Black hole superradiance is a fascinating process in general relativity and a unique window on ultralight particles beyond the standard model. Bosons -- such as axions and dark photons -- with Compton wavelengths comparable to size of astrophysical black holes grow exponentially to form large clouds spinning down the black hole in the process and produce monochromatic continuous gravitational wave radiation. In the era of gravitational wave astronomy and increasingly sensitive observations of astrophysical black holes and their properties superradiance of new light particles is a promising avenue to search for new physics in regimes inaccessible to terrestrial experiments. This workshop will bring together theorists data analysts and observers in particle physics gravitational wave astronomy strong gravity and high energy astrophysics to explore the signatures of black hole superradiance and to study the current and future possibilities of searching for new particles with black holes.
Format results
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Searching for Light Bosons with Black Hole Superradiance
Perimeter Institute for Theoretical Physics -
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Superradiant instabilities and rotating black holes
University of Waterloo -
Measuring Stellar-Mass Black Hole Spins via X-ray Spectroscopy
Massachusetts Institute of Technology (MIT) -
Superradiance Beyond the Linear Regime
Princeton University -
Characterization of compact objects with present and future ground-based gravitational-wave detectors
Massachusetts Institute of Technology (MIT) -
LIGO and Virgo continuous wave searches - Overview and all-sky searches
University of Michigan–Ann Arbor -
Directed and targeted searches for continuous gravitational waves
Albert Einstein Institute -
Where do black hole binaries come from, and can we actually know that?
Canadian Institute for Theoretical Astrophysics (CITA) -
Gravitational wave searches for ultralight bosons
Max Planck Institute for Gravitational Physics - Albert Einstein Institute (AEI) -