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Cosmic Inflation and Structure Formation Through Global Analysis

During the last decades, high-precision experiments have made increasingly detailed measurements of diffuse Extragalactic Background Light (EBL) emitted by cosmological sources. This has revolutionized the understanding of our cos... ver más

31/12/2029

Innovasjon Norge

1M€

Presupuesto del proyecto: 1M€

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Innovasjon Norge No se ha especificado una descripción o un objeto social para esta compañía.

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Financiación concedida El organismo HORIZON EUROPE notifico la concesión del proyecto el día 2024-10-16

ERC-2024-STG: ERC STARTING GRANTS Scope:Objectives

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Innovasjon Norge

1.50M€ | Lider

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Duración del proyecto: 62 meses Fecha Inicio: 2024-10-16
Fecha Fin: 2029-12-31

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Innovasjon Norge No se ha especificado una descripción o un objeto social para esta compañía.

Presupuesto del proyecto 1M€

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Descripción del proyecto During the last decades, high-precision experiments have made increasingly detailed measurements of diffuse Extragalactic Background Light (EBL) emitted by cosmological sources. This has revolutionized the understanding of our cosmic origins. The Cosmic Microwave Background (CMB) is our most precious resource for understanding the Big Bang, while the Cosmic Infrared and Optical Backgrounds (CIB and COB) provide unique constraints on the evolution of large scale structure from the first galaxies to today. Until recently, measurements of these effects were limited by either foregrounds or instrumental noise. However, the combined signal-to-noise ratio has now grown so large that the interplay between astrophysical confusion and instrumental systematic uncertainties dominate the error budget. To make further process, it has become critical to account for all sources of uncertainties simultaneously. In the Origins project, I will solve this challenge through joint integrated end-to-end analysis of multiple state- of-the-art experiments to construct a single coherent model of all main diffuse astrophysical emission processes from 1 um to 23 GHz. In a novel approach, Origins will utilize archival observations from ACT, AKARI, COBE/DIRBE, COBE/FIRAS, IRAS, Planck, and WMAP, many in the form of raw time- ordered data, with upcoming measurements from Simons Observatory and SPHEREx. This will result in the world’s strongest and most robust constraints on primordial inflationary gravitational waves; the most accurate map of CIB fluctuations published to date; and possibly the world’s first map of large-scale COB fluctuations. Simultaneously, it will redefine our understanding of thermal dust emission in the Milky Way spanning a wide range of the electromagnetic spectrum, and will improve the precision of current models of Zodiacal Light by several orders of magnitude. This Open Science project will define a new paradigm for next-generation CMB B-mode and EBL experiments.

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