Efficient Computation of CMB anisotropies in closed FRW models

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dc.creatorLewis, Antony
dc.creatorChallinor, Anthony
dc.creatorLasenby, Anthony
dc.date1999-11-10
dc.date2000-06-01
dc.date.accessioned2026-07-07T11:08:31Z
dc.date.available2026-07-07T11:08:31Z
dc.descriptionWe 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.
dc.description4 pages, 1 figure. Corrected/updated references. Accepted by ApJ. For the F90 source code see http://www.mrao.cam.ac.uk/~aml1005/cmb/
dc.identifierhttps://arxiv.org/abs/astro-ph/9911177
dc.identifierhttp://arxiv.org/abs/astro-ph/9911177
dc.identifierAstrophys.J.538:473-476,2000
dc.identifierdoi:10.1086/309179
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190159
dc.subjectAstrophysics
dc.titleEfficient Computation of CMB anisotropies in closed FRW models
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