Classical Electrodynamics · Problem 16.2

Radiation Damping, Classical Models of Charged Particles — John David Jackson

Physics — E&M · radiation-damping-circular-orbit

Problem

A nonrelativistic electron of charge −e-e and mass mm bound in an attractive Coulomb potential (−Ze2/r)(-Ze^2/r) moves in a circular orbit in the absence of radiation reaction. (a) Show that both the energy and angular-momentum equations (16.13) and (16.16) lead to the solution for the slowly changing orbit radius, r3(t)=r03−9Z(cτ)3tτr^3(t) = r_0^3 - 9Z(c\tau)^3 \frac{t}{\tau} where r0r_0 is the value of r(t)r(t) at t=0t = 0. (b) For circular orbits in a Bohr atom the orbit radius and the principal quantum number nn are related by r=n2a0/Zr = n^2 a_0/Z. If the transition probability for transitions from n→(n−1)n \to (n-1) is defined as −dn/dt-dn/dt, show that the result of part a agrees with that found in Problem 14.21. (c) From part a calculate the numerical value of the times taken for a mu meson of mass m=207mem = 207 m_e to fall from a circular orbit with principal quantum number n1=10n_1 = 10 to one with n2=4n_2 = 4, and n2=1n_2 = 1. These are reasonable estimates of the time taken for a mu meson to cascade down to its lowest orbit after capture by an isolated atom.

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