A Global Network for the Search for High Frequency Gravitational Waves
GravNet aims to develop a networked experimental platform to detect high-frequency gravitational waves, enhancing sensitivity and opening new avenues for astrophysical research.
Projectdetails
Introduction
The overarching goal of the GravNet project is to develop, test, and deploy a novel experimental platform that could enable the first detection of gravitational waves (GWs) in the frequency range of MHz to GHz. This would provide a new and unique window into astrophysical processes that have so far eluded observation.
Background
The first detection of gravitational waves by LIGO in 2015 ushered in a new era of fundamental physics. Since then, a network of ground-based GW interferometers has probed the frequency range from 10 Hz to 10 kHz, detecting nearly a hundred mergers of black-hole and neutron-star binaries.
In 2023, a signal at much lower frequency, in the nHz band, was detected by timing radio signals from pulsars. The race is now on to explore other bands. Of particular interest in this context is access to the MHz-GHz range, as signals may be generated copiously by events such as:
- Primordial-black-hole mergers
- The dynamics of ultra-light dark matter overdensities
- Violent phenomena in primordial cosmological times
These processes are related to some of the most pressing open questions about our Universe.
Methodology
The use of cavities in strong magnetic fields has been identified as one of the most promising techniques to search for high-frequency gravitational waves. So far, efforts have focused on cavities with small volumes that are tuned to search for axion-like particles.
By contrast, the GravNet scheme is based on combining different technologies and methodological approaches to measure synchronously cavity signals from multiple devices in magnetic fields operated as a network across Europe. This approach increases the sensitivity to high-frequency GWs (HFGWs) by several orders of magnitude compared to current methods.
Conclusion
In this way, GravNet will open up a new, vast parameter space for gravitational-wave searches and might be the enabling step towards the first detection of HFGWs, with the potential to revolutionize our understanding of the Universe.
Financiële details & Tijdlijn
Financiële details
Subsidiebedrag | € 9.875.391 |
Totale projectbegroting | € 9.875.391 |
Tijdlijn
Startdatum | 1-3-2025 |
Einddatum | 28-2-2031 |
Subsidiejaar | 2025 |
Partners & Locaties
Projectpartners
- RHEINISCHE FRIEDRICH-WILHELMS-UNIVERSITAT BONNpenvoerder
- INSTITUTO DE FISICA DE ALTAS ENERGIAS
- JOHANNES GUTENBERG-UNIVERSITAT MAINZ
- ISTITUTO NAZIONALE DI FISICA NUCLEARE
Land(en)
Vergelijkbare projecten binnen European Research Council
Project | Regeling | Bedrag | Jaar | Actie |
---|---|---|---|---|
A Gamma-ray Infrastructure to Advance Gravitational Wave AstrophysicsGIGA aims to establish a gamma-ray pulsar timing array to detect gravitational wave backgrounds, enhancing our understanding of supermassive black hole mergers and probing physics beyond the Standard Model. | ERC Starting... | € 1.658.500 | 2024 | Details |
Making Sense of the Unexpected in the Gravitational-Wave SkyGWSky aims to develop a framework for precision gravitational wave astronomy to identify anomalies in signals and enhance our understanding of gravity, particle physics, and cosmology. | ERC Synergy ... | € 11.982.258 | 2025 | Details |
Holography in the Gravitational Wave EraThis project aims to enhance understanding of quantum matter and gravity through holography, focusing on cosmological phase transitions, neutron star mergers, and spacetime singularities. | ERC Advanced... | € 2.499.451 | 2025 | Details |
Dynamical Formation of Black Hole MergersThis ERC research program aims to advance gravitational wave astrophysics by developing tools and methods to investigate binary black hole mergers and their formation in dense stellar environments. | ERC Starting... | € 1.919.186 | 2022 | Details |
Pulsar timing array Inference of the Nanohertz Gravitational wave UniversePINGU aims to establish a robust framework for detecting nano-Hz gravitational waves from supermassive black hole binaries, unlocking new insights into astrophysics and galaxy evolution. | ERC Advanced... | € 2.291.444 | 2025 | Details |
A Gamma-ray Infrastructure to Advance Gravitational Wave Astrophysics
GIGA aims to establish a gamma-ray pulsar timing array to detect gravitational wave backgrounds, enhancing our understanding of supermassive black hole mergers and probing physics beyond the Standard Model.
Making Sense of the Unexpected in the Gravitational-Wave Sky
GWSky aims to develop a framework for precision gravitational wave astronomy to identify anomalies in signals and enhance our understanding of gravity, particle physics, and cosmology.
Holography in the Gravitational Wave Era
This project aims to enhance understanding of quantum matter and gravity through holography, focusing on cosmological phase transitions, neutron star mergers, and spacetime singularities.
Dynamical Formation of Black Hole Mergers
This ERC research program aims to advance gravitational wave astrophysics by developing tools and methods to investigate binary black hole mergers and their formation in dense stellar environments.
Pulsar timing array Inference of the Nanohertz Gravitational wave Universe
PINGU aims to establish a robust framework for detecting nano-Hz gravitational waves from supermassive black hole binaries, unlocking new insights into astrophysics and galaxy evolution.