Week 6
Plasma Physics and Laser–Plasma Interactions
Critical density, SBS, SRS, inverse bremsstrahlung.
~6 hrs Hohlraum, target chamber Critical density ↔ choked flow at Mach 1
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STUDY_PLAN.md§Week 6.
Goals
- Know the three fundamental plasma parameters: Debye length , plasma frequency , critical density .
- Understand the critical density as the cutoff for laser propagation into plasma.
- Know the three main laser-plasma instabilities at NIF: SBS, SRS, two-plasmon decay.
Master equations
Plasma frequency:
Critical density:
So and . 3ω penetrates 9× denser plasma than 1ω — the single biggest reason NIF uses 3ω.
NIF tie-in
The choice of 3ω over 1ω is driven entirely by plasma physics:
- Higher critical density → laser deposits energy closer to the hohlraum wall → more efficient X-ray conversion.
- Higher density → shorter LPI growth lengths → less SBS/SRS.
- Higher inverse-bremsstrahlung absorption at shorter wavelengths.
Pay 28% efficiency loss in KDP frequency tripling → gain a factor of 9 in critical density, ~10× in X-ray drive efficiency, and 10–100× in LPI suppression. This is the master physics-engineering trade of the entire NIF design. In one sentence: "3ω costs us a third of our laser energy in frequency conversion, but it lets us drive 10× denser plasma with 10× less backscatter loss. It's not a choice; it's the physics."
Self-check
Self-check
Answer each from memory. If you can't, re-read the marked section.