Program :
The direct detection of Gravitational Waves (GW) has opened a new window on the observable universe. The sensitivity of current experiments is steadily increasing, and even more sophisticated detectors are planned for the coming decades. The success of this program hinges on producing accurate theoretical predictions which can be used for detection and parameter estimation. The objective of this three-week program is twofold. First, to bring together experts on post-Newtonian, post-Minkowskian, self-force, soft-theorem approaches to the gravitational two-body problem as well as on state-of-the-art detectors, in order to sharpen our theoretical tools and develop new methods and ideas to rise up to the challenges posed by future detectors. Second, to promote the visibility and interactions of young researchers working on these topics, to kick start and maintain collaborations that result in long-lasting research links.
Organisers:
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Stanislav Babak (APC)
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Laura Bernard (OBSPM)
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Carlo Heissenberg (IPhT)
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Andres Luna (NBI)
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Nathan Moynihan (QMUL)
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Julio Parra-Martinez (IHES)
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Matteo Sergola (UCLA)
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Maarten van de Meent (NBI)
Information de la conférence
Application
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