QUBIC - The Q U Bolometric Interferometer for Cosmology - A novel way to look at the polarized Cosmic Microwave Background

A. Mennella,P. A. R. Ade, J. Aumont, S. Banfi,P. Battaglia,E. S. Battistelli,A. Baù,B. Bélier,D. Bennett, L. Bergé,J. Ph. Bernard,M. Bersanelli, M. A. Bigot-Sazy,N. Bleurvacq, G. Bordier,J. Brossard,E. F. Bunn,D. P. Burke, D. Buzi, A. Buzzelli, D. Cammilleri,F. Cavaliere, P. Chanial,C. Chapron,F. Columbro,G. Coppi,A. Coppolecchia, F. Couchot,R. D'Agostino,G. D'Alessandro,P. de Bernardis,G. De Gasperis,M. De Leo, M. De Petris,T. Decourcelle,F. Del Torto,L. Dumoulin,A. Etchegoyen,C. Franceschet,B. Garcia,A. Gault,D. Gayer,M. Gervasi,A. Ghribi, M. Giard, Y. Giraud-Héraud,M. Gradziel, L. Grandsire, J. Ch. Hamilton,D. Harari, V. Haynes,S. Henrot-Versillé,N. Holtzer,F. Incardona,J. Kaplan, A. Korotkov,N. Krachmalnicoff, L. Lamagna, J. Lande, S. Loucatos,A. Lowitz,V. Lukovic, B. Maffei,S. Marnieros, J. Martino,S. Masi,A. May,M. McCulloch, M. C. Medina,L. Mele,S. Melhuish,L. Montier, A. Murphy,D. Néel, M. W. Ng, C. O'Sullivan, A. Paiella, F. Pajot,A. Passerini, A. Pelosi,C. Perbost,O. Perdereau, F. Piacentini,M. Piat, L. Piccirillo,G. Pisano,D. Préle,R. Puddu, D. Rambaud,O. Rigaut, G. E. Romero,M. Salatino, A. Schillaci,S. Scully, M. Stolpovskiy,F. Suarez,A. Tartari,P. Timbie,S. Torchinsky,M. Tristram,C. Tucker,G. Tucker,D. Viganò, N. Vittorio, F. Voisin,B. Watson,M. Zannoni, A. Zullo

arXiv: Instrumentation and Methods for Astrophysics(2018)

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摘要
In this paper we describe QUBIC, an experiment that takes up the challenge posed by the detection of primordial gravitational waves with a novel approach, that combines the sensitivity of state-of-the art bolometric detectors with the systematic effects control typical of interferometers. The so-called "self-calibration" is a technique deeply rooted in the interferometric nature of the instrument and allows us to clean the measured data from instrumental effects. The first module of QUBIC is a dual band instrument (150 GHz and 220 GHz) that will be deployed in Argentina during the Fall 2018.
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cosmology,microwave
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