USAPhO 2005, Полуфинал — B1

2005 Semi-Final Exam · 50 т.

2005 Semi-Final Exam — Instructions

AAPT / AIP — United States Physics Team 2005.

DO NOT OPEN THIS TEST UNTIL YOU ARE TOLD TO BEGIN

  • Work Part A first. You have 90 minutes to complete all four problems.
  • After you have completed Part A, you may take a break.
  • Then work Part B. You have 90 minutes to complete both problems.
  • Show all your work. Partial credit will be given.
  • Start each question on a new sheet of paper. Be sure to put your name in the upper right-hand corner of each page, along with the question number and the page number/total pages for this problem. For example: Doe, Jamie; A1 – 1/3.
  • A hand-held calculator may be used. Its memory must be cleared of data and programs. You may use only the basic functions found on a simple scientific calculator. Calculators may not be shared. Cell phones, PDA’s, or cameras may not be used during the exam or while the exam papers are present. You may not use any tables, books, or collections of formulas.
  • Questions with the same point value are not necessarily of the same difficulty.
  • Do not discuss the contents of this exam with anyone until after the submission deadline.
  • Good luck!

Possibly Useful Information

QuantityValue
Gravitational field at the Earth’s surfaceg=9.8g=9.8 N/kg
Newton’s gravitational constantG=6.67×10−11G=6.67\times10^{-11} N·m2^2/kg2^2
Coulomb’s constantk=1/4πϵ0=8.99×109k=1/4\pi\epsilon_0=8.99\times10^9 N·m2^2/C2^2
Biot-Savart constantkm=μ0/4π=10−7k_m=\mu_0/4\pi=10^{-7} T·m/A
Speed of light in a vacuumc=3.00×108c=3.00\times10^8 m/s
Boltzmann’s constantkB=1.38×10−23k_B=1.38\times10^{-23} J/K
Avogadro’s numberNA=6.02×1023N_A=6.02\times10^{23} (mol)−1^{-1}
Ideal gas constantR=NAkB=8.31R=N_Ak_B=8.31 J/(mol·K)
Stefan-Boltzmann constantσ=5.67×10−8\sigma=5.67\times10^{-8} J/(s·m2^2·K4^4)
Elementary chargee=1.602×10−19e=1.602\times10^{-19} C
1 electron volt1 eV=1.602×10−191\text{ eV}=1.602\times10^{-19} J
Planck’s constanth=6.63×10−34 J⋅s=4.14×10−15 eV⋅sh=6.63\times10^{-34}\text{ J}\cdot\text{s}=4.14\times10^{-15}\text{ eV}\cdot\text{s}
Electron massm=9.109×10−31 kg=0.511 MeV/c2m=9.109\times10^{-31}\text{ kg}=0.511\text{ MeV}/c^2
Binomial expansion(1+x)n≈1+nx(1+x)^n\approx1+nx for ∣x∣≪1\lvert x\rvert\ll1
Small angle approximationssin⁡θ≈θ\sin\theta\approx\theta, cos⁡θ≈1−12θ2\cos\theta\approx1-\tfrac12\theta^2

Copyright © 2005, American Association of Physics Teachers

Условие

A length of wire is formed into a ring of radius bb and total charge QQ that is distributed uniformly around the ring. The ring is in the xx-yy plane and centered on the origin as shown in the accompanying diagram. i^\hat i, j^\hat j, and k^\hat k are unit vectors in the xx, yy, and zz directions respectively. Assume the potential vanishes at infinity.

Uniformly charged ringQ radiusb in xyplane with zaxis and unit vectorsi,j,k.

a.–b.

a. Find the field at any point on the zz axis. [7 т.]

b. Find the potential at any point on the zz axis. [5 т.]

c.–e.

A point charge with mass mm and charge −q-q is placed at z=z0z=z_0 where z0≪bz_0\ll b and released from rest at t=0t=0. Ignore any effects due to radiation.

c. Find the potential energy of the system as a function of zz, the position of the charge. Expand this potential energy function about the origin for ∣z∣≤z0\lvert z\rvert\le z_0. Keep only terms to lowest non-zero order in zz. [10 т.]

d. Find the speed of the charge as it passes through the origin. [5 т.]

e. Find the velocity of the charge as a function of time. [8 т.]

f.–g.

The point charge is removed and the ring is set into rotation about the zz-axis with angular velocity ω⃗=ωk^\vec\omega=\omega\hat k. Ignore any effects due to radiation.

f. Find the magnetic field due to the rotating ring at any point along the zz-axis. [10 т.]

g. A second point charge with mass mm and charge −q-q is placed at z=z0z=z_0 where z0≪bz_0\ll b and released from rest. What is the magnetic force on the charge as it passes through the origin? [5 т.]

Решение


Оригинал в Архива: Semifinal 2005.pdf · официални решения: Semifinal 2005 Solutions.pdf