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.
Projectdetails
Introduction
The cosmic large-scale structure is entering a new ‘full space’ era with the launch of the Euclid galaxy survey satellite in 2023, coinciding with the first light for the Rubin Observatory. My proposal is centred on using galaxy surveys across a third of the sky as a laboratory for fundamental physics beyond the standard model by combining powerful theoretical models with exquisite data for galaxy clustering and weak gravitational lensing.
Objectives
To fully realise the potential of Euclid’s ‘full space’ galaxy survey, I will use my unique expertise in developing analytical, computational, and statistical methods to predict and analyse the cosmic large-scale structure beyond the average.
- I will hunt for fundamental physics by going beyond the average probed by standard two-point analyses.
- I will unlock additional information from novel clustering statistics sensitive to different density environments.
Methodology
I will provide new insights into dark matter dynamics and enable a field-based analysis by pioneering a particle-wave duality inspired phase-space technique that goes beyond the average effective fluid modelling. This will push forward modelling to a new level, overcome limitations of standard fluid and N-body methods, and enable the joint modelling of dark matter, baryons, and massive neutrinos.
Research Impact
My research program will unlock key insights into:
- Particle Physics: By pinning down the total neutrino mass and potential wavelike properties of dark matter.
- The Early Universe: By constraining primordial non-Gaussianity providing hints for inflationary physics.
- Gravity: By measuring the nature of dark energy and potential modifications of general relativity.
- Astrophysics: By determining the relationship between galaxies and dark matter.
Conclusion
My expertise in developing analytical, computational, and statistical methods for clustering dynamics and statistics, along with my leadership within the Euclid collaboration, places me in a strategic position to lead such an ambitious research program.
Financiële details & Tijdlijn
Financiële details
Subsidiebedrag | € 1.496.955 |
Totale projectbegroting | € 1.496.955 |
Tijdlijn
Startdatum | 1-3-2024 |
Einddatum | 28-2-2029 |
Subsidiejaar | 2024 |
Partners & Locaties
Projectpartners
- UNIVERSITAET BIELEFELDpenvoerder
Land(en)
Vergelijkbare projecten binnen European Research Council
Project | Regeling | Bedrag | Jaar | Actie |
---|---|---|---|---|
Gravitational Physics from the Universe Large Scales EvolutionThe project aims to develop a theoretical framework to interpret Euclid mission data, enhancing our understanding of gravity on cosmological scales and its potential deviations from General Relativity. | ERC Consolid... | € 1.999.219 | 2024 | Details |
Towards constraining the pillars of our cosmological model using combined probesThe 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. | ERC Starting... | € 1.634.640 | 2025 | Details |
A Cosmological Lever Arm for Fundamental PhysicsThe project aims to enhance measurements of the Universe's expansion rate and density fluctuations using 3D correlations in the Lyman forest, potentially advancing our understanding of neutrino masses and inflationary models. | ERC Consolid... | € 1.885.000 | 2022 | Details |
Science from the large scale cosmic microwave background polarization structureThe 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. | ERC Consolid... | € 1.998.750 | 2023 | Details |
Observational Cosmology Using Large Imaging SurveysOCULIS aims to enhance the understanding of dark matter and energy by leveraging Euclid satellite data to accurately measure galaxy properties and their relation to cosmic structure formation. | ERC Advanced... | € 2.457.977 | 2023 | Details |
Gravitational Physics from the Universe Large Scales Evolution
The project aims to develop a theoretical framework to interpret Euclid mission data, enhancing our understanding of gravity on cosmological scales and its potential deviations from General Relativity.
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.
A Cosmological Lever Arm for Fundamental Physics
The project aims to enhance measurements of the Universe's expansion rate and density fluctuations using 3D correlations in the Lyman forest, potentially advancing our understanding of neutrino masses and inflationary models.
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.
Observational Cosmology Using Large Imaging Surveys
OCULIS aims to enhance the understanding of dark matter and energy by leveraging Euclid satellite data to accurately measure galaxy properties and their relation to cosmic structure formation.