Skip to main content
Go to the home page of the European Commission (opens in new window)
English en
CORDIS - EU research results
CORDIS

Ultralight Dark Matter Detection and Characterization with LISA

Project description

Tracking dark matter through gravitational waves

Dark matter continues to be one of the most intriguing puzzles in the universe. Despite strong evidence about its existence, we are still in the dark as to what dark matter truly is. Supported by the Marie Skłodowska-Curie Actions programme, the ULDM-GW project seeks to reveal these cosmic secrets by catching dark matter waves with the Laser Interferometer Space Antenna (LISA). These waves interact with the elements of the interferometer and look like continuous, slow gravitational waves with a frequency inaccessible to Earth-based instruments. By studying the different polarisations of these waves, the team develops search algorithms that will enable us to differentiate between dark matter candidates and true gravitational waves from astrophysical objects.

Objective

Despite compelling astrophysical and cosmological evidence for dark matter, its nature remains unknown. Ultralight dark matter (ULDM) is a well-motivated candidate, producing distinctive signatures that can be probed with gravitational wave (GW) interferometers. Spin-0, spin-1, and spin-2 ULDM couple differently to Standard Model particles, inducing measurable effects in GW detectors, but distinguishing between ULDM spins, and between ULDM and continuous astrophysical GWs, is challenging due to signal similarities. This project will exploit LISA’s low-frequency band and orbital configuration to detect ULDM in a frequency band unexplored by ground-based detectors and discriminate signal types through their characteristic polarization content. By combining theoretical modeling of ULDM signals with dedicated search strategies, we will develop the first end-to-end LISA pipeline capable of both detecting ULDM and constraining signal type. The project will be carried out in CEICO-FZU (host) and L2IT-CNRS (secondment), with strong expertise in ULDM and LISA science respectively. We will establish waveform templates and signal characteristics in both time and frequency domains, develop a semi-coherent search and a fully coherent search for ULDM in LISA, and will forecast how effectively polarization measurements can distinguish between spin-0, spin-1, and spin-2 ULDM, and continuous astrophysical GWs. This approach will deliver the highest sensitivity to ULDM across LISA’s frequency range, surpassing existing experimental limits by orders of magnitude, while providing a robust framework to differentiate candidate signals. The outcome will advance both fundamental dark matter searches and GW data analysis, establishing LISA as a powerful probe of the dark sector.

Fields of science (EuroSciVoc)

Keywords

Programme(s)

Topic(s)

Funding Scheme

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

See all projects funded under this funding scheme

Call for proposal

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

See all projects funded under this call

Coordinator

FYZIKALNI USTAV AV CR, VVI
Net EU contribution
€ 191 918,16
Address
NA SLOVANCE 1999/2
182 00 PRAHA 8
Czechia
Region
Česko Praha Hlavní město Praha
Activity type
Higher or Secondary Education Establishments
Links
Total cost
No data

Partners (1)