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Precise predictions for extreme mass ratio inspirals

Project description

New fundamental science through the Laser Interferometer Space Antenna

The first direct observation of gravitational waves was made in 2015 by the Laser Interferometer Gravitational-Wave Observatory (LIGO). The European Space Agency has since approved the space-based Laser Interferometer Space Antenna (LISA) as one of its three highest-priority missions for the 2030s. The sensitivity of LISA will be in the millihertz gravitational-wave band, of which one of the most prominent and significant sources are the so-called extreme mass ratio inspirals (EMRIs). However, the precise predictions for the evolution of EMRIs are not ready yet. The EU-funded PreciseEMRIs project will contribute to the development of these precise predictions. The project will contribute to the discovery of new fundamental science through LISA and other gravitational-wave detectors.

Objective

The gravitational-wave sky has been opened by the first measurement of a gravitational-wave inspiral in 2015 by LIGO. Now, the European detector Virgo has joined the network, and more terrestrial detectors are underway. Furthermore, the European space agency has approved the space-based Laser interferometer space antenna (LISA) as one of its three highest-priority missions for the 2030s. The scientific capabilities of LISA provide European science with a chance to be at the absolute cutting edge of gravitational-wave astronomy.

The sensitivity of LISA will be in the in the millihertz gravitational-wave band. One of the most prominent and interesting sources seen in this band are the so-called extreme mass ratio inspirals (EMRIs), where a light, stellar-mass compact object spirals into a super-massive black hole. However, at the moment the precise predictions for the evolution of EMRIs are not ready, and this, if not rectified, would imply lower yields of valuable science to be obtained from the LISA mission. The subject of this proposal is to contribute to the development of these precise predictions, and to prepare for the discovery of new fundamental science with LISA and other gravitational-wave detectors.

Even though the launch of LISA is more than 10 years in the future, the mathematical and technical challenge of providing the precise predictions is extremely non-trivial, and intense work must thus be initiated now. This research project will not only contribute a significant part of the work needed, but it will also allow the applicant to acquire the necessary skill and network to become one of the leading figures in the field of gravitational-wave theory.

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Keywords

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Programme(s)

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Topic(s)

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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.

MSCA-IF - Marie Skłodowska-Curie Individual Fellowships (IF)

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Call for proposal

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

(opens in new window) H2020-MSCA-IF-2019

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Coordinator

UNIVERSITY COLLEGE DUBLIN, NATIONAL UNIVERSITY OF IRELAND, DUBLIN
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.

€ 184 590,72
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.

€ 184 590,72
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