Scientific Core Workbench
Explore a positive isotropic thermal-tail distribution, relativistic bremsstrahlung, an optically-thin synchrotron emission boundary, and an exact linear ideal-MHD interface benchmark. Every result is scoped to its equation and domain.
Distribution mean energy
Bremsstrahlung emitted power
Synchrotron emission boundary
Canonical interface result
Energy-distribution shape
Normalized energy PDF in keV⁻¹. The chart is a distribution diagnostic, not a fusion-power prediction.
Method and evidence boundaries
Kinetic distribution
The browser uses a convex thermal-tail mixture and reports its normalization and moments. The Python validation suite separately evaluates the full two-isotropic-distribution angular integral and recovers the Maxwellian p–¹¹B reactivity within its declared tolerance. No Fokker–Planck evolution or sustaining-power term is present.
Radiation
Bremsstrahlung uses the Putvinski–Ryutov–Yushmanov relativistic fit. Synchrotron is total optically-thin Maxwell–Jüttner emission. Since absorption, wall reflection and spectral transport are absent, net synchrotron loss deliberately remains unavailable.
Stability
The exact magnetic Rayleigh–Taylor dispersion relation is complete only for two incompressible semi-infinite layers with tangential fields. It is a canonical verification problem, not a Grad–Shafranov-coupled eigenmode calculation and not a stability result for an HBF device.
Completion report · Independent reproduction package · Machine-readable phase status