Preserve the primary constraints using the corrected Hamiltonian from solution. After a spatial integration by parts, the terms in its density are . Hamilton's equations giveWith the definitions of in the paper, the actual massive Gauss law is thereforeThis is also the component of the Proca equation. The zero right-hand sides printed in the source apply only to the massless theory or to special configurations with .
For a concrete counterexample, take , , and the longitudinal on-shell plane waveIt satisfies , but and . Imposing the printed zero-divergence condition would incorrectly remove the physical longitudinal particle polarization.
Phase-space action Created 2026-10-05 Updated 2026-10-06
A phase-space action treats canonical variables as independent fields. Varying them gives Hamilton's equations; Lagrange multipliers can impose constraints.
Regular Lagrangian 2026-10-06
A Lagrangian is regular when its velocity Hessian matrix is invertible. The inverse function theorem then makes the fiber derivative locally invertible, allowing a local Legendre transform in mechanics to a Hamiltonian. If that fiber derivative is globally invertible, the Lagrangian is called a hyperregular Lagrangian. Regularity alone does not assert global invertibility, and singular Lagrangians may give constrained rather than ordinary unconstrained Hamilton's equations.
The type-two generating function for a canonical transformation defines and . On any branch with and , its inverse in mixed coordinates isThe square root equals on this branch. Differentiating proves the generating equations, and proves local invertibility by the inverse function theorem. Also , so the symplectic form obeys . This proves the transformation is canonical locally. It is not a single global chart across the inverse-trigonometric branch boundaries.
Since is independent of time, the transformed Hamiltonian is obtained by substitution, with zero generating-function time correction. An added function of time alone is an irrelevant Hamiltonian freedom, since it leaves Hamilton's equations unchanged.