The physics of magneto-inertial compression
Magneto-inertial fusion compresses a magnetised target on inertial time-scales. The embedded field does not hold the plasma the way a tokamak's field does; it lengthens the path heat must take to leave the fuel while a liner, a jet shell or a colliding plasmoid does the compressing. This page collects the closed-form relations the four device cores of the family evaluate, in the order a shot happens: the drive, the compression, and what the ideal relations leave out.
computational_prototype maturity. The compression laws are conservation laws in their ideal limit: a real liner has finite conductivity and loses flux, a real compression radiates and conducts. They are therefore upper bounds, never predictions. No equation of motion, equation of state or transport equation is solved here; no yield, gain, reactivity, confinement or breakeven statement is made; no value describes or validates any real machine.1 · Where the regime sits
Magnetic confinement holds a low-density plasma for seconds with a field it never lets go of. Inertial confinement compresses a dense target so fast that its own inertia holds it together for the nanoseconds of the burn. Magneto-inertial fusion takes the middle: a target that is already magnetised is compressed by a driver on the microsecond to nanosecond scale, and the field, compressed with it, slows thermal conduction out of the fuel. Density and time-scale sit between the two classical regimes, which is why the four configurations of this family can look so different — a pulsed-power liner, a rotating liquid metal, thirty plasma guns, two colliding compact toroids — and still share one set of governing relations.
2 · The drive
Field and pressure at the liner surface (MagLIF)
An axial current \(I\) through a cylindrical liner of radius \(r\) puts an azimuthal field at its surface, and that field carries a magnetic pressure:
Liner mass and implosion energy (material liner, MagLIF)
A liner is declared from the outside in: inner radius \(r\), wall thickness \(d\), length \(l\), material density \(\rho\). Its mass is the exact annulus, not the thin-shell approximation; the two differ by a fraction \(d/(2r+d)\), which is 0.74 % at the filed Los Alamos design point and comparable to the tolerance the energy anchor is asserted at, so it is not discarded.
Preheat (MagLIF)
The second MagLIF stage deposits laser energy \(E_{\mathrm{pre}}\) into the fuel column the bore encloses. The core records the energy per unit fuel volume:
A liner made of jets (plasma-jet MIF)
An array of \(N\) plasma guns on a launch sphere of radius \(R\) fires jets of radius \(r_j\), speed \(v\) and total mass \(M\). Each jet subtends a half-angle at the centre; the caps add up to a fraction of the sphere; the liner the jets are meant to form has a shell density and a ram pressure:
3 · The compression
Once the liner converges by a ratio \(C = r_0/r\), three ideal conservation laws bound what happens to the enclosed field, density and temperature. The exponent depends on the geometry, and that difference is the reason the plasma-jet core writes its own relations rather than borrowing the cylindrical ones.
Cylindrical liner (MagLIF, material liner, FRC in a theta-pinch coil)
Spherical liner (plasma jets)
What the ideal laws imply for pressure and beta
Combining the cylindrical relations, the thermal pressure \(p = nk_BT\) grows as \(C^{2+2(\gamma-1)} = C^{10/3}\) while the magnetic pressure grows as \(C^4\). Their ratio, the plasma beta, therefore falls as \(C^{-2/3}\) under ideal cylindrical compression: the field gains on the plasma. This is a consequence of the same three laws, stated here for orientation; the cores do not record beta.
4 · What the ideal laws leave out
The relations above are ceilings. Three of the losses that lower them are named explicitly in the family's own repositories, with the solver that carries them living in SCPN-Fusion-Core, never in a device core:
- Finite conductivity. A real liner and a real plasma lose flux. SCPN-Fusion-Core carries a non-adiabatic flux evolution \(\mathrm{d}\psi/\mathrm{d}t = -\psi/\tau_\psi + R_{\mathrm{null}} E_\theta - \eta_{\mathrm{Spitzer}} J_\theta\) after Ono et al. 1997.
- Radiation and conduction. The adiabatic exponent assumes no heat leaves. The embedded field slows conduction; it does not stop it, and it does nothing for radiation.
- Magneto-Rayleigh–Taylor instability. A decelerating or accelerating liner–plasma interface grows ripples; the family's MagLIF core budgets it as device truth, and SCPN-Fusion-Core carries the growth rate \(\gamma(k,a_{\mathrm{eff}}) = \sqrt{k a_{\mathrm{eff}} - k^2 B_\perp^2/(\mu_0 \rho)}\) after Velikovich et al. 2007.
- Jet merging. Whether thirty jets become one liner is a question the filed plasma-jet source studies; the core reports the cap sum and stops.
5 · The target: a field-reversed configuration
Two of the four configurations compress a compact toroid, and the FRC is the target the group's own SCPN-FRC-CORE describes. Its level-0 physics is radial pressure balance and an empirical bound on kinetic scale:
The FRC-compression configuration adds the kinematics of two counter-propagating plasmoids that must arrive at the chamber centre phase-locked. SCPN-MIF-Core writes them as a Doppler-corrected, distance-coupled Kuramoto pair, a chamber-fixed moving frame and a merge-window monitor: