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Thermal architecture for the QUBIC cryogenic receiver
Author(s): A. J. May; C. Chapron; G. Coppi; G. D'Alessandro; P. de Bernardis; S. Masi; S. Melhuish; M. Piat; L. Piccirillo; A. Schillaci; J.-P. Thermeau; P. Ade; G. Amico; D. Auguste; J. Aumont; S. Banfi; G. Barbarán; P. Battaglia; E. Battistelli; A. Baù; B. Bélier; D. Bennett; L. Bergé; J.-Ph. Bernard; M. Bersanelli; M.-A. Bigot-Sazy; N. Bleurvacq; J. Bonaparte; J. Bonis; G. Bordier; E. Bréelle; E. Bunn; D. Burke; D. Buzi; A. Buzzelli; F. Cavaliere; P. Chanial; R. Charlassier; F. Columbro; A. Coppolecchia; F. Couchot; R. D'Agostino; G. De Gasperis; M. De Leo; M. De Petris; A. Di Donato; L. Dumoulin; A. Etchegoyen; A. Fasciszewski; C. Franceschet; M. M. Gamboa Lerena; B. García; X. Garrido; M. Gaspard; A. Gault; D. Gayer; M. Gervasi; M. Giard; Y. Giraud-Héraud; M. Gómez Berisso; M. González; M. Gradziel; L. Grandsire; E. Guerrard; J.-Ch. Hamilton; D. Harari; V. Haynes; S. Henrot-Versillé; D. T. Hoang; F. Incardona; E. Jules; J. Kaplan; A. Korotkov; C. Kristukat; L. Lamagna; S. Loucatos; T. Louis; A. Lowitz; V. Lukovic; R. Luterstein; B. Maffei; S. Marnieros; A. Mattei; M. A. McCulloch; M. C. Medina; L. Mele; A. Mennella; L. Montier; L. M. Mundo; J. A. Murphy; J. D. Murphy; C. O'Sullivan; E. Olivieri; A. Paiella; F. Pajot; A. Passerini; H. Pastoriza; A. Pelosi; C. Perbost; O. Perdereau; F. Pezzotta; F. Piacentini; G. Pisano; G. Polenta; D. Prêle; R. Puddu; D. Rambaud; P. Ringegni; G. E. Romero; M. Salatino; C. G. Scóccola; S. Scully; S. Spinelli; M. Stolpovskiy; F. Suarez; A. Tartari; P. Timbie; S. A. Torchinsky; M. Tristram; V. Truongcanh; C. Tucker; G. Tucker; S. Vanneste; D. Viganó; N. Vittorio; F. Voisin; B. Watson; F. Wicek; M. Zannoni; A. Zullo
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Paper Abstract

QUBIC, the QU Bolometric Interferometer for Cosmology, is a novel forthcoming instrument to measure the B-mode polarization anisotropy of the Cosmic Microwave Background. The detection of the B-mode signal will be extremely challenging; QUBIC has been designed to address this with a novel approach, namely bolometric interferometry. The receiver cryostat is exceptionally large and cools complex optical and detector stages to 40 K, 4 K, 1 K and 350 mK using two pulse tube coolers, a novel 4He sorption cooler and a double-stage 3He/4He sorption cooler. We discuss the thermal and mechanical design of the cryostat, modelling and thermal analysis, and laboratory cryogenic testing.

Paper Details

Date Published: 9 July 2018
PDF: 14 pages
Proc. SPIE 10708, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX, 107083V (9 July 2018); doi: 10.1117/12.2312085
Show Author Affiliations
A. J. May, The Univ. of Manchester (United Kingdom)
C. Chapron, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
G. Coppi, The Univ. of Manchester (United Kingdom)
G. D'Alessandro, Sapienza Univ. di Roma (Italy)
INFN (Italy)
P. de Bernardis, Sapienza Univ. di Roma (Italy)
INFN (Italy)
S. Masi, Sapienza Univ. di Roma (Italy)
INFN (Italy)
S. Melhuish, The Univ. of Manchester (United Kingdom)
M. Piat, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
L. Piccirillo, The Univ. of Manchester (United Kingdom)
A. Schillaci, Sapienza Univ. di Roma (Italy)
Caltech (United States)
J.-P. Thermeau, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
P. Ade, Cardiff Univ. (United Kingdom)
G. Amico, Sapienza Univ. di Roma (Italy)
INFN (Italy)
D. Auguste, Lab. de l'Accélérateur Linéaire, CNRS, IN2P3 (France)
J. Aumont, Institut d'Astrophysique Spatiale, CNRS, NSU (France)
S. Banfi, Univ. degli Studi di Milano-Bicocca (Italy)
INFN (Italy)
G. Barbarán, Comisión Nacional de Energía Atómica (Argentina)
P. Battaglia, Univ. degli Studi di Milano (Italy)
E. Battistelli, Sapienza Univ. di Roma (Italy)
INFN (Italy)
A. Baù, Univ. degli Studi di Milano-Bicocca (Italy)
INFN (Italy)
B. Bélier, Ctr. de Nanosciences et de Nanotechnologies (France)
D. Bennett, National Univ. of Ireland, Maynooth (Ireland)
L. Bergé, Ctr. de Sciences Nucléaires et de Sciences de la Matière de Masse, CNRS, IN2P3 (France)
J.-Ph. Bernard, Institut de Recherche en Astrophysique et Planétologie, CNRS, INSU (France)
M. Bersanelli, Univ. degli Studi di Milano (Italy)
M.-A. Bigot-Sazy, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
N. Bleurvacq, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
J. Bonaparte, Ctr. Atomico Constituyentes (Argentina)
J. Bonis, Lab. de l'Accélérateur Linéaire, CNRS, IN2P3 (France)
G. Bordier, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
E. Bréelle, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
E. Bunn, Univ. of Richmond (United States)
D. Burke, National Univ. of Ireland, Maynooth (Ireland)
D. Buzi, Sapienza Univ. di Roma (Italy)
INFN (Italy)
A. Buzzelli, Univ. degli Studi di Roma "Tor Vergata" (Italy)
INFN (Italy)
F. Cavaliere, Univ. degli Studi di Milano (Italy)
P. Chanial, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
R. Charlassier, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
F. Columbro, Sapienza Univ. di Roma (Italy)
INFN (Italy)
A. Coppolecchia, Sapienza Univ. di Roma (Italy)
INFN (Italy)
F. Couchot, Lab. de l'Accélérateur Linéaire, CNRS, IN2P3 (France)
R. D'Agostino, Univ. degli Studi di Roma "Tor Vergata" (Italy)
G. De Gasperis, Univ. degli Studi di Roma "Tor Vergata" (Italy)
INFN (Italy)
M. De Leo, Sapienza Univ. di Roma (Italy)
INFN (Italy)
M. De Petris, Sapienza Univ. di Roma (Italy)
INFN (Italy)
A. Di Donato, Ctr. Atomico Constituyentes (Argentina)
L. Dumoulin, Ctr. de Sciences Nucléaires et de Sciences de la Matière de Masse, CNRS, IN2P3 (France)
A. Etchegoyen, Instituto de Tecnologías en Detección y Astropartículas (Argentina)
A. Fasciszewski, Ctr. Atomico Constituyentes (Argentina)
C. Franceschet, Univ. degli Studi di Milano (Italy)
M. M. Gamboa Lerena, Univ. Nacional de la Plata (Argentina)
B. García, Instituto de Tecnologías en Detección y Astropartículas (Argentina)
X. Garrido, Lab. de l'Accélérateur Linéaire, CNRS, IN2P3 (France)
M. Gaspard, Lab. de l'Accélérateur Linéaire, CNRS, IN2P3 (France)
A. Gault, Univ. of Wisconsin-Madison (United States)
D. Gayer, National Univ. of Ireland, Maynooth (Ireland)
M. Gervasi, Univ. degli Studi di Milano-Bicocca (Italy)
INFN (Italy)
M. Giard, Institut de Recherche en Astrophysique et Planetologie, CNRS, INSU (France)
Y. Giraud-Héraud, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
M. Gómez Berisso, Ctr. Atómico Bariloche (Argentina)
Instituto Balseiro (Argentina)
M. González, Ctr. Atómico Bariloche (Argentina)
Instituto Balseiro (Argentina)
M. Gradziel, National Univ. of Ireland, Maynooth (Ireland)
L. Grandsire, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
E. Guerrard, Lab. de l'Accélérateur Linéaire, CNRS, IN2P3 (France)
J.-Ch. Hamilton, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
D. Harari, Ctr. Atómico Bariloche (Argentina)
Instituto Balseiro (Argentina)
V. Haynes, The Univ. of Manchester (United Kingdom)
S. Henrot-Versillé, Lab. de l'Accélérateur Linéaire, CNRS, IN2P3 (France)
D. T. Hoang, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
Univ. of Science and Technology of Hanoi (Viet Nam)
Vietnam Academy of Science and Technology (Viet Nam)
F. Incardona, Univ. degli Studi di Milano (Italy)
E. Jules, Lab. de l'Accélérateur Linéaire, CNRS, IN2P3 (France)
J. Kaplan, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
A. Korotkov, Brown Univ. (United States)
C. Kristukat, Univ. Nacional de San Martín (Argentina)
L. Lamagna, Sapienza Univ. di Roma (Italy)
INFN (Italy)
S. Loucatos, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
T. Louis, Lab. de l'Accélérateur Linéaire, CNRS, IN2P3 (France)
A. Lowitz, Univ. of Wisconsin-Madison (United States)
V. Lukovic, Univ. degli Studi di Roma "Tor Vergata" (Italy)
R. Luterstein, Ctr. Atomico Constituyentes (Argentina)
B. Maffei, Institut d'Astrophysique Spatiale, CNRS, NSU (France)
S. Marnieros, Ctr. de Sciences Nucléaires et de Sciences de la Matière de Masse, CNRS, IN2P3 (France)
A. Mattei, INFN (Italy)
M. A. McCulloch, The Univ. of Manchester (United Kingdom)
M. C. Medina, Instituto Argentino de Radioastronomía (Argentina)
L. Mele, Sapienza Univ. di Roma (Italy)
INFN (Italy)
A. Mennella, Univ. degli Studi di Milano (Italy)
INFN (Italy)
L. Montier, Institut de Recherche en Astrophysique et Planetologie, CNRS, INSU (France)
L. M. Mundo, Univ. Nacional de la Plata (Argentina)
J. A. Murphy, National Univ. of Ireland, Maynooth (Ireland)
J. D. Murphy, National Univ. of Ireland, Maynooth (Ireland)
C. O'Sullivan, National Univ. of Ireland, Maynooth (Ireland)
E. Olivieri, Ctr. de Sciences Nucléaires et de Sciences de la Matière de Masse, CNRS, IN2P3 (France)
A. Paiella, Sapienza Univ. di Roma (Italy)
INFN (Italy)
F. Pajot, Institut de Recherche en Astrophysique et Planetologie, CNRS, INSU (France)
A. Passerini, Univ. degli Studi di Milano-Bicocca (Italy)
INFN (Italy)
H. Pastoriza, Ctr. Atómico Bariloche (Argentina)
Instituto Balseiro (Argentina)
A. Pelosi, Sapienza Univ. di Roma (Italy)
INFN (Italy)
C. Perbost, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
O. Perdereau, Lab. de l'Accélérateur Linéaire, CNRS, IN2P3 (France)
F. Pezzotta, Univ. degli Studi di Milano (Italy)
F. Piacentini, Sapienza Univ. di Roma (Italy)
INFN (Italy)
G. Pisano, Cardiff Univ. (United Kingdom)
G. Polenta, Sapienza Univ. di Roma (Italy)
INFN (Italy)
D. Prêle, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
R. Puddu, Sapienza Univ. di Roma (Italy)
INFN (Italy)
D. Rambaud, Institut de Recherche en Astrophysique et Planetologie, CNRS, INSU (France)
P. Ringegni, Univ. Nacional de la Plata (Argentina)
G. E. Romero, Instituto Argentino de Radioastronomía (Argentina)
M. Salatino, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
C. G. Scóccola, Univ. Nacional de la Plata (Argentina)
S. Scully, Institute of Technology Carlow (Ireland)
S. Spinelli, Univ. degli Studi di Milano-Bicocca (Italy)
M. Stolpovskiy, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
F. Suarez, Instituto de Tecnologías en Detección y Astropartículas (Argentina)
A. Tartari, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
P. Timbie, Univ. of Wisconsin-Madison (United States)
S. A. Torchinsky, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
M. Tristram, Lab. de l'Accélérateur Linéaire, CNRS, IN2P3 (France)
V. Truongcanh, Lab. de l'Accélérateur Linéaire, CNRS, IN2P3 (France)
C. Tucker, Cardiff Univ. (United Kingdom)
G. Tucker, Brown Univ. (United States)
S. Vanneste, Lab. de l'Accélérateur Linéaire, CNRS, IN2P3 (France)
D. Viganó, Univ. degli Studi di Milano (Italy)
N. Vittorio, Univ. degli Studi di Roma "Tor Vergata" (Italy)
INFN (Italy)
F. Voisin, Astroparticule et Cosmologie, CNRS, IN2P3 (France)
B. Watson, The Univ. of Manchester (United Kingdom)
F. Wicek, Lab. de l'Accélérateur Linéaire, CNRS, IN2P3 (France)
M. Zannoni, Univ. degli Studi di Milano-Bicocca (Italy)
INFN (Italy)
A. Zullo, Sapienza Univ. di Roma (Italy)
INFN (Italy)


Published in SPIE Proceedings Vol. 10708:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX
Jonas Zmuidzinas; Jian-Rong Gao, Editor(s)

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