USAPhO 2008, Полуфинал — Задача 3. Question A3

AAPT AIP UNITED STATES PHYSICS TEAM 2008 — Semifinal Exam · 25 т.

Important Instructions for the Exam Supervisor

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  • This examination consists of three parts.
  • Part A has four questions and is allowed 90 minutes.
  • Part B has two questions and is allowed 90 minutes.
  • Part C has one question and is allowed 20 minutes. The answer for Part C will not be used for team selection, but will be used for special recognition from the Optical Society of America.
  • The first page that follows is a cover sheet. Examinees may keep the cover sheet for all three parts of the exam.
  • The three parts are then identified by the center header on each page. Examinees are only allowed to do one part at a time, and may not work on other parts, even if they have time remaining.
  • Allow 90 minutes to complete Part A. Do not let students look at Part B or Part C. Collect the answers to Part A before allowing the examinee to begin Part B. Examinees are allowed a 10 to 15 minutes break between parts A and B.
  • Allow 90 minutes to complete Part B. Do not let students look at Part C or go back to Part A. Collect the answers to part B before allowing the examinee to begin Part C. Examinees are allowed a 10 to 15 minutes break between Parts B and C.
  • Allow 20 minutes to complete Part C. This part is optional; scores on Part C will not be used to select the US Team. Examinees may not go back to Part A or B.
  • Ideally the test supervisor will divide the question paper into 4 parts: the cover sheet (page 2), Part A (pages 3-7), Part B (pages 8-10), and Part C (page 11). Examinees should be provided the parts individually, although they may keep the cover sheet.
  • The supervisor must collect all examination questions, including the cover sheet, at the end of the exam, as well as any scratch paper used by the examinees. Examinees may not take the exam questions. The examination questions may be returned to the students after March 31, 2008.
  • Examinees are allowed calculators, but they may not use symbolic math, programming, or graphic features of these calculators. Calculators may not be shared and their memory must be cleared of data and programs. Cell phones, PDA's or cameras may not be used during the exam or while the exam papers are present. Examinees may not use any tables, books, or collections of formulas.
  • Please provide the examinees with graph paper for Part A.
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. Each question is worth 25 points. Do not look at Parts B or C during this time.

  • After you have completed Part A you may take a break.

  • Then work Part B. You have 90 minutes to complete both problems. Each question is worth 50 points. Do not look at Parts A or C during this time.

  • Show all your work. Partial credit will be given. Do not write on the back of any page. Do not write anything that you wish graded on the question sheets.

  • Start each question on a new sheet of paper. Put your school ID number, your name, the question number and the page number/total pages for this problem, in the upper right hand corner of each page. For example,

    School ID #
    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.

  • Part C is an optional part of the test. You will be given 20 additional minutes to complete Part C. Your score on Part C will not affect the selection for the US Team, but can be used for special prizes and recognition to be awarded by the Optical Society of America.

  • In order to maintain exam security, do not communicate any information about the questions (or their answers/solutions) on this contest until after March 31, 2008.

Possibly Useful Information

Possibly Useful Information. You may use this sheet for all three parts of the exam.

g=9.8 N/kgg = 9.8\ \mathrm{N/kg} \qquad G=6.67×10−11 N⋅m2/kg2G = 6.67 \times 10^{-11}\ \mathrm{N \cdot m^2/kg^2}

k=1/4πϵ0=8.99×109 N⋅m2/C2k = 1/4\pi\epsilon_0 = 8.99 \times 10^{9}\ \mathrm{N \cdot m^2/C^2} \qquad km=μ0/4π=10−7 T⋅m/Ak_\mathrm{m} = \mu_0/4\pi = 10^{-7}\ \mathrm{T \cdot m/A}

c=3.00×108 m/sc = 3.00 \times 10^{8}\ \mathrm{m/s} \qquad kB=1.38×10−23 J/Kk_\mathrm{B} = 1.38 \times 10^{-23}\ \mathrm{J/K}

NA=6.02×1023 (mol)−1N_\mathrm{A} = 6.02 \times 10^{23}\ (\mathrm{mol})^{-1} \qquad R=NAkB=8.31 J/(mol⋅K)R = N_\mathrm{A} k_\mathrm{B} = 8.31\ \mathrm{J/(mol \cdot K)}

σ=5.67×10−8 J/(s⋅m2⋅K4)\sigma = 5.67 \times 10^{-8}\ \mathrm{J/(s \cdot m^2 \cdot K^4)} \qquad e=1.602×10−19 Ce = 1.602 \times 10^{-19}\ \mathrm{C}

1eV=1.602×10−19 J1\mathrm{eV} = 1.602 \times 10^{-19}\ \mathrm{J} \qquad h=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}

me=9.109×10−31 kg=0.511 MeV/c2m_e = 9.109 \times 10^{-31}\ \mathrm{kg} = 0.511\ \mathrm{MeV/c^2} \qquad (1+x)n≈1+nx(1+x)^n \approx 1 + nx for ∣x∣≪1|x| \ll 1

sin⁡θ≈θ−16θ3\sin\theta \approx \theta - \frac{1}{6}\theta^3 for ∣θ∣≪1|\theta| \ll 1 \qquad cos⁡θ≈1−12θ2\cos\theta \approx 1 - \frac{1}{2}\theta^2 for ∣θ∣≪1|\theta| \ll 1

Условие

A certain planet of radius RR is composed of a uniform material that, through radioactive decay, generates a net power PP. This results in a temperature differential between the inside and outside of the planet as heat is transferred from the interior to the surface.

The rate of heat transfer is governed by the thermal conductivity. The thermal conductivity of a material is a measure of how quickly heat flows through that material in response to a temperature gradient. Specifically, consider a thin slab of material of area AA and thickness Δx\Delta x where one surface is hotter than the other by an amount ΔT\Delta T. Suppose that an amount of heat ΔQ\Delta Q flows through the slab in a time Δt\Delta t. The thermal conductivity kk of the material is then

k=ΔQΔt1AΔxΔT.k = \frac{\Delta Q}{\Delta t}\frac{1}{A}\frac{\Delta x}{\Delta T}.

It is found that kk is approximately constant for many materials; assume that it is constant for the planet.

For the following assume that the planet is in a steady state; temperature might depend on position, but does not depend on time.

a. Find an expression for the temperature of the surface of the planet assuming blackbody radiation, an emissivity of 1, and no radiation incident on the planet surface. You may express your answer in terms of any of the above variables and the Stephan-Boltzmann constant σ\sigma.

b. Find an expression for the temperature difference between the surface of the planet and the center of the planet. You may express your answer in terms of any of the above variables; you do not need to answer part (a) to be able to answer this part.

Отговори

Решение


Оригинал в Архива: olympiad_2008_semi-final.pdf · официални решения: USAPhO-2008-Solutions.pdf