학술논문
Measuring the CMB primordial B-modes with Bolometric Interferometry
Document Type
article
Author
Mennella A.; Ade P.; Almela A.; Amico G.; Arnaldi L.H.; Aumont J.; Banfi S.; Battistelli E.S.; Bélier B.; Bergé L.; Bernard J.-Ph.; Bersanelli M.; Bonaparte J.; Bonilla J.D.; Bunn E.; Buzi D.; Cacciotti F.; Camilieri D.; Cavaliere F.; Chanial P.; Chapron C.; Colombo L.; Columbro F.; Coppolecchia A.; Costanza M.B.; D’Alessandro G.; de Bernardis P.; De Gasperis G.; De Leo M.; De Petris M.; Del Castillo N.; Dheilly S.; Etchegoyen A.; Ferazzoli S.; Ferreyro L.P.; Franceschet C.; Lerena M.M. Gamboa; Ganga K.; García B.; Redondo M.E. García; Gayer D.; Geria J.M.; Gervasi M.; Giard M.; Gilles V.; Berisso M. Gómez; Gonzalez M.; Gradziel M.; Grandsire L.; Hamilton J.-Ch.; Hampel M.R.; Isopi G.; Kaplan J.; Lamagna L.; Lazarte F.; Loucatos S.; Maffei B.; Mancilla A.; Mandelli S.; Manzan E.; Marchitelli E.; Marnieros S.; Marty W.; Masi S.; May A.; Maya J.; McCulloch M.; Mele L.; Melo D.; Mirón-Granese N.; Montier L.; Mousset L.; Müller N.; Nati F.; O’Sullivan C.; Paiella A.; Pajot F.; Paradiso S.; Pascale E.; Passerini A.; Pelosi A.; Perciballi M.; Pezzotta F.; Piacentini F.; Piat M.; Piccirillo L.; Pisano G.; Platino M.; Polenta G.; Prêle D.; Rambaud D.; Ramos G.; Rasztocky E.; Régnier M.; Reyes C.; Rodríguez F.; Rodríguez C.A.; Romero G.E.; Salum J.M.; Schillaci A.; Scóccola C.; Stankowiak G.; Tartari A.; Thermeau J.-P.; Timbie P.; Tomasi M.; Torchinsky S.; Tucker G.; Tucker C.; Vacher L.; Voisin F.; Wright M.; Zannoni M.; Zullo A.
Source
EPJ Web of Conferences, Vol 293, p 00030 (2024)
Subject
Language
English
ISSN
2100-014X
Abstract
The Q&U Bolometric Interferometer for Cosmology (QL’BIC) is the first bolometric interferometer designed to measure the primordial B-mode polarization of the Cosmic Microwave Background (CMB). Bolometric interferometry is a novel technique that combines the sensitivity of bolometric detectors with the control of systematic effects that is typical of interferometry, both key features in the quest for the faint signal of the primordial B-modes. A unique feature is the so-called “spectral imaging”, i.e., the ability to recover the sky signal in several sub-bands within the physical band during data analysis. This feature provides an in-band spectral resolution of ∆v/v ~ 0.04 that is unattainable by a traditional imager. This is a key tool for controlling the Galactic foregrounds contamination. In this paper, we describe the principles of bolometric interferometry, the current status of the QU BIC experiment and future prospects.