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Efficient Computation of Cosmic Microwave Background Anisotropies in Closed Friedmann‐Robertson‐Walker Models
The Astrophysical Journal · 2000 · Vol. 538(2) · pp. 473–476
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.
Cosmology and Gravitation TheoriesBlack Holes and Theoretical PhysicsAdvanced Differential Geometry ResearchCosmic microwave backgroundFriedmann equationsPhysicsAnisotropyComputationPolarization (electrochemistry)CurvatureScalar (mathematics)Cosmic background radiationCOSMIC cancer database
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References
A Line-of-Sight Integration Approach to Cosmic Microwave Background Anisotropies
The Astrophysical Journal · 1996 · 1,870 citations
Gauge-invariant cosmological perturbations
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · 1980 · 2,267 citations
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