Emergent Lorentz effects — ideal relativistic animation
This animation is an ideal pedagogical illustration based on the exact Lorentz formulas,
not on the Julia soliton solver. It is meant to show clearly what length contraction and clock slowing
look like, even deep in the ultra-relativistic regime.
Rest soliton
Reference profile on a fixed ruler
Moving soliton
Tracked window, same spatial scale
Status distinction: this animation uses the ideal relativistic laws
w(v)=w₀/γ and T(v)=γT₀.
It is therefore a clean illustration of the target behaviour.
The Julia simulations have a different status: they test whether your effective soliton model
dynamically reproduces these Lorentzian predictions.