Use a steady planar sonic ablation model with absorbed intensity Ia, critical mass density ρc=(Ai/Z)munc, and nc=ϵ0me(2πc/λ)2/e2. In the usual isothermal-electron sonic balance, Ia≃4ρccs3 and the ablation pressure is PA≃2ρccs2. Eliminating cs givesFor Ai/Z≃2 and complete absorption, the supplied laser parameters give about 1.15×1013 Pa, or 115 Mbar. Mach one alone fixes neither the material mass per electron nor the enthalpy/absorption coefficient. Different sonic-flow closures change the order-one constant; incomplete absorption multiplies the estimate by its fraction to power 2/3. The robust result is the two-thirds scaling, rather than a material-independent numerical pressure.
PA≃C(Ia/λ)2/3,C=[ZAi2e2muϵ0me(2πc)2]1/3.
An inertially confined sphere disassembles on approximately τ∼r/cs, while ni=ρ/mˉi. Substitute these in the given number-density confinement product to getFor an equal D-T mix, mˉi≃2.5mu. Taking cs∼2kBT/mˉi at 10 keV gives A≃0.365 kg m−2=0.0365 g cm−2. An adiabatic sound-speed convention changes this by an order-one factor. This estimate implements the supplied Lawson product and is not the separate, more stringent alpha-stopping areal-density criterion.
ρr≳1020mˉics≡A.
The final radius is rf=0.5 mm/15=33.3 μm. For a 3.5 MeV alpha particle, p≃2mαEα and the largest perpendicular gyroradius is p/(2eBf). Setting it equal to the core radius givesThis is an order-of-magnitude onset estimate for magnetic deflection, assuming flux freezing and a suitably oriented field. A small gyroradius alone does not ensure complete confinement along open field lines or efficient deposition for every pitch angle.
Bf∼8.1×103 T,Bi=Bf/152∼36 T.
Magnetic pressure is the field energy density PB=Bf2/(2μ0). Using the preceding final field gives PB≃2.6×1013 Pa≃260 Mbar. This uses the compressed field, not the initial 36 T field; substituting the latter would omit the square of the already squared convergence amplification.
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