LIGO Document T2100339-v1
- The population of observed gravitational wave transients continues to grow, and with it, our ability to further constrain deviations from the signals predicted by general relativity. However, our current procedures for computing these constraints will not successfully scale with future transient catalogs. Thus, we leverage modern statistical methods into a new hybrid sampling method, in order to provide more efficient and more complete investigations of the parameter space of deviations from general relativity given gravitational wave observations of binary black hole mergers.
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