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gr-qc2025
Uncertainty-aware waveform modeling for high signal-to-noise ratio gravitational-wave inference
Simone Mezzasoma, Carl-Johan Haster, Caroline B. Owen +2
Semi-analytical waveform models for black hole binaries require calibration against numerical relativity waveforms to accurately represent the late inspiral and merger, where analy…
gr-qc2025
Constraining dark-sector effects using gravitational waves from compact binary inspirals
Caroline B. Owen, Alexandria Tucker, Yonatan Kahn +1
Gravitational wave observations are a powerful tool to constrain fundamental physics. This work considers dark matter that carries charge under a dark abelian massive vector field.…