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EFficient search FOR primordial feaTureS in current and future cosmological data

Project description

Detecting primordial features in cosmic data

Primordial features (PFs) are scale-dependent deviations (often oscillations) in the standard spectra of primordial density perturbations. They arise from disturbances in early-universe models and may reveal new energy scales and properties of the inflaton field. Supported by the Marie Skłodowska-Curie Actions programme, the EFFORTS project will enhance the search for PFs using current and future cosmological data. It will evaluate PF models with the latest Cosmic Microwave Background and Large Scale Structure observations, focusing on both the power spectrum and bispectrum. The project will also develop an efficient code and pipeline to detect these signals in data from the upcoming LISA experiment.

Objective

Primordial features (PFs) are scale-dependent deviations from the leading-order, scale-invariant spectra of primordial density perturbations, often manifesting as oscillations. These PFs arise from disturbances in the potential or internal space of primordial Universe models, which alter the background evolution from the leading trajectory. While the amplitudes of these features are uncertain, their presence is likely, and detecting them would offer insights into the physics of the primordial Universe, such as new energy scales and heavier degrees of freedom coupled to the inflaton field. This proposal aims to maximize the efficiency of the search for PFs in current and future cosmological data. I will test PF models against the most recent Cosmic Microwave Background and Large Scale Structure data for the first time using both the power spectrum and bispectrum of primordial fluctuations. At smaller scales, PF signals must be much larger to be detected through the Stochastic Gravitational Wave Background (SGWB) sourced by large scalar fluctuations. Focusing on the future LISA experiment, I will build an efficient code and pipeline to detect these signals in future data. On the theoretical side, I will also explore the contribution of loop corrections in these models, which may dominate over tree-level results, and design novel non-perturbative techniques to compute the spectra in these cases. This project will set the state of the art for analyzing PFs of any amplitude and at any cosmological scales.

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Topic(s)

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Funding Scheme

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HORIZON-TMA-MSCA-PF-EF - HORIZON TMA MSCA Postdoctoral Fellowships - European Fellowships

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Call for proposal

Procedure for inviting applicants to submit project proposals, with the aim of receiving EU funding.

(opens in new window) HORIZON-MSCA-2024-PF-01

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Coordinator

ORGANISATION EUROPEENNE POUR LA RECHERCHE NUCLEAIRE
Net EU contribution

Net EU financial contribution. The sum of money that the participant receives, deducted by the EU contribution to its linked third party. It considers the distribution of the EU financial contribution between direct beneficiaries of the project and other types of participants, like third-party participants.

€ 292 118,88
Address
ESPLANADE DES PARTICULES 1 PARCELLE 11482 DE MEYRIN BATIMENT CADASTRAL 1046
1211 GENEVE 23
Switzerland

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Region
Schweiz/Suisse/Svizzera Région lémanique Genève
Activity type
Research Organisations
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Total cost

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