Black hole spin will have a large impact on searches for gravitational waves with advanced detectors. While only a few stellar mass black hole spins have been measured using X-ray techniques, gravitational wave detectors have the capacity to greatly increase the statistics of black hole spin measurements. We show what we might learn from these measurements and how the black hole spin values are influenced by their formation channels
Black holes of mass M must have a spin angular momentum S below the Kerr limit (χ ≡ S/M^2 ≤ 1), but ...
Black holes are some of the most mysterious and fascinating objects that exist: with a gravitational...
Gravitational wave detection from binary black hole (BBH) inspirals has become routine thanks to the...
Black hole spin will have a large impact on searches for gravitational waves with advanced detectors...
The observation of gravitational-wave signals from merging black hole binaries enables direct measur...
Characterizing the properties of black holes is one of the most important science objectives for gra...
The Advanced LIGO and Virgo detectors have now observed approximately 50 black hole binary mergers, ...
Ultralight bosons can form clouds around rotating black holes if their Compton wavelength is compara...
Compact binary coalescences are the most promising sources of gravitational waves (GWs) for ground-b...
The gravitational wave measurements of spin-induced multipole moment coefficients of a binary black ...
The era of gravitational-wave astronomy started with the discovery of the binary black hole coalesce...
Gravitational waves are a prediction of general relativity, and with ground-based detectors now runn...
Since the seminal work of Penrose (1969) and Blandford & Znajek (1977), it has been realized tha...
Measuring the spins of supermassive black holes (SMBHs) in active galactic nuclei (AGN) can inform u...
If a black hole has a low spin value, it must double its mass to reach a high spin parameter (Volont...
Black holes of mass M must have a spin angular momentum S below the Kerr limit (χ ≡ S/M^2 ≤ 1), but ...
Black holes are some of the most mysterious and fascinating objects that exist: with a gravitational...
Gravitational wave detection from binary black hole (BBH) inspirals has become routine thanks to the...
Black hole spin will have a large impact on searches for gravitational waves with advanced detectors...
The observation of gravitational-wave signals from merging black hole binaries enables direct measur...
Characterizing the properties of black holes is one of the most important science objectives for gra...
The Advanced LIGO and Virgo detectors have now observed approximately 50 black hole binary mergers, ...
Ultralight bosons can form clouds around rotating black holes if their Compton wavelength is compara...
Compact binary coalescences are the most promising sources of gravitational waves (GWs) for ground-b...
The gravitational wave measurements of spin-induced multipole moment coefficients of a binary black ...
The era of gravitational-wave astronomy started with the discovery of the binary black hole coalesce...
Gravitational waves are a prediction of general relativity, and with ground-based detectors now runn...
Since the seminal work of Penrose (1969) and Blandford & Znajek (1977), it has been realized tha...
Measuring the spins of supermassive black holes (SMBHs) in active galactic nuclei (AGN) can inform u...
If a black hole has a low spin value, it must double its mass to reach a high spin parameter (Volont...
Black holes of mass M must have a spin angular momentum S below the Kerr limit (χ ≡ S/M^2 ≤ 1), but ...
Black holes are some of the most mysterious and fascinating objects that exist: with a gravitational...
Gravitational wave detection from binary black hole (BBH) inspirals has become routine thanks to the...