Masi, S., de Bernardis, P., Giordano, C., Nati, F., Piacentini, F., Polenta, G., Veneziani, M., Gervasi, M., Sironi, G., Tartari, A., Zannoni, M., Peterzen, S., Bartlett, J., Giraud-Heraud, Y., Piat, M., Rosset, C., Giard, M., Pons, R., Maffei, B., Ade, Peter A. R. ![]() ![]() ![]() |
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Abstract
In the current cosmological scenario, part of the linearly polarized emission of the CMB is expected to be rotational (B-modes). This component is due to tensor perturbations of the metric produced by primordial gravitational waves, which are generated a split-second after the Big Bang. The signal expected is of the order of ≲ 0.1 μK, well below the non-rotational component of the polarization signal (E-modes), and beyond the sensitivity of present generation instruments. New, more sensitive instruments are developed in several labs, with the goal to measure the B-modes. Control of systematics and foregrounds will be the key to make the results of these experiments believable. In this paper we shortly outline BRAIN, a bolometric interferometer devoted to B-modes research, and its pathfinder experiment, devoted to test the Dome-C site.
Item Type: | Article |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Additional Information: | Dome C Astronomy & Astrophysics Meeting, Toulouse, France, January 2005. Pdf uploaded in accordance with publisher's policy at http://www.sherpa.ac.uk/romeo/issn/1633-4760/ (accessed 17/04/2014) |
Publisher: | EDP Sciences |
ISSN: | 1633-4760 |
Date of First Compliant Deposit: | 30 March 2016 |
Last Modified: | 11 May 2023 18:58 |
URI: | https://orca.cardiff.ac.uk/id/eprint/36487 |
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