Efficient Computation of CMB anisotropies in closed FRW models

Preprint

1 June 2000

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/9911177

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.

Keywords

EFFICIENT COMPUTATION
METHOD TO CALCULATE
CMB ANISOTROPIES
POLARIZATION
FRW MODELS
CLOSED FRW
MODELS

All Related Versions

Version 1, 1999-11-10, ArXiv
Version 2, 2000-06-01, ArXiv
Published version: The Astrophysical Journal, 538 (2), 473.

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