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Advanced Methodologies for Next Generation Large Scale CMB Polarization Analysis

Project description

DEENESFRITPL

Searching for the needle in our primordial haystack

‘Inflation’ refers to the postulated rapid expansion of the universe after the Big Bang. Cosmic microwave background (CMB) radiation is the remnant of the first light able to travel freely through the universe; it was released soon after the Big Bang and is thus the earliest observable. Gravitational waves would have left their signatures on the CMB in the form of tiny specific anisotropies in CMB polarisation called B-modes, but these are yet to be detected. With the support of the Marie Skłodowska-Curie Actions programme, the CMB-INFLATE project is targeting data analysis and modelling innovations leading to the identification of the mechanism behind cosmic inflation with future experiments at large angular scales.

Objective

The cosmic microwave background (CMB) radiation was emitted when the Universe was 380,000 years old and is observed today at 2.7 K. It is a wonderful probe to study the evolution of the Universe. Tiny anisotropies in its temperature and polarization are induced by quantum scalar (density) and tensor fluctuations (gravitational waves, GW) generated during inflation, a period of accelerated expansion arising 10-35 s after the big bang. Primordial GW imprinted a unique parity-odd pattern on CMB polarization, called B-modes. Such modes, undetected as of today, are a direct probe of the poorly known physics of inflation, and main target of several forthcoming observational projects. These will be search for B-modes at large (> 10°) and intermediate (~1°) angular scales. Among such efforts, Japan is proposing a satellite project (LiteBIRD, to be launched end 20's) with contributions from EU agencies, NASA and CSA. Large angular scales are difficult to measure due to Galactic emissions and instrumental systematics, requiring careful, detailed modelling and advanced data analysis techniques. EU scientists rely on the legacy of the ESA Planck mission (2009), but improvements of analysis methods and modelling of the instruments are now required. The main goal of CMB-INFLATE is to build a community of scientists dedicated to the development of innovative analysis of large angular scale CMB polarisation data to identify the inflation mechanism. CMB-INFLATE will focus on: (1) modelling hardware developed in three continents, including polarization modulators, optical systems, and detectors; (2) the development and implementation of innovative techniques to mitigate systematics from the sky and the instrument. Such advancements will be provided by a wide-scale international consortium involving instrumentalists, data analysis experts and theoreticians. The CMB-INFLATE outcome is expected to strengthen European leadership in the field of primordial GW and connected science.

Fields of science

Programme(s)

Topic(s)

Call for proposal

H2020-MSCA-RISE-2020

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Funding Scheme

MSCA-RISE - Marie Skłodowska-Curie Research and Innovation Staff Exchange (RISE)

Coordinator

UNIVERSITE PARIS CITE
Net EU contribution
€ 285 200,00
Address
85 bd saint germain
75006 Paris
France

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Region
Ile-de-France Ile-de-France Paris
Activity type
Higher or Secondary Education Establishments
Links
Other funding
€ 115 000,00

Participants (8)

Partners (7)

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Last update: 22 January 2023

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Permalink: https://cordis.europa.eu/project/id/101007633

European Union, 2023