Paper 1, Section II, E

Electrodynamics | Part II, 2016

A point particle of charge qq and mass mm moves in an electromagnetic field with 4 -vector potential Aμ(x)A_{\mu}(x), where xμx^{\mu} is position in spacetime. Consider the action

S=mc(ημνdxμdλdxνdλ)1/2dλ+qAμdxμdλdλS=-m c \int\left(-\eta_{\mu \nu} \frac{d x^{\mu}}{d \lambda} \frac{d x^{\nu}}{d \lambda}\right)^{1 / 2} d \lambda+q \int A_{\mu} \frac{d x^{\mu}}{d \lambda} d \lambda

where λ\lambda is an arbitrary parameter along the particle's worldline and ημν=diag(1,+1,+1,+1)\eta_{\mu \nu}=\operatorname{diag}(-1,+1,+1,+1) is the Minkowski metric.

(a) By varying the action with respect to xμ(λ)x^{\mu}(\lambda), with fixed endpoints, obtain the equation of motion

mduμdτ=qFνμuνm \frac{d u^{\mu}}{d \tau}=q F_{\nu}^{\mu} u^{\nu} \text {, }

where τ\tau is the proper time, uμ=dxμ/dτu^{\mu}=d x^{\mu} / d \tau is the velocity 4-vector, and Fμν=μAννAμF_{\mu \nu}=\partial_{\mu} A_{\nu}-\partial_{\nu} A_{\mu} is the field strength tensor.

(b) This particle moves in the field generated by a second point charge QQ that is held at rest at the origin of some inertial frame. By choosing a suitable expression for AμA_{\mu} and expressing the first particle's spatial position in spherical polar coordinates (r,θ,ϕ)(r, \theta, \phi), show from the action ()(*) that

Et˙Γ/rcr2ϕ˙sin2θ\begin{aligned} \mathcal{E} & \equiv \dot{t}-\Gamma / r \\ \ell c & \equiv r^{2} \dot{\phi} \sin ^{2} \theta \end{aligned}

are constants, where Γ=qQ/(4πϵ0mc2)\Gamma=-q Q /\left(4 \pi \epsilon_{0} m c^{2}\right) and overdots denote differentiation with respect to τ\tau.

(c) Show that when the motion is in the plane θ=π/2\theta=\pi / 2,

E+Γr=1+r˙2c2+2r2\mathcal{E}+\frac{\Gamma}{r}=\sqrt{1+\frac{\dot{r}^{2}}{c^{2}}+\frac{\ell^{2}}{r^{2}}}

Hence show that the particle's orbit is bounded if E<1\mathcal{E}<1, and that the particle can reach the origin in finite proper time if Γ>\Gamma>|\ell|.

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