The Earth’s outer radiation belt has long received considerable attention mainly because the MeV electron flux in the belt varies often dramatically and at various time scales. It is now widely accepted that the wave-particle interaction is one of the major mechanisms responsible for such flux variations. The wave-particle interaction can accelerate electrons to MeV energies, explaining the observed flux increase events, and can also scatter the electrons’ motion into the loss cone, resulting in atmospheric precipitation and thus contributing to flux dropouts. In this paper, we provide a review of the current state of research on relativistic electron scattering and precipitation due to the interaction with electromagnetic ion cyclotron (EMIC) waves in the inner magnetosphere. The review is intended to cover progress made over the last ~15 years in the theory and simulations of various issues, including quasilinear resonance diffusion, nonlinear interactions, nonresonant interactions, effects of finite normal angle on pitch angle scattering, effects due to rising tone emission, and ways to scatter near-equatorial pitch angle electrons. The review concludes with suggestions of a few promising topics for future research.

1. INTRODUCTION
 2. PROGRESS FROM QUASILINEAR RESONANCE THEORY
 3. NONLINEAR AND NONRESONANT ERRECTS
 4. NONLINEAR EFFECTS OF OBLIQUE PROPAGATION AND QUASILINEAR POLARIZATION
 5. POSSIBLE WAYS SCATTER NEAR-EQUATORIAL PITCH ANGLE ELECTRONS
 6. PRECIPITAION DUE TO RISING TONE EMISSIONS
 7. CONCLUDING REMARKS
 REFERENCES

• Dae-Young Lee(Department of Astronomy and Space Science, Chungbuk National University) Corresponding Author