New physics from the Cosmic Microwave Background

Details New physics from the Cosmic Microwave Background New physics from the Cosmic Microwave Background

1999-11-17

arxiv.org/abs/astro-ph/9911325v1

Astronomy and Astrophysics

Astrophysics

18 pages using iopconf1.sty, including 2 colour and 2 b&w figures, to appear in "Beyond the Desert `99", edited by H.V. Klapdo

Scientific paper

I review the present status of the Cosmic Microwave Background, with some emphasis on the current and future implications for particle physics. Conclusions are: gravitational instability in a dark matter dominated universe grew today's structure; the Universe remained neutral until z<~50; the CMB power spectrum peaks at 150<~l<~350; the large-scale structure of spacetime appears to be simple; something like inflation is something like proven; we will learn a great deal about cosmology, astrophysics and particle physics from MAP and Planck.

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