期刊
ASTROPHYSICAL JOURNAL
卷 538, 期 2, 页码 473-476出版社
IOP PUBLISHING LTD
DOI: 10.1086/309179
关键词
cosmic microwave background; cosmology : theory
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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