Dodecahedral space topology as an explanation for weak wide-angle temperature correlations in the cosmic microwave background-Reference-Cited by-同舟云学术

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Dodecahedral space topology as an explanation for weak wide-angle temperature correlations in the cosmic microwave background

Published:2003-10 Issue:6958 Volume:425 Page:593-595
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Luminet Jean-Pierre,Weeks Jeffrey R.,Riazuelo Alain,Lehoucq Roland,Uzan Jean-Philippe

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/nature01944.pdf

Reference12 articles.

1. Bennett, C. L. et al. First year Wilkinson Microwave Anisotropy Probe (WMAP 1) observations: Preliminary maps and basic results. Astrophys. J. Suppl. 148, 1–27 (2003)

2. Spergel, D. N. et al. First year Wilkinson Microwave Anisotropy Probe (WMAP 1) observations: Determination of cosmological parameters. Astrophys. J. Suppl. 148, 175–194 (2003)

3. Contaldi, C. R., Peloso, M., Kofman, L. & Linde, A. Suppressing the lower multipoles in the CMB anisotropies. J. Cosmol. Astropart. Phys. 07, 002 (2003)

4. Cline, J. M., Crotty, P. & Lesgourgues, J. Does the small CMB quadrupole moment suggest new physics? J. Cosmol. Astropart. Phys. (in the press); preprint at 〈 http://arXiv.org/astro-ph/0304558 〉 (2003)

5. Efstathiou, G. Is the low CMB quadrupole a signature of spatial curvature? Mon. Not. R. Astron. Soc. 343, L95–L98 (2003)

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