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This paper investigates the speed and dispersion of gravitational waves (GWs) using LISA observations of supermassive black hole binary (SMBHB) mergers. The authors simulate three SMBHB populations over a five-year mission, deriving constraints on graviton mass and dispersion coefficients, with results indicating potential deviations from the speed of light as predicted by general relativity. The study emphasizes the importance of SMBHB mergers as targets for probing gravitational wave propagation effects d

Author

abderrahimelkhou00

Language

EN