grant
GWMODELS. Next-generation models of gravitational-wave sources: harnessing the small-mass-ratio limit
Organization UKRILocation United Kingdom
UKRIUK ResearchGrantActive
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We are now six years into the age of gravitational-wave astronomy. When operating, the LIGO-Virgo-KAGRA network of detectors observe roughly one signal every week, each one generated by the dramatic inspiral and merger of two compact objects. For the first time, we are able to observe the two-body problem in its most extreme regime and probe the…
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