Waves and Modern Physics 203-SN3-RE • CEGEP, Montreal

Corrected practice final exam: waves, optics and modern physics (203-SN3-RE, formerly 203-NYC)

A chapter set announces its topic: you know you are doing wave optics, and half the work is already done. A final exam does not announce anything, and that is the only difference that matters. This practice final covers the whole Waves and Modern Physics course, 203-SN3-RE (formerly 203-NYC), as it is taught in CEGEP physics: oscillations and mechanical waves, sound, geometric and wave optics, and modern physics. It follows the former 203-NYC course, so it keeps geometric optics and leaves out the heat and climate block of the revised syllabus.

Format of the paper: 12 exercises, 100 marks, 3 hours, four parts of 25 marks each. Calculator allowed. Part A covers oscillations and mechanical waves: simple harmonic motion of a mass-spring system and how its energy is shared, a damped pendulum, a travelling wave on a string and the power it carries. Part B covers sound: sound intensity level in decibels, the Doppler effect and the Mach cone, open and closed pipes, beats. Part C covers optics: a converging lens, total internal reflection, a prism at minimum deviation and dispersion, Young's double slit, the diffraction grating and single-slit diffraction. Part D covers modern physics: the photoelectric effect, the Bohr model, the de Broglie wavelength and the Heisenberg uncertainty principle.

Three questions deserve a warning. Exercise 5 has you work out the same Doppler situation twice, once with a moving source and once with a moving observer, and the two results differ: there is no symmetry, because air is a privileged medium. Exercise 9 asks for the missing orders of a double-slit setup, where the diffraction envelope erases fringes that do exist. And exercise 11 ends on a velocity uncertainty larger than the velocity itself, which finally rules out the picture of the electron on its orbit.

The other traps of the course come back in the solutions: an amplitude cut in half that leaves a quarter of the energy, not half (exercise 2), the transverse velocity of a point of the string mistaken for the wave speed (exercise 3), and the five false statements of exercise 12, one for each part of the course.

12 corrected exercises • 100 points • 180 minutes

This chapter is part of 203-SN3-RE, every chapter with its set and sheet

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Course recap

  • • SHM: ω=km\omega=\sqrt{\frac{k}{m}} for a spring, T=2πLgT=2\pi\sqrt{\frac{L}{g}} for a pendulum, with no mass in it. vmax⁡=ωAv_{\max}=\omega A, amax⁡=ω2Aa_{\max}=\omega^{2}A, E=12kA2E=\frac{1}{2}kA^{2}.
  • • Energy and amplitude: the energy of any oscillator or wave varies as A2A^{2}. Half the amplitude therefore means a quarter of the energy, never half.
  • • Wave on a string: v=Fμv=\sqrt{\frac{F}{\mu}} depends only on the medium. Do not confuse the wave speed with the transverse velocity ωA\omega A of a piece of the string.
  • • Decibels: L=10log⁡II0L=10\log\frac{I}{I_{0}}. Doubling the intensity adds 3 dB3\ \mathrm{dB}, multiplying it by ten adds 1010, and multiplying the distance by ten removes 2020.
  • • Doppler: f′=fvv−vsf'=f\frac{v}{v-v_{s}} for a moving source, f′=fv+vovf'=f\frac{v+v_{o}}{v} for a moving observer. The two formulas are not equivalent.
  • • Pipes: open at both ends, f1=v2Lf_{1}=\frac{v}{2L} and all the harmonics; closed at one end, f1=v4Lf_{1}=\frac{v}{4L} and only the odd harmonics. And v=331+0.6θv=331+0.6\theta.
  • • Lenses: 1f=1do+1di\frac{1}{f}=\frac{1}{d_{o}}+\frac{1}{d_{i}} and m=−didom=-\frac{d_{i}}{d_{o}}. The image is real if di>0d_{i}>0, virtual if di<0d_{i}<0. An object at the focal point gives an image at infinity.
  • • Prism: r+r′=Ar+r'=A, and at minimum deviation r=A2r=\frac{A}{2} with Dmin⁡=2i−AD_{\min}=2i-A. The index grows as λ\lambda decreases, so blue is deviated the most.
  • • Interference and diffraction: fringe spacing λDd\frac{\lambda D}{d}, grating sin⁡θ=mλd\sin\theta=\frac{m\lambda}{d}, first minimum of a single slit sin⁡θ=λa\sin\theta=\frac{\lambda}{a}. Orders are missing when m=ndam=n\frac{d}{a} is an integer.
  • • Photon and matter: E (eV)=1240λ (nm)E\ \left(\mathrm{eV}\right)=\frac{1240}{\lambda\ \left(\mathrm{nm}\right)}, Ek,max⁡=E−WE_{k,\max}=E-W, λdB=hmv\lambda_{\mathrm{dB}}=\frac{h}{mv}, En=−13.6n2 eVE_{n}=-\frac{13.6}{n^{2}}\ \mathrm{eV}. The intensity sets the NUMBER of electrons, the frequency sets their ENERGY.

Part A: Oscillations and mechanical waves (/25)

Exercise 1: The mass-spring system and how its energy is shared

A block of mass m=0.25 kgm=0.25\ \mathrm{kg} is attached to a spring of constant k=100 N/mk=100\ \mathrm{N/m} and oscillates without friction with an amplitude A=0.080 mA=0.080\ \mathrm{m}.

The graph below gives the elastic potential energy, the kinetic energy and the total mechanical energy as functions of position.

−0.1−0.050.050.10.10.20.30.4E = 0.32 JEpEkx (m)
  • a) Calculate the angular frequency, the period and the frequency of the oscillations.
  • b) Calculate the maximum speed and the maximum acceleration of the block.
  • c) Calculate the total mechanical energy, and check it against the graph.
  • d) At x=A2x=\dfrac{A}{2}, calculate the potential energy, the kinetic energy and the speed of the block.
  • e) Using the graph, then by calculation, find the position where the two energies are equal.

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  • a) ω=20.0\omega=20.0 rad/s, T=0.314T=0.314 s, f=3.18f=3.18 Hz
  • b) vmax=1.60v_{max}=1.60 m/s at equilibrium, amax=32.0a_{max}=32.0 m/s² at the extremes
  • c) E=12kA2=0.32E=\frac{1}{2}kA^{2}=0.32 J, constant
  • d) Ep=0.080E_{p}=0.080 J, Ek=0.24E_{k}=0.24 J, v=1.39v=1.39 m/s: a quarter and three quarters
  • e) x=A2=0.0566x=\dfrac{A}{\sqrt{2}}=0.0566 m, that is 71 %71\,\% of the amplitude
a)

ω=km=1000.25=400=20.0 rad/s\omega=\sqrt{\dfrac{k}{m}}=\sqrt{\dfrac{100}{0.25}}=\sqrt{400}=20.0\ \mathrm{rad/s}. Then T=2πω=2π20=0.314 sT=\dfrac{2\pi}{\omega}=\dfrac{2\pi}{20}=0.314\ \mathrm{s} and f=1T=3.18 Hzf=\dfrac{1}{T}=3.18\ \mathrm{Hz}.

b)

vmax⁡=ωA=20.0×0.080=1.60 m/sv_{\max}=\omega A=20.0\times 0.080=1.60\ \mathrm{m/s}, reached when passing through the equilibrium position. And amax⁡=ω2A=400×0.080=32.0 m/s2a_{\max}=\omega^{2}A=400\times 0.080=32.0\ \mathrm{m/s^{2}}, reached at the extreme positions, where the restoring force is greatest.

c)

E=12kA2=0.5×100×0.0802=0.32 JE=\dfrac{1}{2}kA^{2}=0.5\times 100\times 0.080^{2}=0.32\ \mathrm{J}. The graph does show the horizontal line at 0.32 J0.32\ \mathrm{J}: the total energy is constant, which reflects the absence of friction.

d)

At x=0.040 mx=0.040\ \mathrm{m}: Ep=12kx2=0.5×100×0.0402=0.080 JE_{p}=\dfrac{1}{2}kx^{2}=0.5\times 100\times 0.040^{2}=0.080\ \mathrm{J}, which is a quarter of the total energy, since EpE_{p} varies as the square of xx. So Ek=0.32−0.080=0.24 JE_{k}=0.32-0.080=0.24\ \mathrm{J}, three quarters. The speed follows from v=2Ekm=0.480.25=1.39 m/sv=\sqrt{\dfrac{2E_{k}}{m}}=\sqrt{\dfrac{0.48}{0.25}}=1.39\ \mathrm{m/s}, which the formula v=ωA2−x2=200.0048=1.39 m/sv=\omega\sqrt{A^{2}-x^{2}}=20\sqrt{0.0048}=1.39\ \mathrm{m/s} confirms. At half amplitude, the block therefore still has 8787 percent of its maximum speed.

e)

On the graph, the two curves cross at the two marked points, at 0.16 J0.16\ \mathrm{J}, which is half the total energy. By calculation: 12kx2=12kA2−12kx2\dfrac{1}{2}kx^{2}=\dfrac{1}{2}kA^{2}-\dfrac{1}{2}kx^{2} gives 2x2=A22x^{2}=A^{2}, so x=±A2=±0.0566 mx=\pm\dfrac{A}{\sqrt{2}}=\pm 0.0566\ \mathrm{m}. This is not at half amplitude: the energy is shared equally at about 7171 percent of the amplitude, because the potential energy is quadratic in xx, not linear.

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Exercise 2: The damped pendulum

A simple pendulum of length L=0.80 mL=0.80\ \mathrm{m} makes small oscillations, with g=9.81 m/s2g=9.81\ \mathrm{m/s^{2}}.

Because of air friction, its amplitude decays exponentially and is cut in half in 12 s12\ \mathrm{s}.

θg = 9.81 m/s²L = 0.80 m
  • a) Calculate the period of the pendulum. Does this period depend on the suspended mass or on the amplitude?
  • b) What length would give a period of exactly 2.0 s2.0\ \mathrm{s}, that is, a seconds pendulum?
  • c) The amplitude is written θmax⁡(t)=θ0 e−γt\theta_{\max}(t)=\theta_{0}\,\mathrm{e}^{-\gamma t}. Find γ\gamma.
  • d) After how long is the amplitude only 10 percent of its initial value? How many oscillations has the pendulum made by then?
  • e) In 12 s12\ \mathrm{s}, what fraction of its mechanical energy has the pendulum lost? Justify that it is not one half.

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  • a) T≈1.79T\approx 1.79 s, independent of the mass and of the amplitude
  • b) L=gπ2≈0.994L=\dfrac{g}{\pi^{2}}\approx 0.994 m
  • c) γ=ln⁡212≈5.78×10−2\gamma=\dfrac{\ln 2}{12}\approx 5.78\times 10^{-2} s⁻¹
  • d) t≈39.9t\approx 39.9 s, about 2222 oscillations
  • e) 75 %75\,\%: energy goes as the square of the amplitude
a)

T=2πLg=2π0.809.81=2π×0.2856=1.79 sT=2\pi\sqrt{\dfrac{L}{g}}=2\pi\sqrt{\dfrac{0.80}{9.81}}=2\pi\times 0.2856=1.79\ \mathrm{s}. This expression does not contain the mass: the period of a simple pendulum is independent of it, because the driving force and the inertia are both proportional to the mass. It is also independent of the amplitude, but only in the small-oscillation approximation, where sin⁡θ≈θ\sin\theta\approx\theta.

b)

From T=2πLgT=2\pi\sqrt{\dfrac{L}{g}} we get L=gT24π2=9.81×4.04π2=gπ2=0.994 mL=\dfrac{gT^{2}}{4\pi^{2}}=\dfrac{9.81\times 4.0}{4\pi^{2}}=\dfrac{g}{\pi^{2}}=0.994\ \mathrm{m}. A pendulum about one metre long therefore beats seconds, each swing in one direction lasting one second.

c)

The amplitude is divided by two in 12 s12\ \mathrm{s}, so e−12γ=12\mathrm{e}^{-12\gamma}=\dfrac{1}{2}, that is 12γ=ln⁡212\gamma=\ln 2 and γ=ln⁡212=5.78×10−2 s−1\gamma=\dfrac{\ln 2}{12}=5.78\times 10^{-2}\ \mathrm{s^{-1}}.

d)

Solve e−γt=0.10\mathrm{e}^{-\gamma t}=0.10, that is t=ln⁡10γ=2.3035.78×10−2=39.9 st=\dfrac{\ln 10}{\gamma}=\dfrac{2.303}{5.78\times 10^{-2}}=39.9\ \mathrm{s}. The number of oscillations is 39.91.79=22.2\dfrac{39.9}{1.79}=22.2, so about 22 complete oscillations. Note that the damping hardly changes the period: the pendulum swings at the same rhythm, and only its amplitude shrinks.

e)

The mechanical energy of an oscillator is proportional to the square of the amplitude. If the amplitude is divided by two, the energy is divided by four: a quarter remains, so the pendulum has lost three quarters of its energy, or 75 percent. It is not one half precisely because the relation is quadratic. The same reasoning explains why an amplitude down to 10 percent corresponds to an energy down to 1 percent.

051015202530354045-1-0.500.51t (s)θ / θ₀half at 12 s10% at 39.9 s
The amplitude follows the envelope θ0 e−γt\theta_{0}\,\mathrm{e}^{-\gamma t} (dashed orange): half at 1212 s, 10 %10\,\% at 39.939.9 s, about 2222 oscillations later. The period does not change: the oscillations stay regular under the envelope.

Exercise 3: A wave on a string, from tension to power

A string of linear mass density μ=0.020 kg/m\mu=0.020\ \mathrm{kg/m} is stretched under a force F=80 NF=80\ \mathrm{N}. A sinusoidal travelling wave of frequency f=120 Hzf=120\ \mathrm{Hz} and amplitude A=5.0 mmA=5.0\ \mathrm{mm} is sustained on it.

vibratorf = 120 Hz, A = 5.0 mmF = 80 Nμ = 0.020 kg/mx
  • a) Calculate the wave speed, then its wavelength.
  • b) Calculate the wave number and the angular frequency, then write the equation of the wave travelling in the direction of increasing xx.
  • c) Calculate the maximum transverse velocity of a point of the string and compare it with the wave speed. Are these two speeds of the same nature?
  • d) The average power carried is P=12μvω2A2P=\dfrac{1}{2}\mu v\omega^{2}A^{2}. Calculate it.
  • e) By what factor is the power multiplied if the tension of the string is doubled? And if the amplitude is doubled? Explain the difference.

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  • a) v=F/μ=63.2v=\sqrt{F/\mu}=63.2 m/s and λ=0.527\lambda=0.527 m
  • b) k=11.9k=11.9 rad/m, ω=754\omega=754 rad/s
  • c) v⊥,max=3.77v_{\perp,max}=3.77 m/s: the material, not the pattern
  • d) P≈8.99P\approx 8.99 W
  • e) 2\sqrt{2} for the tension, 44 for the amplitude: the exponents differ
a)

v=Fμ=800.020=4000=63.2 m/sv=\sqrt{\dfrac{F}{\mu}}=\sqrt{\dfrac{80}{0.020}}=\sqrt{4000}=63.2\ \mathrm{m/s}. The wavelength is λ=vf=63.2120=0.527 m\lambda=\dfrac{v}{f}=\dfrac{63.2}{120}=0.527\ \mathrm{m}. The wave speed depends only on the medium, tension and linear mass density, never on the source.

b)

k=2πλ=2π0.527=11.9 rad/mk=\dfrac{2\pi}{\lambda}=\dfrac{2\pi}{0.527}=11.9\ \mathrm{rad/m} and ω=2πf=2π×120=754 rad/s\omega=2\pi f=2\pi\times 120=754\ \mathrm{rad/s}. The equation is y(x,t)=5.0×10−3sin⁡(754t−11.9x)y(x, t)=5.0\times 10^{-3}\sin\left(754t-11.9x\right), in metres, the minus sign in front of xx expressing propagation toward increasing xx.

c)

The transverse velocity is ∂y∂t\dfrac{\partial y}{\partial t}, whose amplitude is v⊥max⁡=ωA=754×5.0×10−3=3.77 m/sv_{\perp\max}=\omega A=754\times 5.0\times 10^{-3}=3.77\ \mathrm{m/s}. It is well below the wave speed 63.2 m/s63.2\ \mathrm{m/s}, and above all it is of a completely different nature: the wave speed is the speed at which the pattern moves along the string, whereas the transverse velocity is that of a piece of material, perpendicular to the string. No material moves at 63.2 m/s63.2\ \mathrm{m/s}: it is the wave that advances, not the string.

d)

P=12×0.020×63.2×7542×(5.0×10−3)2=0.632×5.68×105×2.5×10−5=8.99 WP=\dfrac{1}{2}\times 0.020\times 63.2\times 754^{2}\times\left(5.0\times 10^{-3}\right)^{2}=0.632\times 5.68\times 10^{5}\times 2.5\times 10^{-5}=8.99\ \mathrm{W}.

e)

If the tension is doubled, v=Fμv=\sqrt{\dfrac{F}{\mu}} is multiplied by 2\sqrt{2}. Since PP is proportional to vv, at fixed frequency and amplitude, the power is multiplied by only 2≈1.41\sqrt{2}\approx 1.41. If the amplitude is doubled, PP being proportional to A2A^{2}, it is multiplied by 4. The difference comes from the exponent: the amplitude enters squared, the wave speed to the first power, and the wave speed itself depends on the tension only through a square root. To carry more power, working on the amplitude is therefore far more effective than tightening the string.

00.20.40.60.811.2-505x (m)y (mm)λ = 0.527 mA = 5.0 mmv = 63.2 m/s →v⊥ max = 3.77 m/s
The string at a given instant, y=−5.0sin⁡(11.9x)y=-5.0\sin(11.9x) in millimetres: two crests are separated by λ=0.527\lambda=0.527 m. The vertical axis is greatly stretched: 55 mm of amplitude for half a metre of wavelength. The purple point, where the string crosses zero, has the maximum transverse velocity, 3.773.77 m/s, while the pattern advances at 63.263.2 m/s.

Part B: Sound, intensity and the Doppler effect (/25)

Exercise 4: Decibels, distance and multiple sources

A point sound source emits uniformly in all directions. At 1.0 m1.0\ \mathrm{m} from the source, the measured sound intensity level is 90 dB90\ \mathrm{dB}.

Recall L=10log⁡II0L=10\log\dfrac{I}{I_{0}} with I0=1.0×10−12 W/m2I_{0}=1.0\times 10^{-12}\ \mathrm{W/m^{2}}.

90 dBL = ?point source1.0 m10 m
  • a) Calculate the sound intensity at 1.0 m1.0\ \mathrm{m}, then the total acoustic power emitted by the source.
  • b) Calculate the intensity and the sound level at 10 m10\ \mathrm{m}. By how many decibels has the level dropped?
  • c) A second identical source is added at the same place. What is the new level at 1.0 m1.0\ \mathrm{m}? And with ten identical sources?
  • d) The threshold of pain is 120 dB120\ \mathrm{dB}. At what distance from the single source is this threshold reached?
  • e) Explain why doubling the sound power does not double the level in decibels.

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  • a) I=1.0×10−3I=1.0\times 10^{-3} W/m² and P≈13P\approx 13 mW
  • b) 7070 dB: multiplying the distance by ten costs 2020 dB
  • c) 93.093.0 dB with two sources, 100100 dB with ten
  • d) r≈3.2r\approx 3.2 cm: hence the danger of earphones
  • e) The scale is logarithmic: doubling adds 10log⁡2≈310\log 2\approx 3 dB
a)

From L=90L=90 we get II0=109\dfrac{I}{I_{0}}=10^{9}, so I=10−12×109=1.0×10−3 W/m2I=10^{-12}\times 10^{9}=1.0\times 10^{-3}\ \mathrm{W/m^{2}}. The power crosses a sphere of radius 1.0 m1.0\ \mathrm{m}, so P=I×4πr2=1.0×10−3×4π=1.26×10−2 WP=I\times 4\pi r^{2}=1.0\times 10^{-3}\times 4\pi=1.26\times 10^{-2}\ \mathrm{W}. A source of only 13 milliwatts of acoustic power is therefore enough to produce 90 decibels at one metre.

b)

The intensity falls off as the inverse square of the distance: at 10 m10\ \mathrm{m} it is divided by 100100, so I=1.0×10−5 W/m2I=1.0\times 10^{-5}\ \mathrm{W/m^{2}}. The level is L=10log⁡(107)=70 dBL=10\log\left(10^{7}\right)=70\ \mathrm{dB}. It has therefore dropped by 20 dB20\ \mathrm{dB}: multiplying the distance by ten costs exactly 20 decibels, whatever the source.

c)

Two identical sources double the intensity, so L=10log⁡(2×109)=90+10log⁡2=93.0 dBL=10\log\left(2\times 10^{9}\right)=90+10\log 2=93.0\ \mathrm{dB}. With ten sources, the intensity is multiplied by ten and L=90+10=100 dBL=90+10=100\ \mathrm{dB}. Doubling the number of sources adds 3 decibels, multiplying it by ten adds 10.

d)

120 dB120\ \mathrm{dB} corresponds to I=1.0 W/m2I=1.0\ \mathrm{W/m^{2}}. Solve P4πr2=1.0\dfrac{P}{4\pi r^{2}}=1.0, that is r2=1.26×10−24π=1.0×10−3r^{2}=\dfrac{1.26\times 10^{-2}}{4\pi}=1.0\times 10^{-3}, hence r=3.2×10−2 mr=3.2\times 10^{-2}\ \mathrm{m}, about 3.2 cm3.2\ \mathrm{cm}. You would have to put your ear against the source, which explains the danger of earphones.

e)

Because the decibel scale is logarithmic, not proportional. The level measures the logarithm of the ratio of intensities: doubling the intensity adds 10log⁡2≈3 dB10\log 2\approx 3\ \mathrm{dB}, a constant amount, not a factor of two. This scale was chosen because the sensation of hearing roughly follows the logarithm of the intensity: a gain of 10 decibels, a factor of ten in intensity, is perceived as a sound about twice as loud.

48121620242832365060708090100110sound level (dB)distance (m)each doubling of distancecosts 6 dB, not 3intensity falls as 1/r², and 10 log(1/4) = −6 dB

Exercise 5: The Doppler effect and the Mach cone

The speed of sound in air is taken to be 343 m/s343\ \mathrm{m/s}. An ambulance sounds a siren of frequency 800 Hz800\ \mathrm{Hz} and travels at 25 m/s25\ \mathrm{m/s}.

The figure shows the shock cone of an aircraft flying at 500 m/s500\ \mathrm{m/s}.

μv = 500 m/sshock front
  • a) Calculate the frequency heard by a stationary pedestrian when the ambulance approaches, then when it moves away.
  • b) Calculate the difference between these two frequencies. Is this jump audible?
  • c) Swap the roles: the ambulance is stationary and the pedestrian travels at 25 m/s25\ \mathrm{m/s} toward it. Calculate the frequency heard and compare it with the result of part a).
  • d) Calculate the Mach number of the aircraft, then the half-angle at the apex of its shock cone.
  • e) Does an observer on the ground hear the aircraft approach? Justify using the figure.

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  • a) 863863 Hz on approach, 746746 Hz on moving away
  • b) 117117 Hz difference, perfectly audible
  • c) 858858 Hz: close but not equal, the air serving as the reference
  • d) M=1.46M=1.46 and μ=43.3°\mu=43.3°
  • e) No: all the sound is confined inside the cone, behind the aircraft
a)

Source moving toward the observer: f′=fvv−vs=800×343343−25=800×343318=863 Hzf'=f\dfrac{v}{v-v_{s}}=800\times\dfrac{343}{343-25}=800\times\dfrac{343}{318}=863\ \mathrm{Hz}. Source moving away: f′=800×343368=746 Hzf'=800\times\dfrac{343}{368}=746\ \mathrm{Hz}.

b)

The difference is 863−746=117 Hz863-746=117\ \mathrm{Hz}. It is perfectly audible: it amounts to about two and a half semitones of the musical scale, and it is exactly the jump in pitch you hear when an ambulance passes in front of you.

c)

Observer moving toward a stationary source: f′=fv+vov=800×368343=858 Hzf'=f\dfrac{v+v_{o}}{v}=800\times\dfrac{368}{343}=858\ \mathrm{Hz}. This is very close to 863 Hz863\ \mathrm{Hz}, but not equal. The two situations are therefore not equivalent, contrary to what the relativity of motion might suggest, and the reason is that there is a privileged medium of propagation here, the air: speeds count relative to it. When the source moves, it squeezes the wavelengths; when the observer moves, he simply meets the crests faster. The two effects are different, which gives different formulas.

d)

M=vplanevsound=500343=1.46M=\dfrac{v_{\mathrm{plane}}}{v_{\mathrm{sound}}}=\dfrac{500}{343}=1.46. The half-angle satisfies sin⁡μ=1M=343500=0.686\sin\mu=\dfrac{1}{M}=\dfrac{343}{500}=0.686, so μ=43.3∘\mu=43.3^{\circ}, as shown on the figure.

e)

No. Since the aircraft is faster than sound, it constantly stays ahead of the waves it emits: all the sound is confined inside the cone, behind the aircraft. An observer on the ground therefore hears absolutely nothing until the cone has reached them. They see the aircraft pass overhead in silence, then receive the sonic boom all at once as the surface of the cone sweeps over them. The sound does not come from the direction where the aircraft is at that moment, but from the position it occupied earlier.

Exercise 6: Sound pipes, beats and temperature

A pipe of length L=0.60 mL=0.60\ \mathrm{m} is at first open at both ends. The speed of sound is 343 m/s343\ \mathrm{m/s} at 20 ∘C20\ \mathrm{^{\circ}C}, and follows the law v=331+0.6 θv=331+0.6\,\theta with θ\theta in degrees Celsius.

open at both endsclosed at one endsound: v = 343 m/s at 20 °CL = 0.60 m
  • a) Calculate the fundamental frequency of the open pipe, then those of the next two harmonics.
  • b) One end is closed. Calculate the new fundamental frequency and the next two harmonics, stating which ones exist.
  • c) The open pipe is played at the same time as a string tuned to 288.0 Hz288.0\ \mathrm{Hz}. Calculate the beat frequency heard.
  • d) By what percentage would the tension of the string have to be changed to eliminate these beats, given that the frequency of a string is proportional to the square root of its tension?
  • e) The room warms up to 35 ∘C35\ \mathrm{^{\circ}C}. Recalculate the frequency of the open pipe and the new beat frequency, the string being assumed insensitive to temperature. What happens in practice in an orchestra?

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  • a) f1=v2L=286f_{1}=\dfrac{v}{2L}=286 Hz, then 572572 and 858858 Hz
  • b) f1=v4L=143f_{1}=\dfrac{v}{4L}=143 Hz, and only odd orders: 429429 and 715715 Hz
  • c) ∣288.0−285.8∣≈2.17|288.0-285.8|\approx 2.17 Hz
  • d) Slacken by about 1.5 %1.5\,\%
  • e) v=352v=352 m/s, pipe at 293293 Hz, beats at 5.335.33 Hz: the families drift apart
a)

A pipe open at both ends has a displacement antinode at each end, so L=λ2L=\dfrac{\lambda}{2} for the fundamental and f1=v2L=3431.20=286 Hzf_{1}=\dfrac{v}{2L}=\dfrac{343}{1.20}=286\ \mathrm{Hz}. All the harmonics exist: f2=572 Hzf_{2}=572\ \mathrm{Hz} and f3=858 Hzf_{3}=858\ \mathrm{Hz}.

b)

With one closed end, there must be a displacement node at the closed end and an antinode at the open end, so L=λ4L=\dfrac{\lambda}{4} and f1=v4L=3432.40=143 Hzf_{1}=\dfrac{v}{4L}=\dfrac{343}{2.40}=143\ \mathrm{Hz}, an octave lower than the open pipe of the same length. Only the odd harmonics exist: the next ones are f3=429 Hzf_{3}=429\ \mathrm{Hz} and f5=715 Hzf_{5}=715\ \mathrm{Hz}. It is this absence of even harmonics that gives the closed pipe its hollower tone.

c)

The beat frequency is the absolute value of the difference: ∣288.0−285.8∣=2.17 Hz\left|288.0-285.8\right|=2.17\ \mathrm{Hz}. You therefore hear the intensity vary about twice per second.

d)

The string must go from 288.0288.0 to 285.83 Hz285.83\ \mathrm{Hz}. Since f∝Ff\propto\sqrt{F}, we have F′F=(f′f)2=(285.83288.0)2=0.985\dfrac{F'}{F}=\left(\dfrac{f'}{f}\right)^{2}=\left(\dfrac{285.83}{288.0}\right)^{2}=0.985. The string must therefore be slackened by about 1.51.5 percent. Note that a frequency difference of 0.750.75 percent calls for a tension adjustment twice as large, the square root damping the effect.

e)

At 35 ∘C35\ \mathrm{^{\circ}C}, v=331+0.6×35=352 m/sv=331+0.6\times 35=352\ \mathrm{m/s}. The open pipe then rises to f1=3521.20=293 Hzf_{1}=\dfrac{352}{1.20}=293\ \mathrm{Hz}. The string having stayed at 288.0 Hz288.0\ \mathrm{Hz}, the new beat frequency is ∣288.0−293.3∣=5.33 Hz\left|288.0-293.3\right|=5.33\ \mathrm{Hz}, more than double. This is exactly the problem in orchestras: wind instruments go sharp as the room warms up, since their pitch follows the speed of sound in air, whereas strings tend to go flat as they slacken. The two families therefore drift out of tune in opposite directions, which is why you retune after the instruments have warmed up, not before.

f₁ = 286 Hzf₁ = 143 Hzf₂ = 572 Hzf₃ = 429 Hzf₃ = 858 Hzf₅ = 715 Hzopen at both endsclosed at left
Displacement envelopes of the air in the pipe. Open at both ends (blue), an antinode at each end: every order exists. Closed at the left (purple), a node at the closed end, an antinode at the opening: an ODD number of quarter wavelengths is needed, hence 143143, 429429 and 715715 Hz.

Part C: Geometric and wave optics (/25)

Exercise 7: A converging lens and its two regimes

A thin converging lens has a focal length f=+15 cmf=+15\ \mathrm{cm}. Use the thin lens equation 1f=1do+1di\dfrac{1}{f}=\dfrac{1}{d_{o}}+\dfrac{1}{d_{i}} and the magnification m=−didom=-\dfrac{d_{i}}{d_{o}}, with do>0d_{o}>0 for a real object.

converging lensf = +15 cmFF'Oobject a)object b)20 cm10 cm
  • a) The object is placed at do=20 cmd_{o}=20\ \mathrm{cm}. Calculate the position of the image and the magnification, and state the nature of the image.
  • b) The object is now placed at do=10 cmd_{o}=10\ \mathrm{cm}. Redo the calculation and state the nature of the image again.
  • c) What happens if the object is placed exactly at do=15 cmd_{o}=15\ \mathrm{cm}?
  • d) In which of the two cases a) and b) can the image be caught on a screen? Justify.
  • e) An object 2.0 cm2.0\ \mathrm{cm} tall is placed at 20 cm20\ \mathrm{cm}. Calculate the size of its image and state its orientation.

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  • a) di=+60d_{i}=+60 cm and m=−3.0m=-3.0: real, inverted, enlarged
  • b) di=−30d_{i}=-30 cm and m=+3.0m=+3.0: virtual, upright, enlarged. The magnifying glass
  • c) 1di=0\dfrac{1}{d_{i}}=0: the rays emerge parallel
  • d) Only the real image of case a) can be caught on a screen
  • e) 6.06.0 cm, inverted
a)

1di=115−120=4−360=160\dfrac{1}{d_{i}}=\dfrac{1}{15}-\dfrac{1}{20}=\dfrac{4-3}{60}=\dfrac{1}{60}, so di=+60 cmd_{i}=+60\ \mathrm{cm}. The magnification is m=−6020=−3.0m=-\dfrac{60}{20}=-3.0. The image is real since di>0d_{i}>0, inverted since m<0m<0, and three times larger than the object.

b)

1di=115−110=2−330=−130\dfrac{1}{d_{i}}=\dfrac{1}{15}-\dfrac{1}{10}=\dfrac{2-3}{30}=-\dfrac{1}{30}, so di=−30 cmd_{i}=-30\ \mathrm{cm}. Then m=−−3010=+3.0m=-\dfrac{-30}{10}=+3.0. The image is virtual since di<0d_{i}<0, upright since m>0m>0, and three times larger: this is how a magnifying glass works. The object is here between the lens and its focal point.

c)

1di=115−115=0\dfrac{1}{d_{i}}=\dfrac{1}{15}-\dfrac{1}{15}=0, so did_{i} tends to infinity: the rays emerge parallel and there is no image at a finite distance. This is the collimation position, used in every collimator and at the input of telescopes set to infinity.

d)

Only case a). A real image is formed by rays that actually converge at a point, so a screen can be placed there and the image seen on it. In case b), the emerging rays diverge and cross nowhere: their intersection exists only on their extensions behind the lens. A virtual image can be seen only by an eye or another instrument, never caught on a screen.

e)

The size of the image is ∣m∣×h=3.0×2.0=6.0 cm\left|m\right|\times h=3.0\times 2.0=6.0\ \mathrm{cm}. Since the magnification is negative, the image is inverted: it is 6.0 cm6.0\ \mathrm{cm} tall and points down if the object points up.

FF'objectreal, inverted imageconverging lensobject BEYOND F: real, inverted image;object between F and the lens: virtual, upright image

Exercise 8: Total internal reflection, the prism and dispersion

The index of water is n=1.33n=1.33. A glass prism with apex angle A=60.0∘A=60.0^{\circ} has an index n=1.52n=1.52 for yellow light, 1.531.53 for blue and 1.511.51 for red.

airwater, n = 1.33diverline of sightA = 60.0°lightglass: n = 1.51 (red),1.52 (yellow), 1.53 (blue)
  • a) Calculate the critical angle for total internal reflection at a water-air interface.
  • b) A diver looks up toward the surface. Describe what they see beyond the critical angle.
  • c) At minimum deviation in a prism, the two internal angles of refraction are equal. Show that they are then equal to A2\dfrac{A}{2}, then calculate the corresponding angle of incidence for yellow light.
  • d) Calculate the minimum deviation for yellow light.
  • e) Calculate the minimum deviation for blue and for red, then the angular separation between these two colours. Which colour is deviated the most?

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  • a) θc=48.8°\theta_{c}=48.8°
  • b) The surface acts as a mirror: this is Snell's window
  • c) r=A2=30.0°r=\dfrac{A}{2}=30.0° and i=49.5°i=49.5°
  • d) Dmin=2i−A≈38.9°D_{min}=2i-A\approx 38.9°
  • e) 39.8°39.8° for blue against 38.1°38.1° for red: 1.76°1.76° apart
a)

Total internal reflection occurs when light goes from the more refractive medium to the less refractive one, here from water to air. The critical angle satisfies nsin⁡θc=1×sin⁡90∘n\sin\theta_{c}=1\times\sin 90^{\circ}, so sin⁡θc=11.33=0.752\sin\theta_{c}=\dfrac{1}{1.33}=0.752 and θc=48.8∘\theta_{c}=48.8^{\circ}.

b)

Beyond 48.8∘48.8^{\circ} from the vertical, the surface behaves like a perfect mirror: the diver no longer sees the sky there but the reflection of the bottom. The whole outside world appears squeezed into a cone of half-angle 48.8∘48.8^{\circ} above their head, a phenomenon called Snell's window, and the entire horizon is concentrated on the edge of this circle.

c)

In the prism, the relation between the internal angles is r+r′=Ar+r'=A. At minimum deviation the path of the ray is symmetric, so r=r′r=r', which gives 2r=A2r=A and r=A2=30.0∘r=\dfrac{A}{2}=30.0^{\circ}. Snell's law at entry then gives sin⁡i=nsin⁡r=1.52×sin⁡30.0∘=1.52×0.500=0.760\sin i=n\sin r=1.52\times\sin 30.0^{\circ}=1.52\times 0.500=0.760, hence i=49.5∘i=49.5^{\circ}.

d)

The deviation is D=i+i′−AD=i+i'-A, and by symmetry i′=ii'=i at the minimum, so Dmin⁡=2i−A=2×49.46−60.0=38.9∘D_{\min}=2i-A=2\times 49.46-60.0=38.9^{\circ}.

e)

For blue, sin⁡i=1.53×0.500=0.765\sin i=1.53\times 0.500=0.765 gives i=49.91∘i=49.91^{\circ} and Dmin⁡=39.8∘D_{\min}=39.8^{\circ}. For red, sin⁡i=1.51×0.500=0.755\sin i=1.51\times 0.500=0.755 gives i=49.03∘i=49.03^{\circ} and Dmin⁡=38.1∘D_{\min}=38.1^{\circ}. The separation is 39.81−38.05=1.76∘39.81-38.05=1.76^{\circ}. Blue is deviated the most, because the index of glass grows as the wavelength decreases. This dispersion is what spreads white light into a spectrum, and it is also what, in raindrops, puts red on the outside of the rainbow and violet on the inside.

48.8°diverbottomthe whole sky, in this conemirror: reflection of the bottomairwater, n = 1.33
a) and b) Rays coming from the sky, even grazing ones, all enter a cone of half-angle θc=48.8°\theta_{c}=48.8° above the diver: this is Snell's window. Beyond it, the surface acts as a mirror and the diver sees the bottom there (purple, 60°>θc60°>\theta_{c}).
A = 60°i = 49.5°rr'i' = 49.5°D = 38.9°n = 1.52yellow light
c) and d) At minimum deviation, the path is symmetric: the ray crosses the prism parallel to the base, r=r′=A2=30.0°r=r'=\dfrac{A}{2}=30.0°, and i=i′=49.5°i=i'=49.5°. The dotted extensions meet at an angle Dmin=2i−A=38.9°D_{min}=2i-A=38.9°.
A = 60°49.5°white lightred: D = 38.1°blue: D = 39.8°glass
e) White light at the same incidence: blue (n=1.53n=1.53) is deviated by 39.8°39.8°, red (n=1.51n=1.51) by 38.1°38.1°, a separation of 1.76°1.76°. The emerging rays are extended so that the separation can be seen; at this incidence, each colour is within 0.01°0.01° of its own minimum.

Exercise 9: Young, grating and slit: three ways to diffract

A sodium lamp of wavelength λ=589 nm\lambda=589\ \mathrm{nm} is used, with a screen placed at D=2.0 mD=2.0\ \mathrm{m}.

sodium lampλ = 589 nmaperturescreena) two slitsd = 0.25 mmb) grating600 lines/mmc) single slita = 0.10 mmopenings seen face on, enlargedD = 2.0 m
  • a) Two slits a distance d=0.25 mmd=0.25\ \mathrm{mm} apart produce interference fringes. Calculate the fringe spacing.
  • b) The two slits are replaced by a grating of 600 lines per millimetre. Calculate the angle of the first order, then the total number of orders observable on each side.
  • c) A single slit of width a=0.10 mma=0.10\ \mathrm{mm} diffracts on its own. Calculate the angle of the first minimum and the width of the central maximum on the screen.
  • d) Return to the double-slit setup, each slit having width a=0.10 mma=0.10\ \mathrm{mm} and the slits being d=0.25 mmd=0.25\ \mathrm{mm} apart. Find the missing orders.
  • e) Compare the sharpness of the grating maxima with that of Young's fringes. Why is a grating, and not two slits, used to measure a wavelength precisely?

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  • a) i=λDd≈4.71i=\dfrac{\lambda D}{d}\approx 4.71 mm
  • b) θ1=20.7°\theta_{1}=20.7°; m≤2.83m\leq 2.83, so two orders on each side
  • c) θ=0.337°\theta=0.337° and a central maximum 23.623.6 mm wide
  • d) m=2.5 nm=2.5\,n: orders 55 and 1010 are missing
  • e) Thousands of sources sharpen the maxima: you can pinpoint them better
a)

The fringe spacing is i=λDd=589×10−9×2.00.25×10−3=4.71×10−3 mi=\dfrac{\lambda D}{d}=\dfrac{589\times 10^{-9}\times 2.0}{0.25\times 10^{-3}}=4.71\times 10^{-3}\ \mathrm{m}, that is 4.71 mm4.71\ \mathrm{mm}.

b)

The grating spacing is d=1 mm600=1.667×10−6 md=\dfrac{1\ \mathrm{mm}}{600}=1.667\times 10^{-6}\ \mathrm{m}. The first order satisfies sin⁡θ1=λd=589×10−91.667×10−6=0.353\sin\theta_{1}=\dfrac{\lambda}{d}=\dfrac{589\times 10^{-9}}{1.667\times 10^{-6}}=0.353, so θ1=20.7∘\theta_{1}=20.7^{\circ}. Orders exist as long as sin⁡θ=mλd≤1\sin\theta=\dfrac{m\lambda}{d}\leq 1, that is m≤dλ=2.83m\leq\dfrac{d}{\lambda}=2.83: orders 1 and 2 are therefore observed on each side, and order 3 is out of reach.

c)

The first diffraction minimum satisfies sin⁡θ=λa=589×10−90.10×10−3=5.89×10−3\sin\theta=\dfrac{\lambda}{a}=\dfrac{589\times 10^{-9}}{0.10\times 10^{-3}}=5.89\times 10^{-3}, so θ=0.337∘\theta=0.337^{\circ}, a very small angle. The central maximum extends on both sides, and its total width on the screen is 2λDa=2×2.0×5.89×10−3=2.36×10−2 m\dfrac{2\lambda D}{a}=2\times 2.0\times 5.89\times 10^{-3}=2.36\times 10^{-2}\ \mathrm{m}, that is 23.6 mm23.6\ \mathrm{mm}.

d)

An interference order is missing when it falls exactly on a diffraction minimum, that is when mλd=nλa\dfrac{m\lambda}{d}=\dfrac{n\lambda}{a}, or m=nda=2.5 nm=n\dfrac{d}{a}=2.5\,n. For n=1n=1 this gives 2.52.5, which is not an integer, so no order is lost. For n=2n=2 we get m=5m=5, and for n=4n=4 we get m=10m=10. The missing orders are therefore orders 5 and 10: the diffraction envelope erases these interference fringes, which exist in principle but receive zero intensity.

e)

Young's fringes are broad and sinusoidal: the intensity varies gently, so pinpointing the centre of a maximum is imprecise. A grating of 600 lines makes not two but thousands of coherent sources interfere, and all of them must be in phase to give a maximum: the slightest change of angle destroys the agreement and the intensity collapses. The maxima are therefore extremely sharp, which allows their position, and hence λ\lambda, to be measured with far better precision. It is the same principle as the Wheatstone bridge: measuring by looking for a sharp condition is always more precise than reading a slow variation.

two slits: equal fringesgrating: sharp and well separatedsingle slit: wide centresame wavelength, three setups:the GEOMETRY of the opening shapes the pattern

Part D: Modern physics (/25)

Exercise 10: The photoelectric effect

A metal plate of work function W=2.30 eVW=2.30\ \mathrm{eV} is illuminated by light of wavelength 400 nm400\ \mathrm{nm}.

Use the practical relation E (in eV)=1240λ (in nm)E\ \left(\mathrm{in\ eV}\right)=\dfrac{1240}{\lambda\ \left(\mathrm{in\ nm}\right)}.

lampλ = 400 nmmetal plateW = 2.30 eV
  • a) Calculate the energy of an incident photon, in electronvolts.
  • b) Calculate the maximum kinetic energy of the emitted electrons, then the stopping potential.
  • c) Calculate the threshold wavelength beyond which no electron is emitted.
  • d) Calculate the maximum speed of the emitted electrons, with me=9.109×10−31 kgm_{e}=9.109\times 10^{-31}\ \mathrm{kg}.
  • e) The light intensity is doubled without changing the wavelength. What is observed for the number of emitted electrons and for their kinetic energy? Why was this result decisive against the wave model?

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  • a) E=1240400=3.10E=\dfrac{1240}{400}=3.10 eV
  • b) Ek,max=0.80E_{k,max}=0.80 eV and U0=0.80U_{0}=0.80 V
  • c) λ0=12402.30≈539\lambda_{0}=\dfrac{1240}{2.30}\approx 539 nm
  • d) vmax≈5.30×105v_{max}\approx 5.30\times 10^{5} m/s, nonrelativistic
  • e) The current doubles, the kinetic energy does not change
a)

E=1240400=3.10 eVE=\dfrac{1240}{400}=3.10\ \mathrm{eV}.

b)

Einstein's relation gives Ek,max⁡=E−W=3.10−2.30=0.80 eVE_{k,\max}=E-W=3.10-2.30=0.80\ \mathrm{eV}. The stopping potential is the voltage that blocks even the fastest electrons: eU0=Ek,max⁡eU_{0}=E_{k,\max}, so U0=0.80 VU_{0}=0.80\ \mathrm{V}. Numerically, the kinetic energy in electronvolts and the stopping potential in volts have the same value, which is the very convenience of the electronvolt.

c)

The threshold corresponds to E=WE=W, so λ0=12402.30=539 nm\lambda_{0}=\dfrac{1240}{2.30}=539\ \mathrm{nm}. Any light of longer wavelength, hence redder than yellow-green, ejects no electron, whatever its intensity.

d)

Ek,max⁡=0.80 eV=0.80×1.602×10−19=1.28×10−19 JE_{k,\max}=0.80\ \mathrm{eV}=0.80\times 1.602\times 10^{-19}=1.28\times 10^{-19}\ \mathrm{J}. Then vmax⁡=2Ek,max⁡me=2.563×10−199.109×10−31=5.30×105 m/sv_{\max}=\sqrt{\dfrac{2E_{k,\max}}{m_{e}}}=\sqrt{\dfrac{2.563\times 10^{-19}}{9.109\times 10^{-31}}}=5.30\times 10^{5}\ \mathrm{m/s}, about one five-hundredth of the speed of light, which justifies the nonrelativistic calculation.

e)

Doubling the intensity doubles the number of photons per second, hence doubles the number of emitted electrons and so the current. But the maximum kinetic energy does not change at all, because it depends only on the energy of an individual photon, set by the wavelength. This is precisely what the wave model could not explain: in that model, a more intense wave carries more energy and should therefore give more energy to each electron, and a weak wave should eventually eject electrons after a time of accumulation. Experiment shows the opposite: a frequency threshold, no delay, and an energy independent of the intensity. Light had to be admitted to exchange its energy in grains, one photon for one electron.

0123456789-3-2-101f (10¹⁴ Hz)Ek,max (eV)400 nm : 0.80 eVthreshold:5.56 × 10¹⁴ Hz (539 nm)−W = −2.30 eVslope: h
Einstein's relation Ek,max=hf−WE_{k,max}=hf-W is a straight line of slope hh. It cuts the frequency axis at the threshold f0=5.56×1014f_{0}=5.56\times 10^{14} Hz, that is 539539 nm; below it (dashed), no electron leaves, whatever the intensity. At 400400 nm, f=7.50×1014f=7.50\times 10^{14} Hz and Ek,max=0.80E_{k,max}=0.80 eV.

Exercise 11: Bohr, de Broglie and uncertainty

In the Bohr model, the energy levels of the hydrogen atom are En=−13.6n2 eVE_{n}=-\dfrac{13.6}{n^{2}}\ \mathrm{eV}.

Take h=6.626×10−34 J⋅sh=6.626\times 10^{-34}\ \mathrm{J\cdot s}, ℏ=1.0546×10−34 J⋅s\hbar=1.0546\times 10^{-34}\ \mathrm{J\cdot s} and me=9.109×10−31 kgm_{e}=9.109\times 10^{-31}\ \mathrm{kg}.

  • a) Calculate the energy of the photon emitted in the transition from n=3n=3 to n=2n=2, then its wavelength. What colour does it correspond to?
  • b) Calculate the energy needed to ionize a hydrogen atom from its ground state.
  • c) Calculate the de Broglie wavelength of an electron moving at the speed 5.30×105 m/s5.30\times 10^{5}\ \mathrm{m/s} found in exercise 10.
  • d) An electron is localized in a region of size Δx=0.10 nm\Delta x=0.10\ \mathrm{nm}, the order of magnitude of an atom. Estimate the minimum uncertainty on its speed using Δp Δx≥ℏ2\Delta p\,\Delta x\geq\dfrac{\hbar}{2}.
  • e) Compare this uncertainty with the speed itself. What can be concluded about the notion of an electron orbit?

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  • a) ΔE=1.89\Delta E=1.89 eV, that is λ≈656\lambda\approx 656 nm: the red Hα\alpha line
  • b) 13.613.6 eV
  • c) λ=hmev≈1.4\lambda=\dfrac{h}{m_{e}v}\approx 1.4 nm, ten times the size of an atom
  • d) Δp≈5.27×10−25\Delta p\approx 5.27\times 10^{-25} kg·m/s and Δv≈5.79×105\Delta v\approx 5.79\times 10^{5} m/s
  • e) The uncertainty exceeds the speed: the orbit makes no physical sense
a)

ΔE=E3−E2=−13.69+13.64=−1.511+3.400=1.889 eV\Delta E=E_{3}-E_{2}=-\dfrac{13.6}{9}+\dfrac{13.6}{4}=-1.511+3.400=1.889\ \mathrm{eV}. The wavelength is λ=12401.889=656 nm\lambda=\dfrac{1240}{1.889}=656\ \mathrm{nm}, which corresponds to red. This is the H-alpha line, the brightest in the visible spectrum of hydrogen, and it is what gives nebulae their red tint.

b)

To ionize from the ground state is to take the electron from n=1n=1 to n=∞n=\infty, where the energy is zero. We must therefore supply 0−(−13.6)=13.6 eV0-\left(-13.6\right)=13.6\ \mathrm{eV}. This is the ionization energy of hydrogen.

c)

λ=hmev=6.626×10−349.109×10−31×5.30×105=6.626×10−344.83×10−25=1.37×10−9 m\lambda=\dfrac{h}{m_{e}v}=\dfrac{6.626\times 10^{-34}}{9.109\times 10^{-31}\times 5.30\times 10^{5}}=\dfrac{6.626\times 10^{-34}}{4.83\times 10^{-25}}=1.37\times 10^{-9}\ \mathrm{m}, about 1.4 nm1.4\ \mathrm{nm}. This is more than ten times the size of an atom, which explains why an electron of this energy cannot be treated as a little ball at all.

d)

Δp≥ℏ2Δx=1.0546×10−342×1.0×10−10=5.27×10−25 kg⋅m/s\Delta p\geq\dfrac{\hbar}{2\Delta x}=\dfrac{1.0546\times 10^{-34}}{2\times 1.0\times 10^{-10}}=5.27\times 10^{-25}\ \mathrm{kg\cdot m/s}. The uncertainty on the speed is then Δv=Δpme=5.27×10−259.109×10−31=5.79×105 m/s\Delta v=\dfrac{\Delta p}{m_{e}}=\dfrac{5.27\times 10^{-25}}{9.109\times 10^{-31}}=5.79\times 10^{5}\ \mathrm{m/s}.

e)

The uncertainty on the speed, 5.79×105 m/s5.79\times 10^{5}\ \mathrm{m/s}, is of the same order as the speed itself, and even slightly larger. This means that for an electron confined in an atom, the speed is not even approximately known: it is completely undetermined. Speaking of an orbit, that is, a trajectory along which both position and speed would be known at every instant, therefore makes no physical sense. The Bohr model gives the right energy levels, which explains its success, but its picture of an electron travelling around a well-defined circle is wrong. Quantum mechanics replaces it with a probability density of presence, the orbital.

n = 1−13.6 eVn = 2−3.40 eVn = 3−1.51 eVn = ∞0 eV1.89 eV, λ = 656 nmionization: 13.6 eV
Bohr levels to scale. The drop from n=3n=3 to n=2n=2 releases 1.891.89 eV, the red H-alpha line at 656656 nm; ionizing from n=1n=1 takes the whole depth of the well, 13.613.6 eV. The levels crowd together toward 00: beyond n=3n=3, they are no longer named.

Exercise 12: Five statements to check

Each of the following five statements is false. For each one, explain the error and, where possible, rely on a numerical result from the previous exercises.

Each of the five concerns a different part of the course.

  • a) “The period of a simple pendulum increases if the suspended mass is made heavier.”
  • b) “Doubling the amplitude of a wave doubles the power it carries.”
  • c) “Doubling the intensity of a sound doubles its level in decibels.”
  • d) “An object placed at the object focal point of a converging lens has its image at the image focal point.”
  • e) “Illuminating a metal plate more intensely increases the kinetic energy of the electrons it emits.”

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  • a) The mass does not appear in T=2πL/gT=2\pi\sqrt{L/g}
  • b) P∝A2P\propto A^{2}: it QUADRUPLES
  • c) Doubling the intensity adds ≈3\approx 3 dB, not a factor of two
  • d) An object at the object focal point gives an image at infinity
  • e) The intensity sets the number of electrons, not their energy
a)

False. The period is T=2πLgT=2\pi\sqrt{\dfrac{L}{g}}: the mass does not appear in it. A heavier mass does increase the restoring force, but increases in exactly the same proportion the inertia to be set in motion, and the two effects cancel. It is the same reason that makes all bodies fall with the same acceleration. Only the length and gravity matter, as exercise 2 shows, where L=0.994 mL=0.994\ \mathrm{m} gives two seconds for any mass.

b)

False. The power carried is proportional to the SQUARE of the amplitude, P=12μvω2A2P=\dfrac{1}{2}\mu v\omega^{2}A^{2}. Doubling the amplitude therefore multiplies the power by four, as calculated in exercise 3. This is also why the energy of a damped oscillator falls to a quarter when its amplitude falls to half, the result obtained in exercise 2.

c)

False, and the error is of the same type as the previous one but in the opposite direction. The decibel scale is logarithmic: doubling the intensity adds 10log⁡2≈3.0 dB10\log 2\approx 3.0\ \mathrm{dB}. Exercise 4 puts numbers on it: two identical sources take you from 9090 to 93 dB93\ \mathrm{dB}, not to 180 dB180\ \mathrm{dB}, which would in any case be far beyond anything the atmosphere can transmit. To double the level in decibels, the intensity would have to be multiplied by 10910^{9}.

d)

False, and the opposite is in fact what happens. An object placed at the object focal point gives an image at INFINITY: the rays emerge parallel, as calculated in part c) of exercise 7, where do=15 cm=fd_{o}=15\ \mathrm{cm}=f leads to 1di=0\dfrac{1}{d_{i}}=0. Conversely, an object at infinity gives its image at the image focal point. The two focal points are each conjugate to infinity, not to each other.

e)

False, and it is the observation that forced the photon on us. The intensity sets the number of photons per second, hence the number of electrons emitted and the current, but the maximum kinetic energy depends only on the energy of one photon, that is, on the wavelength: Ek,max⁡=1240λ−WE_{k,\max}=\dfrac{1240}{\lambda}-W. In exercise 10 it is 0.80 eV0.80\ \mathrm{eV} at 400 nm400\ \mathrm{nm}, and doubling the intensity leaves it strictly unchanged. Light redder than 539 nm539\ \mathrm{nm} ejects no electron at all, however intense it is, which is incomprehensible in a purely wave model.

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© Ahmed Squalli Houssaini. Exercise set published at www.letuteurscientifique.ca/en/exercices/cegep-phys3-practice-final-optics. Free for personal and classroom use; republishing it elsewhere requires written permission (legal notice).

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