Science from the large scale cosmic microwave background polarization structure
The project aims to enhance observational cosmology by developing advanced models and algorithms to accurately measure cosmic microwave background polarization, focusing on primordial B-modes to revolutionize our understanding of the early Universe.
Projectdetails
Introduction
Observational cosmology is moving towards its next major milestone: high-precision measurements of the cosmic microwave background polarization with the goal of detecting and characterizing the primordial B-modes. These polarization patterns would provide a unique picture of the early Universe, shedding light on the conditions at that time, be it cosmic inflation, gauge fields, or more exotic possibilities.
Impact of Observations
In a regime of energy where standard models are expected to break, such observations could revolutionize our current picture of cosmology and high energy physics. Characterizing such signals requires:
- Reaching extremely low instrumental sensitivity levels.
- Controlling instrumental and astrophysical systematic effects with unprecedented fidelity.
While (1) is about to be reached with the planned deployment of funded, cutting-edge observatories such as the Simons Array/Observatory, CMB-S4, and LiteBIRD, (2) is already limiting the current constraints and will be studied and uniquely mitigated by SciPol.
Project Goals
My project is an opportunity to claim a leadership role for Europe in one of the most active and impactful research areas in physics, complementing the hardware efforts led by the US and Japan. I will:
- Construct accurate, open-source, and versatile models for the instrumental, astrophysical signals, and noise properties.
- Develop and exploit new, general algorithms adjusting previous models from observations, and producing a unique set of instrument- and foreground-corrected maps.
- Make a statistically robust cosmological inference of these, especially on the large scale, implementing a gravitational lensing correction.
Experience and Positioning
I have been at the forefront of this research for the last 10 years, made key contributions to the analysis and scientific exploitation of the POLARBEAR data sets, and to preparations and scientific optimization of the forthcoming efforts. I am consequently uniquely positioned to deliver the objectives of the proposed work.
Financiële details & Tijdlijn
Financiële details
Subsidiebedrag | € 1.998.750 |
Totale projectbegroting | € 1.998.750 |
Tijdlijn
Startdatum | 1-1-2023 |
Einddatum | 31-12-2027 |
Subsidiejaar | 2023 |
Partners & Locaties
Projectpartners
- CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRSpenvoerder
Land(en)
Vergelijkbare projecten binnen European Research Council
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POLarization Orientation CALibrator for Cosmology
The project aims to enhance CMB polarization measurements using aerial drones for calibration, improving accuracy in detecting gravitational waves and cosmic phenomena.
Towards constraining the pillars of our cosmological model using combined probes
The PiCo project aims to refine the ΛCDM cosmological model by employing advanced statistical methods to analyze galaxy clustering and CMB data, addressing primordial fluctuations and cosmic acceleration.
Probing cosmic large-scale structure beyond the average
This project aims to explore fundamental physics beyond the standard model using the Euclid galaxy survey and advanced statistical methods to analyze cosmic structures and dark matter dynamics.
Massively parallel joint end-to-end Bayesian analysis of past, present, and future CMB experiments
Develop a massively parallel framework for joint analysis of CMB data to enhance sensitivity, control systematics, and potentially detect primordial gravitational waves, transforming computational cosmology.
Cosmic Inflation and Structure Formation Through Global Analysis
The Origins project aims to create a unified model of diffuse astrophysical emissions using advanced data analysis, enhancing our understanding of cosmic origins and improving measurements of gravitational waves and dust emissions.