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

Making Sense of the Unexpected in the Gravitational-Wave Sky

Project description

New models to separate gravitational wave signals from noise

General relativity remains the cornerstone of our understanding of gravity, predicting phenomena such as black holes and gravitational waves, both resulting in Nobel prizes. The future of gravitational wave astronomy seems bright since detectors are expected to observe black holes at cosmic dawn and their enigmatic event horizons, where general relativity and quantum mechanics clash. However, interpreting these signals requires a groundbreaking framework to solve complex non-linear equations of general relativity and model waveforms with unprecedented accuracy. The ERC-funded GWSky project plans to develop such a framework that should help distinguish true anomalies from effects caused by nearby matter or imprecise calculations. GWSky advanced tools should allow more accurate gravitational wave observations in upcoming research campaigns.

Objective

General Relativity (GR) is more than a century old, but is still our best macroscopic description of gravity. Key GR predictions are black holes (BHs) and gravitational waves (GWs), whose spectacular confirmation led to two recent physics Nobel Prizes. The future of GW astronomy, however, is even brighter, since detectors will observe BHs at cosmic dawn and probe their enigmatic event horizon, where GR clashes with quantum mechanics in the information loss paradox. These experiments will measure signals hundreds of times smaller than today, necessarily discovering anomalies and deviations from current predictions, e.g. due to the astrophysical environment. On the fundamental side, precision GW astronomy will open countless possibilities for understanding the standard model of particle physics (and its extensions), gravity and cosmology. By itself, however, precision is not knowledge. To harness the power of these measurements, a groundbreaking framework is urgently needed to solve the very nonlinear equations of GR and develop waveform models to unprecedented accuracy, and to convert these results into concrete interpretation tools. GWSky will leverage the world-leading expertise of its PIs in astrophysics, GW-source modeling, particle physics and GR, and recent paradigm shifts to build an overarching framework answering a fundamental question: When, inevitably, an anomaly in a GW signal is identified, what is it? A gravitational effect not predicted by GR? The influence of nearby matter? Or merely an imprecise calculation of the expected signal? Even tiny deviations from GR would shake physics to its core, but to claim a deviation from it, one needs to filter out first the contributions from the astrophysical environment, instrumental artifacts and systematic modeling uncertainties. GWSky will provide tools to disentangle these contributions, enabling precision GW astronomy with upcoming observational runs, and new facilities on the ground and in space.

Keywords

Project’s keywords as indicated by the project coordinator. Not to be confused with the EuroSciVoc taxonomy (Fields of science)

Programme(s)

Multi-annual funding programmes that define the EU’s priorities for research and innovation.

Topic(s)

Calls for proposals are divided into topics. A topic defines a specific subject or area for which applicants can submit proposals. The description of a topic comprises its specific scope and the expected impact of the funded project.

Funding Scheme

Funding scheme (or “Type of Action”) inside a programme with common features. It specifies: the scope of what is funded; the reimbursement rate; specific evaluation criteria to qualify for funding; and the use of simplified forms of costs like lump sums.

HORIZON-ERC-SYG - HORIZON ERC Synergy Grants

See all projects funded under this funding scheme

Call for proposal

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

(opens in new window) ERC-2024-SyG

See all projects funded under this call

Host institution

MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV
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.

€ 3 265 398,25
Address
HOFGARTENSTRASSE 8
80539 MUNCHEN
Germany

See on map

Region
Bayern Oberbayern München, Kreisfreie Stadt
Activity type
Research Organisations
Links
Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

€ 3 265 398,25

Beneficiaries (4)

My booklet 0 0