Bayesian analysis of LISA EMRIs in AGN disks constrains disk surface density and accretion rate to ~10% using relativistic torque models, invalidating Fisher-matrix forecasts and enabling dark-siren cosmology without EM counterparts.
Science opportunities of wet extreme mass-ratio inspi- rals,
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
QPE observations yield EMRI rates of 2.88e-6 (stellar) and 6.07e-6 (black hole) per galaxy per year, with only black hole EMRIs potentially exceeding LISA sensitivity in the 1-10 mHz band.
citing papers explorer
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Gotta light? Illuminating AGN disks with LISA EMRIs
Bayesian analysis of LISA EMRIs in AGN disks constrains disk surface density and accretion rate to ~10% using relativistic torque models, invalidating Fisher-matrix forecasts and enabling dark-siren cosmology without EM counterparts.
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Extreme Mass Ratio Inspirals in Light of Quasi-periodic Eruptions: Milli-Hertz Gravitational Wave Background
QPE observations yield EMRI rates of 2.88e-6 (stellar) and 6.07e-6 (black hole) per galaxy per year, with only black hole EMRIs potentially exceeding LISA sensitivity in the 1-10 mHz band.