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Exploring the Cosmos with the Vera Rubin Observatory

Descripción del proyecto

Nuevos conocimientos físicos de las estructuras a gran escala del Universo

El Observatorio Vera C. Rubin es un enorme telescopio que observará el Universo con un detalle sin precedentes. Los catálogos resultantes contendrán datos de miles de millones de galaxias y otros objetos exóticos, como las contrapartes electromagnéticas de las fuentes de ondas gravitatorias. El objetivo del proyecto CosmicExplorer, financiado con fondos europeos, es obtener nuevos conocimientos físicos de estos catálogos y abordará tres retos principales: reducir el tiempo de cálculo para modelizar con precisión estos datos complejos; dilucidar señales sutiles de errores sistemáticos (posiblemente desconocidos); y desarrollar nuevas sondas de la estructura a gran escala del Universo. El equipo de CosmicExplorer combinará técnicas avanzadas de emulación de datos, métodos de inteligencia artificial y modelos bayesianos jerárquicos para lograr un gran avance en la comprensión de la cosmología física.

Objetivo

The standard model of cosmology postulates ingredients that are not present in the standard model of particle physics – dark matter, dark energy, and a primordial origin for cosmic structure. Their physical nature remains a mystery. In the past few years, it has become clear that formidable modelling and data analysis challenges stand in the way of establishing how these ingredients fit into fundamental physics.

Starting in 2023, we have an opportunity to uncover the physical underpinning of the cosmological model, using a new window on the universe opened by the Vera C. Rubin Observatory’s Legacy Survey of Space and Time (LSST). Just in its first year, LSST will see more of the universe than all previous surveys combined. By repeatedly mapping huge sky areas, it will create the first motion picture of our universe. The resulting catalogues will contain billions of galaxies and other, more exotic objects such as the electromagnetic counterparts of gravitational wave sources.

This project aims to turn these catalogues into physical insight by solving three pressing challenges: (1) the formidable computational expense of accurately modelling this complex data; (2) the need to tease out subtle signals from (possibly unknown) systematics; (3) capturing the rich information in the “cosmic web” of galaxies tracing the large-scale structure of the universe, inaccessible by standard analysis methods. I will achieve these aims through a unique approach, combining innovative data emulation techniques to accelerate forward-modelling, a ground-breaking ‘explainable artificial intelligence’ approach to scientific discovery, and advanced hierarchical Bayesian methods to achieve not just precision (small error-bars) but accuracy (unbiased results). The combination of the unique tools I will develop, and LSST’s new view of the universe, opens up a vast discovery space. I will explore this space with the aim of achieving a breakthrough in our understanding of physical cosmology.

Régimen de financiación

ERC-ADG - Advanced Grant

Institución de acogida

THE CHANCELLOR MASTERS AND SCHOLARS OF THE UNIVERSITY OF CAMBRIDGE
Aportación neta de la UEn
€ 1 296 935,00
Dirección
TRINITY LANE THE OLD SCHOOLS
CB2 1TN Cambridge
Reino Unido

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Región
East of England East Anglia Cambridgeshire CC
Tipo de actividad
Higher or Secondary Education Establishments
Enlaces
Coste total
€ 1 296 935,00

Beneficiarios (2)