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New Technologies for Next-Generation Gravitational-Wave Detectors

Project description

Gravitational-wave astronomy deepens insight into the universe

More than a decade since the first gravitational-wave detection, this new field of astronomy has changed how we perceive the cosmos. Detectors have identified hundreds of cosmic collisions and have revealed secrets about black holes, neutron stars, and the universe’s expansion. Next-generation observatories promise even deeper insights by capturing thousands more events with greater precision. Supported by the Marie Skłodowska-Curie Actions programme, the GRAVITY project will develop new technologies to improve detector sensitivity and data analysis, sharing innovations in optics and quantum technology. Overall, the project aims to promote education and inspire new generations to explore the mysteries of gravitational waves and the universe.

Objective

Since the first detection of gravitational waves in 2015 and the multi-messenger observation of a binary neutron star merger in 2017, gravitational-wave (GW) astronomy has advanced rapidly, delivering groundbreaking discoveries in astrophysics, cosmology, and fundamental physics. The international GW network—LIGO, Virgo, and KAGRA—has detected over 200 sources, with ongoing upgrades to enhance sensitivity and astrophysical reach.
Future next-generation observatories, including the Einstein Telescope in Europe and Cosmic Explorer in the U.S. are set to begin operations beyond 2035. The Einstein Telescope will detect hundreds of thousands of compact-object mergers up to redshifts of a few tens, enabling precise measurements of the Hubble constant (H₀) and dark energy parameters, searches for dark matter candidates, new GW sources like spinning neutron stars and supernovae, and detailed mapping of compact-object mass distributions. Multi-messenger observations will further enrich our understanding of the universe.
The GRAVITY project fosters international collaborations on key experimental advancements for future detectors, including cryogenic techniques for thermal noise reduction, quantum noise suppression, and fused-silica-based suspensions. It will also focus on detector characterization, glitch identification, advanced data-analysis algorithms, and interdisciplinary data interpretation.
A crucial aspect is the transfer of knowledge to private companies, driving innovation in precision optics, quantum technologies, and advanced materials. These collaborations will enhance detector performance and create broader technological applications, benefiting both science and industry.
Gravitational-wave science, bridging classical physics, general relativity, and quantum mechanics, is also a powerful tool for outreach and education. Alongside cutting-edge research, GRAVITY will engage in educational initiatives and public outreach to inspire future generations.

Fields of science (EuroSciVoc)

Programme(s)

Topic(s)

Funding Scheme

HORIZON-TMA-MSCA-SE - HORIZON TMA MSCA Staff Exchanges

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Call for proposal

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

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Coordinator

UNIVERSITA DEGLI STUDI DI PERUGIA
Net EU contribution
€ 70 140,00
Address
PIAZZA DELL UNIVERSITA 1
06123 Perugia
Italy
Region
Centro (IT) Umbria Perugia
Activity type
Higher or Secondary Education Establishments
Links
Total cost
No data

Participants (10)

Partners (4)