambridge (GB)
ORCID: Lewis, Antony
Challinor, Anthony
Lasenby, Anthony
Venue: The Astrophysical Journal
Publisher: American Astronomical Society
Published: 2000-08
Volume: 538
Issue: 2
Pages: 473-476
ISSN: 0004-637X (ISSN-L)
1538-4357
DOI: 10.1086/309179
OpenAlex: W1944901286
Cited by: 4,920
References: 22
Citations by year: 2026: 226 · 2025: 298 · 2024: 272 · 2023: 263 · 2022: 265 · 2021: 291 · 2020: 327 · 2019: 278 · 2018: 281 · 2017: 259 · 2016: 325 · 2015: 252 · 2014: 270 · 2013: 250 · 2012: 234
FWCI: 17.05
Type: journal article
Language: en
Open access: bronze
doi.org
Locations: The Astrophysical Journal (publishedVersion)
arXiv (Cornell University) (submittedVersion)
CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
arXiv (Cornell University)
Topics: Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
Keywords: cosmic microwave background anisotropies, CMB polarization, line-of-sight integration, positive spatial curvature, scalar perturbations, tensor perturbations, cosmological perturbation theory

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Efficient Computation of Cosmic Microwave Background Anisotropies in Closed Friedmann‐Robertson‐Walker Models

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