Massive black hole binary mergers produce orphaned low-frequency signals in PTA pulsar terms that can be stacked for archival multiband gravitational-wave detection.
Living Reviews in Relativity , volume =
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The Hubble parameter produces a frequency-independent angular enhancement in LISA timing residuals above 100 mHz, potentially enabling a percent-level H0 measurement without standard sirens.
A large collaboration compiles and compares merger rate predictions for massive black holes across multiple galaxy formation models to forecast LISA detections and quantify uncertainties.
Calculations showing that rapidly spinning black holes permit stable orbits close enough to the horizon for extreme time dilation matching Interstellar, with suggested astrophysical uses.
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Archival Multiband Gravitational-Wave Signals from Massive Black Hole Binary Mergers
Massive black hole binary mergers produce orphaned low-frequency signals in PTA pulsar terms that can be stacked for archival multiband gravitational-wave detection.
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Impact of $H_0$ on gravitational wave propagation: prospects for the LISA mission
The Hubble parameter produces a frequency-independent angular enhancement in LISA timing residuals above 100 mHz, potentially enabling a percent-level H0 measurement without standard sirens.
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The LISA Astrophysics MBHcatalogues Project: A comparison of predictions of simulated massive black hole binaries
A large collaboration compiles and compares merger rate predictions for massive black holes across multiple galaxy formation models to forecast LISA detections and quantify uncertainties.
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Astrophysical Applications of the Physics presented in the Film Interstellar
Calculations showing that rapidly spinning black holes permit stable orbits close enough to the horizon for extreme time dilation matching Interstellar, with suggested astrophysical uses.