Laser–plasma instabilities and hot-electron preheat are another physics issues that may behave differently at the NIF scale than at Omega scale. Planar experiments on the NIF have identified that stimulated Raman scattering (SRS) is the primary hot-electron source, in contrast to two-plasmon decay (TPD) on OMEGA.5,6 Hot-electron energy deposited in PDD implosions has been diagnosed using hard x-ray measurements and is close to levels thought to be tolerable in direct-drive ignition designs.
Preheat experiments in PDD implosions have also demonstrated the use of Si layers to mitigate preheat in implosions. Further NIF experiments are needed to extrapolate and estimate the level of preheat that is expected in ignition-scale cryogenic implosions.