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Related papers: QUBIC V: Cryogenic system design and performance

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Cryogenic calorimeters, also known as bolometers, are among the leading technologies for searching for rare events. The CUPID experiment is exploiting this technology to deploy a tonne-scale detector to search for neutrinoless double-beta…

Instrumentation and Detectors · Physics 2025-03-07 The CUPID Collaboration , K. Alfonso , A. Armatol , C. Augier , F. T. Avignone , O. Azzolini , A. S. Barabash , G. Bari , A. Barresi , D. Baudin , F. Bellini , G. Benato , L. Benussi , V. Berest , M. Beretta , M. Bettelli , M. Biassoni , J. Billard , F. Boffelli , V. Boldrini , E. D. Brandani , C. Brofferio , C. Bucci , M. Buchynska , J. Camilleri , A. Campani , J. Cao , C. Capelli , S. Capelli , V. Caracciolo , L. Cardani , P. Carniti , N. Casali , E. Celi , C. Chang , M. Chapellier , H. Chen , D. Chiesa , D. Cintas , M. Clemenza , I. Colantoni , S. Copello , O. Cremonesi , R. J. Creswick , A. D'Addabbo , I. Dafinei , F. A. Danevich , F. De Dominicis , M. De Jesus , P. de Marcillac , S. Dell'Oro , S. Di Domizio , S. Di Lorenzo , V. Dompè , A. Drobizhev , L. Dumoulin , G. Fantini , M. El Idrissi , M. Faverzani , E. Ferri , F. Ferri , F. Ferroni , E. Figueroa-Feliciano , J. Formaggio , A. Franceschi , S. Fu , B. K. Fujikawa , J. Gascon , S. Ghislandi , A. Giachero , M. Girola , L. Gironi , A. Giuliani , P. Gorla , C. Gotti , C. Grant , P. Gras , P. V. Guillaumon , T. D. Gutierrez , K. Han , E. V. Hansen , K. M. Heeger , D. L. Helis , H. Z. Huang , M. T. Hurst , L. Imbert , A. Juillard , G. Karapetrov , G. Keppel , H. Khalife , V. V. Kobychev , Yu. G. Kolomensky , R. Kowalski , H. Lattaud , M. Lefevre , M. Lisovenko , R. Liu , Y. Liu , P. Loaiza , L. Ma , F. Mancarella , N. Manenti , A. Mariani , L. Marini , S. Marnieros , M. Martinez , R. H. Maruyama , Ph. Mas , D. Mayer , G. Mazzitelli , E. Mazzola , Y. Mei , M. N. Moore , S. Morganti , T. Napolitano , M. Nastasi , J. Nikkel , C. Nones , E. B. Norman , V. Novosad , I. Nutini , T. O'Donnell , E. Olivieri , M. Olmi , B. T. Oregui , S. Pagan , M. Pageot , L. Pagnanini , D. Pasciuto , L. Pattavina , M. Pavan , Ò. Penek , H. Peng , G. Pessina , V. Pettinacci , C. Pira , S. Pirro , O. Pochon , D. V. Poda , T. Polakovic , O. G. Polischuk , E. G. Pottebaum , S. Pozzi , E. Previtali , A. Puiu , S. Puranam , S. Quitadamo , A. Rappoldi , G. L. Raselli , A. Ressa , R. Rizzoli , C. Rosenfeld , P. Rosier , M. Rossella , J. A. Scarpaci , B. Schmidt , R. Serino , A. Shaikina , K. Shang , V. Sharma , V. N. Shlegel , V. Singh , M. Sisti , P. Slocum , D. Speller , P. T. Surukuchi , L. Taffarello , S. Tomassini , C. Tomei , A. Torres , J. A. Torres , D. Tozzi , V. I. Tretyak , D. Trotta , M. Velazquez , K. J. Vetter , S. L. Wagaarachchi , G. Wang , L. Wang , R. Wang , B. Welliver , J. Wilson , K. Wilson , L. A. Winslow , F. Xie , M. Xue , J. Yang , V. Yefremenko , V. I. Umatov , M. M. Zarytskyy , T. Zhu , A. Zolotarova , S. Zucchelli

Access to lower temperatures has consistently enabled scientific breakthroughs. Pushing the limits of \emph{on-chip} temperatures deep into the microkelvin regime would open the door to unprecedented quantum coherence, novel quantum states…

BICEP1 is a millimeter-wavelength telescope designed specifically to measure the inflationary B-mode polarization of the Cosmic Microwave Background (CMB) at degree angular scales. We present results from an analysis of the data acquired…

The BICEP experiment was designed specifically to search for the signature of inflationary gravitational waves in the polarization of the cosmic microwave background (CMB). Using a novel small-aperture refractor and 49 pairs of…

A major goal of upcoming experiments measuring the Cosmic Microwave Background Radiation (CMBR) is to reveal the subtle signature of inflation in the polarization pattern which requires unprecedented sensitivity and control of systematics.…

Astrophysics · Physics 2019-08-13 Dorothea Samtleben

In this paper we present details of the construction of a wideband, cryogenic receiver and its successful commissioning on the Arecibo 12m telescope. The cryogenic receiver works in the 2.5-14 GHz frequency range. The telescope is operated…

Instrumentation and Methods for Astrophysics · Physics 2023-08-14 D. Anish Roshi , Phil Perillat , Felix Fernandez , Hamdi Mani , Benetge Perera , P. K. Manoharan , Luis Quintero , Arun Venkataraman

In this paper we present the design and measured performance of a novel cryogenic motor based on a superconducting magnetic bearing (SMB). The motor is tailored for use in millimeter-wave half-wave plate (HWP) polarimeters, where a HWP is…

Instrumentation and Methods for Astrophysics · Physics 2017-10-06 B. R. Johnson , F. Columbro , D. Araujo , M. Limon , B. Smiley , G. Jones , B. Reichborn-Kjennerud , A. Miller , S. Gupta

We present a measurement and analysis scheme for determining traceable thermodynamic temperature at cryogenic temperatures using Coulomb blockade thermometry. The uncertainty of the electrical measurement is improved by utilizing two…

The Q/U Imaging ExperimenT (QUIET) is designed to measure polarization in the Cosmic Microwave Background, targeting the imprint of inflationary gravitational waves at large angular scales (~ 1 degree). Between 2008 October and 2010…

Accurate on-chip temperature sensing is critical for the optimal performance of modern CMOS integrated circuits (ICs), to understand and monitor localized heating around the chip during operation. The development of quantum computers has…

The Atacama B-mode Search (ABS) experiment is a 145 GHz polarimeter designed to measure the B-mode polarization of the Cosmic Microwave Background (CMB) at large angular scales. The ABS instrument will ship to the Atacama Desert of Chile…

This paper presents the first experimental investigation and physical discussion of the cryogenic behavior of a commercial 28 nm bulk CMOS technology. Here we extract the fundamental physical parameters of this technology at 300, 77 and 4.2…

Mesoscale and Nanoscale Physics · Physics 2018-06-05 Arnout Beckers , Farzan Jazaeri , Andrea Ruffino , Claudio Bruschini , Andrea Baschirotto , Christian Enz

In-vacuo cryogenic environments are ideal for applications requiring both low temperatures and extremely low particle densities. This enables reaching long storage and coherence times for example in ion traps, essential requirements for…

We present a new method for measuring the CMB temperature quadrupole, using large scale CMB polarization. The method exploits the fact that CMB polarization is partially sourced by the local temperature quadrupole. We link the temperature…

Astrophysics · Physics 2007-05-23 Constantinos Skordis , Joseph Silk

Measurements of the 2.7 K cosmic microwave background (CMB) radiation now provide the most stringent constraints on cosmological models. The power spectra of the temperature anisotropies and the $E$-mode polarization of the CMB are…

Cosmology and Nongalactic Astrophysics · Physics 2010-07-01 Siddharth Savyasachi Malu , Peter T Timbie

We describe the design and expected performance of Clover, a new instrument designed to measure the B-mode polarization of the cosmic microwave background. The proposed instrument will comprise three independent telescopes operating at 90,…

The cosmic microwave background (CMB), a remnant of the Big Bang, provides unparalleled insights into the primordial universe, its energy content, and the origin of cosmic structures. The success of forthcoming terrestrial and space…

In this paper, we explore the power of the cosmic microwave background (CMB) polarization (E-mode) data to corroborate four potential anomalies in CMB temperature data: the lack of large angular-scale correlations, the alignment of the…

Measuring the faint polarization signal of the cosmic microwave background (CMB) not only requires high optical throughput and instrument sensitivity but also control over systematic effects. Polarimetric cameras or receivers used in this…

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