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Black Holes Black Hole Mergers Detection Methods LIGO Binary Black Holes Extreme Mass-Ratio Inspirals Waveform Modeling Pulsar Timing Arrays Black Hole Collisions Black Hole Scattering Quasinormal Modes Detection Technology Quasi-Normal Modes Primordial Black Holes Binary Coalescences Mathematical Modeling Black Hole Perturbations Observational Astronomy Black Hole Spectroscopy General Relativity Cosmic Strings Einstein Telescope LIGO-India Electromagnetic Signals Supermassive Black Hole Binaries Instability Dynamics Statistical Modeling Self-Force Theory Post-Newtonian Approximations Black Hole Binaries Waveform Models Pulsars Future Observatories Massive Pulsars Detector Technology Detection of Black Holes Ringdown Phase Binary Black Hole Mergers Mini-EMRIs Mass Ratios and Spins Pulsar Timing Detection X-ray Signals Neutron Star Mergers Laser Interferometer Space Antenna (LISA) Detection Process Neutron Stars
The analysis links specific mass thresholds for human injury to tentative limits on primordial black holes as dark matter.
