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Red teaming the H0 Tension

Project description

Profiling the source of the Hubble tension

The standard model is the best description to date of the particle universe, despite known limitations. Recently, observations from large sky surveys and distance measurements with a variety of advanced cosmological probes have pointed to ‘tensions’ – differences in certain measurements predicted to be equal. The most important is the expansion rate of the universe, quantified by the Hubble parameter, H0. Early-universe standard model predictions are different from ‘late-universe’ direct measurements. The ERC-funded RedH0T project aims to determine whether the inconsistency arises from observational issues or limitations in the current model by systematically combining data from all available cosmological probes. Inconsistencies in the model would reshape understanding of the nature of the universe.

Objective

Despite the spectacular success of the standard cosmological model over the past two decades, recent observations from large sky surveys and distance measurements with a broad range of cosmological probes suggest cracks to the accepted paradigm: differences now appear in measurements of quantities the current cosmological model predicts as equal. These are called “tensions”. The most important tension concerns the Hubble parameter, H0, which quantifies the expansion rate of the Universe now, some 13 billion years after Big-Bang. The Hubble tension is the discrepancy between the value of H0, when inferred as a global parameter of the standard cosmological model relying heavily on early-Universe physics, and when measured directly in the late-time Universe from the redshift-to-distance relation. While the tension is well-established, there is no consensus on its actual significance nor on what it means for the standard cosmological model, even broadly speaking. Comparing the values of H0 from the early and the late Universe is like “Threading a needle from the other side of the Universe”; in a very unique way it enables vital end-to-end tests of cosmology to be performed.

RedH0T proposes to determine, in a self-consistent manner and using the synergies between all available cosmological probes, whether the tension arises from observational issues or from limitations in the current cosmological model. In the former case, we will impose strong limits of possible deviations from the standard cosmological. But if the latter is confirmed, it will represent one of the most significant discoveries of the 21st century, with profound implications not only for cosmology, but also for physics in general. The team gathers all required expertise to tackle the problem from all view-angles, addressing in a self-critical and constructive way all theoretical and observational aspects simultaneously.

Fields of science (EuroSciVoc)

Keywords

Programme(s)

Topic(s)

Funding Scheme

HORIZON-ERC-SYG - HORIZON ERC Synergy Grants

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Call for proposal

(opens in new window) ERC-2025-SyG

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Host institution

UNIVERSITAT DE BARCELONA
Net EU contribution
€ 6 454 299,00
Address
GRAN VIA DE LES CORTS CATALANES 585
08007 Barcelona
Spain
Region
Este Cataluña Barcelona
Activity type
Higher or Secondary Education Establishments
Links
Total cost
€ 6 454 299,00

Beneficiaries (5)