Efficient computation of CMB anisotropies in closed FRW models - INSPIRE

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Efficient computation of CMB anisotropies in closed FRW models

Nov, 1999

4 pages

Published in:

Astrophys.J. 538 (2000) 473-476

e-Print:

astro-ph/9911177 [astro-ph]

DOI:

10.1086/309179

View in:

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Abstract: (arXiv)

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.

Note:

4 pages, 1 figure. Corrected/updated references. Accepted by ApJ. For the F90 source code see http://www.mrao.cam.ac.uk/~aml1005/cmb/ Journal-ref: Astrophys.J. 538 (2000) 473

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Figures(0)

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