Cosmological Inflation, Microwave Background Anisotropies and Large Scale Structure of the Universe

Details Cosmological Inflation, Microwave Background Anisotropies and Large Scale Structure of the Universe Cosmological Inflation, Microwave Background Anisotropies and Large Scale Structure of the Universe

1994-12-05

arxiv.org/abs/astro-ph/9412012v2

Astronomy and Astrophysics

Astrophysics

Corrected version (Latex bugs removed), 34 pages, RevTex using Latex 2.09, Hard copy figures will be sent upon request. (To ap

Scientific paper

Cosmological inflation provides the simplest and most promising mechanism for generating fluctuations for structure formation. Using powerful Hamilton-Jacobi methods, I will describe (1) how to compute density fluctuations and cosmic microwave anisotropies arising from inflation, and (2) improvements of the Zel'dovich approximation describing gravitational collapse. I compare these results with the latest cosmological observations.

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