OPhO 2024, Теория — Задача 1. Penned Particles

2024 Online Physics Olympiad: Invitational Contest — Theoretical Examination · 35 т.

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Instructions for Theoretical Exam

The theoretical examination consists of 4 long answer questions over 2 full days from August 30, 12:00AM UTC to September 1, 12:00 AM UTC.

  • The team leader should submit their final solution document in this google form. We don’t anticipate a tie, but in the rare circumstance that there is one, the time you submit will be used to break it.

  • If you wish to request a clarification, please use this form. To see all clarifications, view this document.

  • Participants are given a Google Form where they are allowed to submit up 50 MB of data for each problem solution. It is recommended that participants write their solutions in LaTeX. However, handwritten solutions (or a combination of both) are accepted too. If participants have more than one photo of a handwritten solution (jpg, png, etc), it is required to organize them in the correct order in a pdf before submitting. If you wish a premade LaTeX template, we have made one for you here.

  • Since each question is a long answer response, participants will be judged on the quality of your work. To receive full points, participants need to show their work, including deriving equations. As a general rule of thumb, any common equations (such as the ones in the IPhO formula sheet) can be cited without proof.

  • Remember to state any approximations made and which system of equations were solved after every step. Explicitly showing every step of algebra is not necessary. Participants may leave all final answers in symbolic form (in terms of variables) unless otherwise specified. Be sure to state all assumptions.

Problems

  • T1: Penned Particles
  • T2: Bouncy Bubble
  • T3: Stellar Shaping
  • T4: Hot Solids
List of Constants
  • Proton mass, mp=1.67⋅10−27 kgm_p=1.67\cdot10^{-27}\ \mathrm{kg}
  • Neutron mass, mn=1.67⋅10−27 kgm_n=1.67\cdot10^{-27}\ \mathrm{kg}
  • Electron mass, me=9.11⋅10−31 kgm_e=9.11\cdot10^{-31}\ \mathrm{kg}
  • Avogadro’s constant, N0=6.02⋅1023 mol−1N_0=6.02\cdot10^{23}\ \mathrm{mol^{-1}}
  • Universal gas constant, R=8.31 J/(mol⋅K)R=8.31\ \mathrm{J/(mol\cdot K)}
  • Boltzmann’s constant, kB=1.38⋅10−23 J/Kk_B=1.38\cdot10^{-23}\ \mathrm{J/K}
  • Electron charge magnitude, e=1.60⋅10−19 Ce=1.60\cdot10^{-19}\ \mathrm C
  • 1 electron volt, 1 eV=1.60⋅10−19 J1\ \mathrm{eV}=1.60\cdot10^{-19}\ \mathrm J
  • Speed of light, c=3.00⋅108 m/sc=3.00\cdot10^8\ \mathrm{m/s}
  • Universal Gravitational constant, G=6.67⋅10−11 (N⋅m2)/kg2G=6.67\cdot10^{-11}\ \mathrm{(N\cdot m^2)/kg^2}
  • Solar Mass, M⊙=1.988⋅1030 kgM_\odot=1.988\cdot10^{30}\ \mathrm{kg}
  • Acceleration due to gravity, g=9.8 m/s2g=9.8\ \mathrm{m/s^2}
  • 1 unified atomic mass unit, 1 u=1.66⋅10−27 kg=931 MeV/c21\ \mathrm u=1.66\cdot10^{-27}\ \mathrm{kg}=931\ \mathrm{MeV}/c^2
  • Planck’s constant, h=6.63⋅10−34 J⋅s=4.41⋅10−15 eV⋅sh=6.63\cdot10^{-34}\ \mathrm{J\cdot s}=4.41\cdot10^{-15}\ \mathrm{eV\cdot s}
  • Permittivity of free space, ϵ0=8.85⋅10−12 C2/(N⋅m2)\epsilon_0=8.85\cdot10^{-12}\ \mathrm{C^2/(N\cdot m^2)}
  • Coulomb’s law constant, k=14πϵ0=8.99⋅109 (N⋅m2)/C2k=\frac1{4\pi\epsilon_0}=8.99\cdot10^9\ \mathrm{(N\cdot m^2)/C^2}
  • Permeability of free space, μ0=4π⋅10−7 T⋅m/A\mu_0=4\pi\cdot10^{-7}\ \mathrm{T\cdot m/A}
  • Magnetic constant, μ04π=1⋅10−7 (T⋅m)/A\frac{\mu_0}{4\pi}=1\cdot10^{-7}\ \mathrm{(T\cdot m)/A}
  • 1 atmospheric pressure, 1 atm=1.01⋅105 N/m2=1.01⋅105 Pa1\ \mathrm{atm}=1.01\cdot10^5\ \mathrm{N/m^2}=1.01\cdot10^5\ \mathrm{Pa}
  • Wien’s displacement constant, b=2.9⋅10−3 m⋅Kb=2.9\cdot10^{-3}\ \mathrm{m\cdot K}
  • Stefan-Boltzmann constant, σ=5.67⋅10−8 W/m2/K4\sigma=5.67\cdot10^{-8}\ \mathrm{W/m^2/K^4}

Условие

A Penning trap is a device used to store charged particles using static magnetic and electric fields. In this problem we will investigate the motion of an ion inside the trap.

1.1

a. The trap is a cylinder, parallel to the zz-axis, with the origin at the center. Inside, the electric potential is V=V0z2−r22d2V=V_0\frac{z^2-r^2}{2d^2}, where dd is the characteristic dimension of the trap. In order to generate the quadrupole field inside, there are two sets of electrodes: two endcaps and the ring electrode, which are held at potential difference V0V_0, and are solids of revolution. Refer to part (e) for a diagram. Let the minimum distance between endcaps be 2z02z_0, and the smallest inside diameter of the ring be 2r02r_0.

  • Take a cross section parallel to the zz-axis through the origin. What are the equations of the cross section of the ring and endcap electrodes?
  • Express dd in terms of r0r_0 and z0z_0.

b. The magnetic field B=B0z^\mathbf B=B_0\hat z is homogeneous inside the trap. Suppose we have a particle with charge qq and mass mm. Assume its speed is nonrelativistic, and neglect energy loss from radiation. Throughout the rest of the problem, assume qq is positive.

  • The zz-axis motion is simple harmonic. Find the angular frequency ωz\omega_z.
  • Write the differential equation for the motion in the xyxy-plane.
  • Suppose ωz=0\omega_z=0. Solve the differential equation, and find the angular frequency of the motion ωc\omega_c. This is the cyclotron frequency.

Typically, ωc≫ωz\omega_c\gg\omega_z. Assume this for the rest of the problem.

c. The motion of the electron in the xyxy-plane consists of two separate uniform circular motions overlaid on top of each other. One is the cyclotron motion and the other is the magnetron motion. Find expressions for the angular frequencies of the cyclotron motion and the magnetron motion, in terms of ωz\omega_z and ωc\omega_c.

1.2

d. We will now consider the effects of radiation. Typically, the magnetron motion has a much lower frequency than the cyclotron motion, so the decay of the magnetron motion is negligible. The power radiated by an accelerating particle is:

P=q2a26πϵ0c3.P=\frac{q^2a^2}{6\pi\epsilon_0c^3}.
  • The energy of the orbit decays as e−t/γce^{-t/\gamma_c}. Find γc\gamma_c.
  • Now consider the radiation damping of the axial motion. The energy of the oscillation decays as e−t/γze^{-t/\gamma_z}. Find γz\gamma_z.

e. For an electron at typical ωc\omega_c, γc\gamma_c is quite small, allowing for easy damping. However, γz\gamma_z is much larger, and for a proton, radiation damping is insignificant. In order to cool large particles, a circuit is used instead. We first consider axial damping.

The oscillations of the ion induce image charges in the electrode, which can be interpreted as a current II. See the following circuit:

Complete native hand-drawn Penning trap circuit: both endcaps, ring, ion, z-axis direction, image-current arrow, resistor R and full connecting wires.

You may ignore the quadrupole potential in this part.

  • There will be a potential difference of IRIR between the endcap and the ring (as well as the other endcap). This will produce an electric field Ez^E\hat z proportional to II inside the trap. Find EE, up to a constant factor κ\kappa, which depends on the geometry of the electrodes. Hint: if the endcaps are infinite flat planes, κ\kappa is equal to 1.
  • Consider the power lost through the resistor. Use this to derive the force on the ion, f=−mζz˙f=-m\zeta\dot z. Write an expression for ζ\zeta.

f. To conclude, we will consider how to cool the magnetron motion (decrease its radius).

  • Find the total energy of the magnetron motion. Assume z=0z=0.

The process works as follows. We shine photons of energy ℏ(ωz+ωm)\hbar(\omega_z+\omega_m), which interact with the ion. Let the quantum numbers of the zz motion and the magnetron motion be kk and ll respectively. Then, the cooling transition is from (k,l)→(k+1,l−1)(k,l)\to(k+1,l-1), and the heating transition is from (k,l)→(k−1,l+1)(k,l)\to(k-1,l+1). Using quantum mechanics, we can derive that these happen at rates proportional to (k+1)l(k+1)l and k(l+1)k(l+1) respectively. The magnetron motion will be cooled until l=kl=k, at which point it will be in equilibrium, and there is no long term change in temperature.

  • We will now derive the equilibrium energy of the magnetron motion. Assume that at equilibrium, the axial and magnetron motions are at temperatures TzT_z and TmT_m respectively. As we continue to shine photons, consider the change in entropy. Use this to derive TmT_m in terms of ωm\omega_m, ωz\omega_z, and TzT_z.

Published organizer clarifications — separately quoted from the 2024 OPhO Clarifications document.

T1 - Penned Particles

This problem’s last update: 8/31 16:15 GMT

We have been made aware that a valid potential should be proportional to (2z2−r2)(2z^2-r^2), and that (z2−r2)(z^2-r^2) is unphysical. This does not change anything in the problem except some numerical coefficients. You may solve the problem by consistently choosing either of:

  1. V=V0(z2−r2)/2d2V=V_0(z^2-r^2)/2d^2
  2. V=V0(2z2−r2)/2d2V=V_0(2z^2-r^2)/2d^2

(a) In the potential function, r and z are coordinates. r2=x2+y2r^2=x^2+y^2.

(b) You may answer using any of r0r_0, z0z_0, and dd.

(c)

(d) You may use whatever quantities you deem necessary in the expressions for gamma. The formula for power from an accelerating charge should have an extra factor of pi in the denominator; we won’t penalize you if you use the formula as given in the original pdf. The formula for power is now correct in the new pdf.

(e) The expression for zeta is meant to contain kappa. You may use any constant quantity in your expression.

(f) You are supposed to find the energy in terms of the radius of the orbit. The first task is to solve for the energy, the second task is to solve for TmT_m. When it says ℏ(wz+wm)\hbar(w_z+w_m), it is supposed to be ωz\omega_z and ωm\omega_m. We’ve fixed this in the problem pdf.

Решение


Оригинал в Архива: theory.pdf · официални решения: theory_sol.pdf · допълнителни данни: Clarifications.pdf