The BOOMERanG experiment has recently produced detailed maps of the Cosmic Microwave Background, where sub-horizon structures are resolved with good signal to noise ratio. A power spectrum (spherical harmonics) analysis of the maps detects three peaks, at multipoles l = (213(-13)(+10)), (541(-32)(+20)), (845(-25)(+12)). In this paper we discuss the data analysis and the implications; of these results for cosmology.

l-space spectroscopy of the Cosmic Microwave Background with the BOOMERanG experiment

NATOLI, Paolo;
2002

Abstract

The BOOMERanG experiment has recently produced detailed maps of the Cosmic Microwave Background, where sub-horizon structures are resolved with good signal to noise ratio. A power spectrum (spherical harmonics) analysis of the maps detects three peaks, at multipoles l = (213(-13)(+10)), (541(-32)(+20)), (845(-25)(+12)). In this paper we discuss the data analysis and the implications; of these results for cosmology.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11392/1737913
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