Detecting stochastic gravitational waves with binary resonance

LIGO and Virgo have initiated the era of gravitational-wave (GW) astronomy; but in order to fully explore GW frequency spectrum, we must turn our attention innovative techniques for detection. One such approach is use binary systems as dynamical detectors by studying subtle perturbations their orbits caused impinging GWs. We present a powerful new formalism calculating orbital evolution generic coupled stochastic background GWs, deriving from first principles secularly-averaged Fokker-Planck equation which characterises statistical all six binary's elements. also develop practical tools numerically integrating this equation, derive necessary search GWs observational data pulsars laser-ranging experiments.