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QUBIC: the Q&U Bolometric Interferometer for Cosmology

TitleQUBIC: the Q&U Bolometric Interferometer for Cosmology
Publication TypeJournal Article
Year of Publication2012
AuthorsPiat, M, Battistelli, E, Bau, A, Bennett, D, Bergé, L, Bernard, JP, de Bernardis, P, Bigot-Sazy, MA, Bordier, G, Bounab, A, Bréelle, E, Bunn, EF, Calvo, M, Charlassier, R, Collin, S, Cruciani, A, Curran, G, Dumoulin, L, Gault, A, Gervasi, M, Ghribi, A, Giard, M, Giordano, C, Giraud-Heraud, Y, Gradziel, M, Guglielmi, L, Hamilton, JC, Haynes, V, Kaplan, J, Korotkov, A, Lande, J, Maffei, B, Maiello, M, Malu, S, Marnieros, S, Martino, J, Masi, S, Montier, L, Murphy, A, Nati, F, O'Sullivan, C, Pajot, F, Parisel, C, Passerini, A, Peterzen, S, Piacentini, F, Piccirillo, L, Pisano, G, Polenta, G, Prele, D, Romano, D, Rosset, C, Salatino, M, Schillaci, A, Sironi, G, Sordini, R, Spinelli, S, Tartari, A, Timbie, P, Tucker, G, Vibert, L, Voisin, F, Watson, RA, Zannoni, M
JournalJournal of Low Temperature Physics
Volume167
Pagination872-878
Date PublishedJun
ISBN Number0022-2291
Accession NumberWOS:000303461600048
Abstract

The primordial B-mode polarisation of the Cosmic Microwave Background is the imprints of the gravitational wave background generated by inflation. Observing the B-mode is up to now the most direct way to constrain the physics of the primordial Universe, especially inflation. To detect these B-modes, high sensitivity is required as well as an exquisite control of systematics effects. To comply with these requirements, we propose a new instrument called QUBIC (Q and U Bolometric Interferometer for Cosmology) based on bolometric interferometry. The control of systematics is obtained with a close-packed interferometer while bolometers cooled to very low temperature allow for high sensitivity. We present the architecture of this new instrument, the status of the project and the self-calibration technique which allows accurate measurement of the instrumental systematic effects.

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