Project description
Gravitational-wave observations using more accurate waveforms
The study of gravitational waves has deepened our understanding of stellar phenomena such as binary black holes and neutron stars, driving major breakthroughs across physics and astronomy. However, gravitational-wave (GW) signals are often weaker than background noise in detectors, making them difficult to identify and challenging to analyse due to the need for highly accurate waveforms. Supported by the Marie Skłodowska-Curie Actions programme, the AccModBinary project aims to improve both the detection and parameter inference of GW signals by developing more precise waveforms for increasingly sensitive detectors. To achieve this, it will refine the analytical description of compact binary dynamics within both general relativity and modified gravity theories.
Objective
Gravitational-wave (GW) observations have revolutionized our understanding of binary black holes and neutron stars. Since GW signals are typically weaker than the noise in the detectors, searching for GW signals and inferring their parameters requires accurate waveforms. The goal of this project to improve the analytical description of compact binary dynamics in general relativity and modified gravity theories, through the following related objectives: 1) deriving post-Newtonian results for the dissipative dynamics of spinning binaries, 2) developing the foundations of an effective-one-body waveform model for precessing spins in generic orbits, 3) modeling dynamical scalarization in Einstein-scalar-Gauss-Bonnet gravity to facilitate theory-specific searches for deviations from general relativity, and 4) complement gravitational self-force results with post-Newtonian information to model extreme mass-ratio inspirals in generic orbits. The results of this project will yield more accurate waveforms that are crucial for the increasing sensitivity of the LIGO-Virgo-KAGRA detectors and for future detectors, such as the Einstein telescope and the Laser Interferometer Space Antenna.
Fields of science (EuroSciVoc)
CORDIS classifies projects with EuroSciVoc, a multilingual taxonomy of fields of science, through a semi-automatic process based on NLP techniques. See: The European Science Vocabulary.
CORDIS classifies projects with EuroSciVoc, a multilingual taxonomy of fields of science, through a semi-automatic process based on NLP techniques. See: The European Science Vocabulary.
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Keywords
Project’s keywords as indicated by the project coordinator. Not to be confused with the EuroSciVoc taxonomy (Fields of science)
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.
Multi-annual funding programmes that define the EU’s priorities for research and innovation.
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HORIZON.1.2 - Marie Skłodowska-Curie Actions (MSCA)
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Topic(s)
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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
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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-TMA-MSCA-PF-EF - HORIZON TMA MSCA Postdoctoral Fellowships - European Fellowships
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Call for proposal
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Procedure for inviting applicants to submit project proposals, with the aim of receiving EU funding.
(opens in new window) HORIZON-MSCA-2024-PF-01
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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.
1165 KOBENHAVN
Denmark
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