2.II.15B

Classical Dynamics | Part II, 2008

A particle of mass mm, charge ee and position vector r=(x1,x2,x3)q\mathbf{r}=\left(x_{1}, x_{2}, x_{3}\right) \equiv \mathbf{q} moves in a magnetic field whose vector potential is A. Its Hamiltonian is given by

H(p,q)=12m(peAc)2H(\mathbf{p}, \mathbf{q})=\frac{1}{2 m}\left(\mathbf{p}-e \frac{\mathbf{A}}{c}\right)^{2}

Write down Hamilton's equations and use them to derive the equations of motion for the charged particle.

Define the Poisson bracket [F,G][F, G] for general F(p,q)F(\mathbf{p}, \mathbf{q}) and G(p,q)G(\mathbf{p}, \mathbf{q}). Show that for motion governed by the above Hamiltonian

[mx˙i,xj]=δij, and [mx˙i,mx˙j]=ec(AjxiAixj)\left[m \dot{x}_{i}, x_{j}\right]=-\delta_{i j}, \quad \text { and } \quad\left[m \dot{x}_{i}, m \dot{x}_{j}\right]=\frac{e}{c}\left(\frac{\partial A_{j}}{\partial x_{i}}-\frac{\partial A_{i}}{\partial x_{j}}\right)

Consider the vector potential to be given by A=(0,0,F(r))\mathbf{A}=(0,0, F(r)), where r=x12+x22r=\sqrt{x_{1}^{2}+x_{2}^{2}}. Use Hamilton's equations to show that p3p_{3} is constant and that circular motion at radius rr with angular frequency Ω\Omega is possible provided that

Ω2=(p3eFc)em2crdFdr\Omega^{2}=-\left(p_{3}-\frac{e F}{c}\right) \frac{e}{m^{2} c r} \frac{d F}{d r}

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