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.
Significance of the Research
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.
Challenges in Characterization
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 Objectives
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.
Personal Background
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)
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