In cylindrical coordinates the orthogonal velocity components are r˙, rθ˙, z˙. Their squared magnitudes add, and r˙⋅A=z˙A(r). Thus L=m(r˙2+r2θ˙2+z˙2)/2+qz˙A(r). Taking the curl gives Bθ=−A′(r), consistent with the prescribed field.
Velocity differentiation gives pr=mr˙, pθ=mr2θ˙, pz=mz˙+qA(r). The coordinates θ and z are cyclic, so pθ,pz are conserved. The radial momentum generally changes. In particular the conserved axial canonical momentum differs from the axial mechanical momentum by qA.
The Legendre transform cancels the velocity-linear magnetic term. Expressing velocities in terms of momenta givesThe Hamiltonian is time independent and hence conserved. It equals kinetic energy because a static magnetic field does no work; its dependence on A is through the mechanical momentum combination.
H=2mpr2+2mr2pθ2+2m[pz−qA(r)]2.
The initial condition makes pθ=0 at all times. Accessible radii obey ∣pz−qA(r)∣≤2mH. For q>0 and pz>2mH, monotonicity of A gives exactly the two stated turning equations and confinement to the interval between their unique roots.
The squared condition alone omits a sign qualification. More generally both positive roots require pz/q>0, and are the sorted roots A(r)=(pz±2mH)/q. For example q=−1, A=r, pz=−3, 2mH=1 confines the orbit to 2≤r≤4, but the source's named r1,r2 equations reverse those labels. This is a convention issue, not a failure of confinement.
Expand A(r)=A(r0)+A′(r0)s+O(s2) about qA(r0)=pz. Then pz−qA≃−qA′(r0)s and conservation of energy givesHere Ω=qA′(r0)/m can be signed, but the physical oscillation frequency and amplitude are nonnegative. The small-energy condition ensures that this local expansion samples only a narrow range about r0, provided the field varies smoothly there.
s˙2+Ω2s2=m2H=Ω2ρ2,ρ=∣Ω∣2H/m,s(t)=ρcos(∣Ω∣t+ϕ).
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