Piat, M., Rosset, C. and Pisano, Giampaolo ![]() |
Official URL: http://arxiv.org/abs/astro-ph/0412590
Abstract
The characterisation of CMB polarisation is one of the next challenge in observationnal cosmology. This is especially true for the so-called B-modes that are at least 3 order of magnitude lower than CMB temperature fluctuations. A precise measurement of the angular power spectrum of these B-modes will give important constraints on inflation parameters. In this talk, I will describe two complementary experiments, BRAIN and CLOVER, dedicated to CMB polarisation measurement. These experiments are proposed to be installed in Dome-C, Antarctica, to take advantage of the extreme dryness of the atmosphere and to allow long integration time.
Item Type: | Conference or Workshop Item (Paper) |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Publisher: | EDP Sciences |
Related URLs: | |
Last Modified: | 27 Oct 2022 09:35 |
URI: | https://orca.cardiff.ac.uk/id/eprint/66569 |
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