USAPhO 2004, Полуфинал — Задача 5. B1

AAPT UNITED STATES PHYSICS TEAM AIP 2004 — 2004 Semi-Final Exam · 50 т.

Указания

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
Gravitational field at the Earth’s surfaceg=9.8 N/kgg = 9.8\ \mathrm{N/kg}
Newton’s gravitational constantG=6.67×10−11 N⋅m2/kg2G = 6.67 \times 10^{-11}\ \mathrm{N\cdot m^2/kg^2}
Coulomb’s constantk=1/4πε0=8.99×109 N⋅m2/C2k = 1/4\pi\varepsilon_0 = 8.99 \times 10^{9}\ \mathrm{N\cdot m^2/C^2}
Biot-Savart constantkm=μ0/4π=10−7 T⋅m/Ak_\mathrm{m} = \mu_0/4\pi = 10^{-7}\ \mathrm{T\cdot m/A}
Speed of light in a vacuumc=3.00×108 m/sc = 3.00 \times 10^{8}\ \mathrm{m/s}
Boltzmann’s constantkB=1.38×10−23 J/Kk_\mathrm{B} = 1.38 \times 10^{-23}\ \mathrm{J/K}
Avogadro’s numberNA=6.02×1023 (mol)−1N_\mathrm{A} = 6.02 \times 10^{23}\ \mathrm{(mol)^{-1}}
Ideal gas constantR=NAkB=8.31 J/(mol⋅K)R = N_\mathrm{A}k_\mathrm{B} = 8.31\ \mathrm{J/(mol\cdot K)}
Stefan-Boltzmann constantσ=5.67×10−8 J/(s⋅m2⋅K4)\sigma = 5.67 \times 10^{-8}\ \mathrm{J/(s\cdot m^2\cdot K^4)}
Elementary chargee=1.602×10−19 Ce = 1.602 \times 10^{-19}\ \mathrm{C}
1 electron volt1 eV=1.602×10−19 J1\ \mathrm{eV} = 1.602 \times 10^{-19}\ \mathrm{J}
Planck’s constanth=6.63×10−34 J⋅s=4.14×10−15 eV⋅sh = 6.63 \times 10^{-34}\ \mathrm{J\cdot s} = 4.14 \times 10^{-15}\ \mathrm{eV\cdot s}
Electron massm=9.109×10−31 kg=0.511 MeV/c2m = 9.109 \times 10^{-31}\ \mathrm{kg} = 0.511\ \mathrm{MeV/c^2}
Binomial expansion(1+x)n≈1+nx(1 + x)^n \approx 1 + nx for ∣x∣≪1\lvert x\rvert \ll 1
Small angle approximationssin⁡θ≈θ\sin\theta \approx \theta, cos⁡θ≈1−12θ2\cos\theta \approx 1 - \frac{1}{2}\theta^2

Copyright © 2004, American Association of Physics Teachers

Условие

a. In 1913, Niels Bohr first derived a formula for the energy levels of the hydrogen atom. He postulated that the single electron orbited a very massive proton under the influence of the electrostatic force and that the circular electron orbits had quantized angular momentum

L=nℏ=nh2πL = n\hbar = n\frac{h}{2\pi}

where n=1,2,3,…n = 1, 2, 3, \ldots and hh is Planck’s constant. These postulates gave rise to discrete values of the electron’s total energy EnE_n. Derive these Bohr Model energy levels. Express your answer in terms of Coulomb’s constant kk, the electron mass mm, the electron charge ee, ℏ\hbar, and nn. If done correctly, your answer should evaluate to

En=−2.18×10−18 Jn2=−13.6 eVn2.E_n = -\frac{2.18 \times 10^{-18}\ \mathrm{J}}{n^2} = -\frac{13.6\ \mathrm{eV}}{n^2}.

[20 т.]

b. In a hypothetical modern day experiment, electrons are accelerated from rest through a potential VV into a cloud of cold atomic hydrogen (Figure 1-1). A series of plates with aligned holes select a beam of scattered electrons moving perpendicular to the plates. Immediately beyond the final plate, the electrons enter a uniform magnetic field BB perpendicular to the beam; they curve and strike a piece of film mounted on the final plate.

Figure 1-1: an electron gun with accelerating potential V sends electrons e- into a grey cloud H of hydrogen; scattered electrons pass through a series of parallel plates with aligned holes and curve in a magnetic field B (pointing out of the page) onto the final plate.
Figure 1-1
Figure 1-2: the developed film showing the entrance hole (open circle, labelled “hole through which electrons entered”) and a row of spots; the distances from the hole to the two most distant spots are marked 3.980 cm and 9.491 cm.
Figure 1-2

When the film is developed, a series of spots is observed (Figure 1-2). The distances between the hole and the two most distant spots are measured. You may assume that the film is large enough to have intercepted all of the electrons, i.e. that there are no spots farther from the hole than those shown. The number of spots shown is not necessarily accurate.

Make the approximation that the mass of the hydrogen atom is much larger than the mass of the electron. Assume that each electron scatters off only one atom, which is initially in the ground state (lowest energy state) and has negligible thermal velocity.

Determine:

i. The magnitude of the magnetic field BB. [10 т.]

ii. The magnitude of the accelerating potential VV. [10 т.]

iii. The total number of spots on the film. [10 т.]

Отговори

Решение


Оригинал в Архива: Semifinal 2004.pdf · официални решения: Semifinal 2004 Solutions.pdf