  We generalize the worldline EFT formalism developed in [4-9] to calculate the
non-conservative tidal effects on spinning black holes in a long wavelength
approximation that is valid to all orders in the magnitude of the spin. We
present results for the rate of change of mass and angular momentum in a
background field and find agreement with previous calculations obtained by
different techniques. We also present new results for both the non-conservative
equations of motion and power loss/gain for a binary inspiral, which start at
5PN and 2.5PN order respectively and manifest the Penrose process.
