Electron Motion in Charged Sphere with Radiation · USAPhO 2016 #B2

Physics · electromagnetism

Problem

a. A spherical region of space of radius RR has a uniform charge density and total charge +Q+Q. An electron of charge −e-e is free to move inside or outside the sphere, under the influence of the charge density alone. For this first part ignore radiation effects. i. Consider a circular orbit for the electron where r<Rr < R. Determine the period of the orbit TT in terms of any or all of rr, RR, QQ, ee, and any necessary fundamental constants. ii. Consider a circular orbit for the electron where r>Rr > R. Determine the period of the orbit TT in terms of any or all of rr, RR, QQ, ee, and any necessary fundamental constants. iii. Assume the electron starts at rest at r=2Rr = 2R. Determine the speed of the electron when it passes through the center in terms of any or all of RR, QQ, ee, and any necessary fundamental constants. b. Accelerating charges radiate. The total power PP radiated by charge qq with acceleration aa is given by P=CξanP = C\xi a^n where CC is a dimensionless numerical constant (which is equal to 1/6π1/6\pi), ξ\xi is a physical constant that is a function only of the charge qq, the speed of light cc, and the permittivity of free space ϵ0\epsilon_0, and nn is a dimensionless constant. Determine ξ\xi and nn. c. Consider the electron in the first part, except now take into account radiation. Assume that the orbit remains circular and the orbital radius rr changes by an amount ∣Δr∣≪r|\Delta r| \ll r. i. Consider a circular orbit for the electron where r<Rr < R. Determine the change in the orbital radius Δr\Delta r during one orbit in terms of any or all of rr, RR, QQ, ee, and any necessary fundamental constants. Be very specific about the sign of Δr\Delta r. ii. Consider a circular orbit for the electron where r>Rr > R. Determine the change in the orbital radius Δr\Delta r during one orbit in terms of any or all rr, RR, QQ, ee, and any necessary fundamental constants. Be very specific about the sign of Δr\Delta r.

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