2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/178581The close agreement between the predictions of dynamical general relativity for the radiated power of a compact binary system and the observed orbital decay of the binary pulsars PSR B1913+16 and PSR B1534+12 allows us to bound the graviton mass to be less than 7.6 x 10^{-20} eV with 90% confidence. This bound is the first to be obtained from dynamic, as opposed to static-field, relativity. The resulting limit on the graviton mass is within two orders of magnitude of that from solar system measurements, and can be expected to improve with further observations.16 pages, 1 figure. Added appendix on other choices for mass termGeneral Relativity and Quantum CosmologyAstrophysicsHigh Energy Physics - Theorytext