2.I.9C

Classical Dynamics | Part II, 2007

The Lagrangian for a particle of mass mm and charge ee moving in a magnetic field with position vector r=(x,y,z)\mathbf{r}=(x, y, z) is given by

L=12mr˙2+er˙AcL=\frac{1}{2} m \dot{\mathbf{r}}^{2}+e \frac{\dot{\mathbf{r}} \cdot \mathbf{A}}{c}

where the vector potential A(r)\mathbf{A}(\mathbf{r}), which does not depend on time explicitly, is related to the magnetic field B\mathbf{B} through

B=×A\mathbf{B}=\nabla \times \mathbf{A}

Write down Lagrange's equations and use them to show that the equation of motion of the particle can be written in the form

mr¨=er˙×Bcm \ddot{\mathbf{r}}=e \frac{\dot{\mathbf{r}} \times \mathbf{B}}{c}

Deduce that the kinetic energy, TT, is constant.

When the magnetic field is of the form B=(0,0,dF/dx)\mathbf{B}=(0,0, d F / d x) for some specified function F(x)F(x), show further that

x˙2=2Tm(eF(x)+C)2m2c2+D\dot{x}^{2}=\frac{2 T}{m}-\frac{(e F(x)+C)^{2}}{m^{2} c^{2}}+D

where CC and DD are constants.

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