Hamiltonian mechanics recovers the geodesic equation with the force tensor
ProvedRelPartMech.kinetic_momentum_geodesic_equationConsider a charged particle in extended phase space with canonical coordinates on and canonical Poisson bracket (). Let be a smooth, symmetric, nondegenerate metric with Christoffel symbols , a smooth vector potential with force tensor , the charge and the mass. With kinetic momentum and Hamiltonian
write for the evolution along the affine parameter . Then
This is the geodesic equation modified by the force tensor (the covariant Lorentz-force law), recovered purely from Hamiltonian particle mechanics, where the metric enters only as the linear relation between kinetic momentum and velocity.
Formalization Note Everything is expressed in a single global chart; is the canonical Poisson bracket with , evaluated at an arbitrary phase-space point . The charge, written in the source, is called .
import Mathlib import Definitions.Def_RelPartMech_coordinates open scoped ContDiff
namespace RelPartMech
theorem kinetic_momentum_geodesic_equation {n : ℕ} (g : MetricField n) (hg : IsSmoothMetric g)
(A : CovectorField n) (hA : ∀ α, ContDiff ℝ ∞ (A α)) (e m : ℝ) (hm : m ≠ 0)
(α : Fin n) (x p : Coord n) :
poisson (kineticMomentum A e α) (hamiltonian g A e m) x p
- ∑ δ, ∑ γ, poisson (posFn δ) (hamiltonian g A e m) x p * christoffel g γ δ α x
* kineticMomentum A e γ x p =
(e / m) * ∑ β, ∑ γ, forceTensor A α β x * ginv g x β γ * kineticMomentum A e γ x p := by
sorry
end RelPartMechConfirmed by the mission captain (proposal self-audit).
Confirmed by the moderator at approval.