After the current Phase 3 of Cosmic Microwave Background (CMB) polarization measurements, aimed at the detection of the B-mode, there is a need of new experiments with higher sensitivity, better control of systematic effects, and the capability to separate polarized contaminants. Using the transfer matrix function method, we designed a novel experimental configuration, working as a nulling spectropolarimeter. This optical design has the capability to retrieve the spectral information of the sole linear polarization component of the incident radiation, rejecting unpolarized radiation. We present the optical design, its main features and an end-to-end forecast simulation about the absolute polarization angle measurement. This measurement is crucial for forthcoming experiments which aim to measure CMB B-mode.

Novel nulling spectropolarimeter design for polarization measurement of the cosmic microwave background / D'Alessandro, Giuseppe; de Bernardis, Paolo; Carbone, Aurora; Cataldi, Elisa; Coppolecchia, Alessandro; Masi, Silvia; Mele, Lorenzo; Micheli, Silvia; Kalemi, Benedetta; Piacentini, Francesco; Presta, Giuseppe. - (2022), p. 96. (Intervento presentato al convegno SPIE Astronomical Telescopes + Instrumentation, tenutosi a Montreal) [10.1117/12.2626789].

Novel nulling spectropolarimeter design for polarization measurement of the cosmic microwave background

D'Alessandro, Giuseppe
;
de Bernardis, Paolo;Carbone, Aurora;Cataldi, Elisa;Coppolecchia, Alessandro;Masi, Silvia;Mele, Lorenzo;Micheli, Silvia;Piacentini, Francesco;Presta, Giuseppe
2022

Abstract

After the current Phase 3 of Cosmic Microwave Background (CMB) polarization measurements, aimed at the detection of the B-mode, there is a need of new experiments with higher sensitivity, better control of systematic effects, and the capability to separate polarized contaminants. Using the transfer matrix function method, we designed a novel experimental configuration, working as a nulling spectropolarimeter. This optical design has the capability to retrieve the spectral information of the sole linear polarization component of the incident radiation, rejecting unpolarized radiation. We present the optical design, its main features and an end-to-end forecast simulation about the absolute polarization angle measurement. This measurement is crucial for forthcoming experiments which aim to measure CMB B-mode.
2022
SPIE Astronomical Telescopes + Instrumentation,
Instrumentation and Methods for Astrophysics, Spectrometers, Polarimeter, Cosmic microwave Background
04 Pubblicazione in atti di convegno::04b Atto di convegno in volume
Novel nulling spectropolarimeter design for polarization measurement of the cosmic microwave background / D'Alessandro, Giuseppe; de Bernardis, Paolo; Carbone, Aurora; Cataldi, Elisa; Coppolecchia, Alessandro; Masi, Silvia; Mele, Lorenzo; Micheli, Silvia; Kalemi, Benedetta; Piacentini, Francesco; Presta, Giuseppe. - (2022), p. 96. (Intervento presentato al convegno SPIE Astronomical Telescopes + Instrumentation, tenutosi a Montreal) [10.1117/12.2626789].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1655430
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