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Module: Kosmische Hintergrundstrahlung

Sequence: Start

Branching Point: The Most Ancient Radiation in the Universe

Sequence: Cosmic Background Radiation

Slide: Where Everything Started From

Slide: The Cosmological Timeline

Slide: Nucleosynthesis

Slide: Recombination Era

Slide: The Universe Becomes Transparent

Slide: How did Anisotropies Form in Early Universe?

Slide: The Origin of Galaxies and Clusters

Sequence: peebles

Slide: Nucleosynthesis in the Big Bang

Slide: Extracts from Alan Guth's The Inflationary Universe: The Quest for a New Theory of Cosmic Origins.

Sequence: The Tenerife Experiment

Slide: The Tenerife Experiment

Slide: Twin-Horn Microwave Receivers

Slide: Function Principle of a Twin Horn Receiver

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Slide: Tenerife Experiment: The Result

Sequence: COBE

Slide: The COBE Satellite

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Slide: COBE Instruments

Slide: The Differential Microwave Radiometer

Slide: Sky Maps from COBE

Slide: Fluctuations in the Cosmisc Background Radiation

Sequence: WMAP

Slide: The WMAP Satellite

Slide: Results of the WMAP Mission

Slide: The Microwave Sky as Seen by WMAP

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The Origin of Galaxies and Clusters

Astrophysicists and cosmologists have developed models that shall explain how spacous structures in universe like galaxies and clusters could develop.