Imaging the Early Universe with the Boomerang Experiment

Details Imaging the Early Universe with the Boomerang Experiment Imaging the Early Universe with the Boomerang Experiment

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003trso.conf..209m&link_type=abstract

2001: A RELATIVISTIC SPACETIME ODYSSEY Experiments & Theoretical Viewpoints on General Relativity and Quantum Gravity. Proceedin

Mathematics

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Scientific paper

The BOOMERanG experiment has recently detected temperature fluctuations the Cosmic Microwave Background (CMB), the otherwise isotropic radiation coming from the early Universe. These anisotropies have a low contrast (about 30 ppm) and feature a peculiar angular power spectrum at angles corresponding to sub-horizon scales at recombination. In the current cosmological model, these structures result from acoustic oscillations in the primeval plasma. In the framework of the Hot Big Bang theory with the inflationary hypothesis, the statistical properties of the image of the CMB allow us to measure most of the cosmological parameters.

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