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Astrophysical Frontiers in Feebly Interacting Particle Searches: Multi-Wavelength Analyses and Predictive Strategies for Next-Generation Observations

Project description

Expanding our understanding of light new particles with astrophysical observations

The Standard Model (SM) of particle physics has advanced remarkably, but phenomena like neutrino masses and dark matter remain unexplained. Extensions of the SM, such as Beyond the Standard Model (BSM) theories, incorporate feebly interacting particles (FIPs), including axions and dark photons. This enhances our understanding of phenomena that might leave detectable imprints in astrophysical environments, even if they cannot be observed in the lab. Supported by the Marie Skłodowska-Curie Actions programme, the ASTROFIP project will develop a framework that combines stellar population synthesis with detailed stellar evolution models and conduct multi-wavelength searches for FIP signatures. Overall, the project’s goal is to expand our exploration and understanding of FIPs.

Objective

The Standard Model (SM) of particle physics, despite its remarkable successes, cannot explain several key phenomena, including for instance neutrino masses and dark matter. A compelling class of extensions of the SM (BSM) involves Feebly Interacting Particles (FIPs) - such as axions, axion-like particles, dark photons, and sterile neutrinos - whose extremely weak couplings evade laboratory detection but may leave imprints in astrophysical environments. Ordinary stars, supernovae, and galaxies act as natural laboratories where FIPs can be produced, potentially generating observable multi-wavelength signals.
This project aims to advance the exploration of BSM particles through a novel, interdisciplinary strategy. First, I will develop a systematic framework combining stellar population synthesis with detailed stellar evolution models to reduce astrophysical uncertainties in FIP production. Second, I will perform targeted multi-wavelength searches for FIP signatures in archival datasets, from radio to X-ray and gamma-ray observations of star-forming galaxies and the Galactic center. Stacked analyses across diverse environments will provide robust constraints while improving astrophysical background modeling. Third, I will deliver realistic predictions and observational strategies for next-generation missions, which aim to enhance sensitivity to FIP-induced signals.
By integrating astrophysical modeling with particle physics phenomenology, this project will strengthen synergies between astrophysics and particle physics and will deliver the most stringent constraints on FIPs to date, based on multi-wavelength observations, while directly informing the design and strategy of upcoming observatories.

Fields of science (EuroSciVoc)

Keywords

Programme(s)

Topic(s)

Funding Scheme

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

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Call for proposal

(opens in new window) HORIZON-MSCA-2025-PF

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Coordinator

CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS
Net EU contribution
€ 226 420,56
Address
RUE MICHEL ANGE 3
75794 Paris
France
Region
Ile-de-France Ile-de-France Paris
Activity type
Research Organisations
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Total cost
No data