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The detection of B-modes in the CMB polarization pattern is a major issue in modern cosmology and must therefore be handled with analytical methods that produce reliable results. We describe a method that uses the frequency dependency of…

Investigating the polarization properties of light in the mid-infrared (mid-IR) spectrum is crucial for molecular sensing, biomedical diagnostics, and IR imaging system technologies. Traditional methods, limited by bulky size and intricate…

Cosmological Birefringence (CB), a rotation of the polarization plane of radiation coming to us from distant astrophysical sources, may reveal parity violation in either the electromagnetic or gravitational sectors of the fundamental…

宇宙学与河外天体物理 · 物理学 2013-05-30 Amit P. S. Yadav , Meir Shimon , Brian G. Keating

We discuss instrumental and analytic methods that have been developed for the first generation of bolometric cosmic microwave background (CMB) polarimeters. The design, characterization, and analysis of data obtained using Polarization…

We describe a novel method to measure the absolute orientation of the polarization plane of the CMB with arcsecond accuracy, enabling unprecedented measurements for cosmology and fundamental physics. Existing and planned CMB polarization…

天体物理仪器与方法 · 物理学 2017-05-26 Federico Nati , Mark J. Devlin , Martina Gerbino , Bradley R. Johnson , Brian Keating , Luca Pagano , Grant Teply

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…

天体物理学 · 物理学 2007-05-23 Constantinos Skordis , Joseph Silk

In this paper we describe QUBIC, an experiment that will observe the polarized microwave sky with a novel approach, which combines the sensitivity of state-of-the art bolometric detectors with the systematic effects control typical of…

天体物理仪器与方法 · 物理学 2019-01-24 Aniello Mennella , Peter Ade , Giorgio Amico , Didier Auguste , Jonathan Aumont , Stefano Banfi , Gustavo Barbaràn , Paola Battaglia , Elia Battistelli , Alessandro Baù , Benoit Bélier , David G. Bennett , Laurent Bergé , Jean Philippe Bernard , Marco Bersanelli , Marie Anne Bigot Sazy , Nathat Bleurvacq , Juan Bonaparte , Julien Bonis , Emory F. Bunn , David Burke , Daniele Buzi , Alessandro Buzzelli , Francesco Cavaliere , Pierre Chanial , Claude Chapron , Romain Charlassier , Fabio Columbro , Gabriele Coppi , Alessandro Coppolecchia , Rocco D'Agostino , Giuseppe D'Alessandro , Paolo De Bernardis , Giancarlo De Gasperis , Michele De Leo , Marco De Petris , Andres Di Donato , Louis Dumoulin , Alberto Etchegoyen , Adrián Fasciszewski , Cristian Franceschet , Martin Miguel Gamboa Lerena , Beatriz Garcia , Xavier Garrido , Michel Gaspard , Amanda Gault , Donnacha Gayer , Massimo Gervasi , Martin Giard , Yannick Giraud Héraud , Mariano Gómez Berisso , Manuel González , Marcin Gradziel , Laurent Grandsire , Eric Guerard , Jean Christophe Hamilton , Diego Harari , Vic Haynes , Sophie Henrot Versillé , Duc Thuong Hoang , Nicolas Holtzer , Federico Incardona , Eric Jules , Jean Kaplan , Andrei Korotkov , Christian Kristukat , Luca Lamagna , Soutiris Loucatos , Amy Lowitz , Vladimir Lukovic , Louis Thibault , Raùl Horacio Luterstein , Bruno Maffei , Stefanos Marnieros , Silvia Masi , Angelo Mattei , Andrew May , Mark McCulloch , Maria C. Medina , Lorenzo Mele , Simon J. Melhuish , Ludovic Montier , Louise Mousset , Luis Mariano Mundo , John Anthony Murphy , James Murphy , Creidhe O'Sullivan , Emiliano Olivieri , Alessandro Paiella , Francois Pajot , Andrea Passerini , Hernan Pastoriza , Alessandro Pelosi , Camille Perbost , Maurizio Perciballi , Federico Pezzotta , Francesco Piacentini , Michel Piat , Lucio Piccirillo , Giampaolo Pisano , Gianluca Polenta , Damien Prêle , Roberto Puddu , Damien Rambaud , Pablo Ringegni , Gustavo E. Romero , Maria Salatino , Alessandro Schillaci , Claudia G. Scóccola , Stephen P. Scully , Sebastiano Spinelli , Michail Stolpovskiy , Federico Suarez , Guillaume Stankowiak , Andrea Tartari , Jean Pierre Thermeau , Peter Timbie , Maurizio Tomasi , Steve A. Torchinsky , Mathieu Tristram , Gregory S. Tucker , Carole E. Tucker , Sylvain Vanneste , Daniele Viganò , Nicola Vittorio , Fabrice Voisin , Robert Watson , Francois Wicek , Mario Zannoni , Antonio Zullo

The cosmic microwave background polarization is rich of cosmological information complementary to those from temperature anisotropies. Linear polarization can be decomposed uniquely in two components of opposite parities, called E and B.…

天体物理学 · 物理学 2007-05-23 C. Rosset , the PLANCK-HFI Collaboration

The quasi-optical modulation of linear polarization at millimeter and sub-millimeter wavelengths can be achieved by using rotating half wave plates (HWPs) in front of polarization sensitive detectors. Large operational bandwidths are…

The polarization of light conveys unique information that can be exploited by crucial applications. The bulky and costly discrete optical components used in conventional polarimeters limit their broad adoption. A compact, low-cost…

应用物理 · 物理学 2019-03-27 Zhongjin Lin , Leslie Rusch , Yuxuan Chen , Wei Shi

The B-mode detection of Cosmic Microwave Background polarization will require new technological developments, able to get sensitivities at least 2 orders of magnitude better than for the E-mode. This really ambitious goal cannot be reached…

天体物理学 · 物理学 2007-05-23 S. Cortiglioni , E. Carretti

We present an approach to classical polarimetry that requires no moving parts, is compact and robust, and that encodes the complete polarization information on a single data frame, accomplished by replacing the rotation of components such…

天体物理仪器与方法 · 物理学 2019-05-29 William B. Sparks , Thomas A. Germer , Rebecca M. Sparks

CMB (Cosmic Microwave Background) polarization observations test many aspects of cosmological models. Effective pseudoscalar-photon interaction(s) would induce a rotation of linear polarization of electromagnetic wave propagating with…

宇宙学与河外天体物理 · 物理学 2009-08-20 Wei-Tou Ni

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…

We have simulated the interferometric observation of the Cosmic Microwave Background (CMB) temperature and polarization fluctuations. We have constructed data pipelines from the time-ordered raw visibility samples to the CMB power spectra…

天体物理学 · 物理学 2009-11-07 Chan-Gyung Park , Kin-Wang Ng , Changbom Park , Guo-Chin Liu , Keiichi Umetsu

The B-mode polarisation power spectrum in the Cosmic Microwave Background (CMB) is about four orders of magnitude fainter than the CMB temperature power spectrum. Any instrumental imperfections that couple temperature fluctuations to B-mode…

宇宙学与河外天体物理 · 物理学 2017-01-18 Christopher G. R. Wallis , Michael L. Brown , Richard A. Battye , Jacques Delabrouille

This work aims to demonstrate that two arrays of Lumped Element Kinetic Inductance Detectors (LEKIDs), when employed in filled array configuration and separated by an external linear polarizer oriented at 45 degrees, can achieve the…

We show that it is possible to measure polarization with a polarimeter that gets rid of the seeing while still measuring at a frequency well below that of the seeing. We study a standard polarimeter made of two retarders and a beamsplitter.…

天体物理仪器与方法 · 物理学 2016-04-20 A. Asensio Ramos

With the forthcoming release of high precision polarization measurements, such as from the Planck satellite, the metrology of polarization needs to improve. In particular, it is crucial to take into account full knowledge of the noise…

天体物理仪器与方法 · 物理学 2015-02-11 L. Montier , S. Plaszczynski , F. Levrier , M. Tristram , D. Alina , I. Ristorcelli , J. -P. Bernard

The Primordial Inflation Explorer (PIXIE) is an Explorer-class mission concept to measure the energy spectrum and linear polarization of the cosmic microwave background (CMB). A single cryogenic Fourier transform spectrometer compares the…