PHYS 101 Introductory Physics, Mechanics • McGill University, Montreal

Second practice final exam, fully corrected (PHYS 101)

This is a second practice final examination for PHYS 101, Introductory Physics, Mechanics, the algebra based first year course at McGill University. It follows the format of the real final: ten conceptual questions worth three points each (Part A), then seven problems worth ten points each (Part B), three hours, a calculator and the official formula sheet allowed. The values of the sheet are used throughout, g=9.81g = 9.81 m/s2^2 and 330330 m/s for sound, and every solution names the line of the sheet it uses. No derivative and no integral appears anywhere.

It covers the whole course except geometric optics, which belongs to PHYS 102: light enters only through its speed in a medium, thin films, gratings, polarization and the Rayleigh criterion. Vectors and the angle of the formula sheet (questions 1 and 11), projectiles (2 and 14), Newton's laws and friction (3 and 12), gravitation (4), work, energy and power (5, 11 and 13), momentum and the centre of mass (6 and 14), rotation, angular momentum and rolling (7 and 15), oscillations (8 and 16), sound, decibels, the Doppler effect and beats (9 and 16), wave optics (10 and 17). It gives more room than the first practice final to angular momentum, rolling, decibels, beats, thin films, gratings, polarization and the Rayleigh criterion.

Four problems are solved in letters before any number, as the tutorials of the course ask: the snowboarder (question 12), the loop (question 13), the cue ball (question 15) and the tuning fork (question 16). Each one checks the dimensions of its result, a limiting case and the way the answer varies with a parameter. Not one of the seventeen situations appears in the twelve chapter sets of this site or in the first practice final.

The traps named in the solutions: the supplement of the angle in the formula that adds two vectors (questions 1 and 11), a friction force that keeps its direction after the turn around (question 12), a toy car expected to reach the top of the loop at rest (question 13), kinetic energy conserved in a burst (question 14), a single Doppler shift where there are two (question 16), the half wavelength shift forgotten in a thin film and the cosine of Malus's law without its square (question 17), and, in Part A, the decibel read as a plain unit (question 9).

17 corrected exercises • 100 points • 180 minutes

This chapter is part of PHYS 101, every chapter with its set and sheet

Self-checking set Type your answers and check them question by question: the page tells you right or wrong before you open the solution. With an account, every answer right on the first try earns points, and your right answers stay filled in when you come back.

Part A: conceptual questions (/30)

Exercise 1: Two tractors on one stump: adding two forces at 120 degrees

This is a three hour practice final for PHYS 101. Part A asks ten conceptual questions worth three points each: choose one answer, and justify it in one or two sentences, because the justification is what earns the marks. Part B asks seven problems worth ten points each. The official PHYS 101 formula sheet is allowed, as at the real exam, and so is a calculator. Take g=9.81g = 9.81 m/s2^2 and a speed of sound in air of 330330 m/s, the values of the formula sheet, unless a question gives its own.

Two tractors pull on the same tree stump with ropes, each with a tension of 300300 N. Seen from above, the angle between the two ropes, measured between the two directions of pull, is 120∘120^{\circ}, as drawn.

300 N, tractor 1300 N, tractor 2120°stump
  • a) What is the magnitude of the total force the two ropes exert on the stump?
  • b) The tractors move until the angle between the ropes is 60∘60^{\circ}. Find the new magnitude.

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  • a) 300300 N
  • b) 520520 N
a)

Formula sheet, General equations: ∣a⃗+b⃗∣2=a2+b2+2abcos⁡θ|\vec a+\vec b|^{2} = a^{2}+b^{2}+2ab\cos\theta, where θ\theta is the interior angle between the two vectors drawn from the same point, exactly the 120∘120^{\circ} of the figure.

∣F⃗∣2=3002+3002+2(300)(300)cos⁡120∘=90000+90000−90000=90000|\vec F|^{2} = 300^{2}+300^{2}+2(300)(300)\cos 120^{\circ} = 90000+90000-90000 = 90000, so ∣F⃗∣=300|\vec F| = 300 N.

Check by components along the dashed bisector: each rope gives 300cos⁡60∘=150300\cos 60^{\circ} = 150 N along it, the sideways parts cancel, and 150+150=300150+150 = 300 N.

Pitfall: 520520 N uses cos⁡60∘\cos 60^{\circ}, the angle of the triangle drawn head to tail, which is the supplement of the angle between the vectors. The angle of the sheet is the one between the two vectors placed tail to tail.

600600 N adds the magnitudes, which is right only when the two ropes pull the same way.

424424 N is Pythagoras, 3002300\sqrt 2, right only at 90∘90^{\circ}.

00 N would need the two ropes to pull in opposite directions, at 180∘180^{\circ}.

b)

∣F⃗∣2=3002+3002+2(300)(300)cos⁡60∘=180000+90000=270000|\vec F|^{2} = 300^{2}+300^{2}+2(300)(300)\cos 60^{\circ} = 180000+90000 = 270000, so ∣F⃗∣=519.6|\vec F| = 519.6 N, about 520520 N.

The 520520 N of the wrong answer in a) belongs here: closing the angle between two pulls makes their sum larger.

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Exercise 2: Two stones from a footbridge: speed at the water and order of arrival

From a footbridge 12.012.0 m above a river, a hiker throws two identical stones, one after the other, with the same speed of 9.09.0 m/s: stone 1 at 30∘30^{\circ} above the horizontal, stone 2 at 30∘30^{\circ} below it. Air resistance is neglected.

9.0 m/sstone 19.0 m/sstone 230°30°river12.0 m
  • a) Which stone hits the water with the greater speed? Give that speed.
  • b) Which stone reaches the water first?

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  • a) The same speed for both, 17.817.8 m/s
  • b) Stone 2, after 1.171.17 s, against 2.092.09 s for stone 1
a)

Formula sheet, Work and energy: with no air resistance only gravity does work, so KE+PEKE + PE is the same on the bridge and at the water: 12mv2=12mv02+mgh\frac{1}{2}mv^{2} = \frac{1}{2}mv_{0}^{2} + mgh.

v=v02+2ghv = \sqrt{v_{0}^{2}+2gh}: neither the direction of the throw nor the mass appears.

v=9.02+2(9.81)(12.0)=81.0+235.4=17.8v = \sqrt{9.0^{2}+2(9.81)(12.0)} = \sqrt{81.0+235.4} = 17.8 m/s for both stones.

Stone 1 does stay longer in the air, but it first climbs and loses speed: when it falls back through the level of the bridge it has 9.09.0 m/s again, pointing 30∘30^{\circ} below the horizontal, exactly like stone 2.

Stone 2 heads down from the start, but with the same speed and the same 12.012.0 m to fall, so it gains the same energy.

The masses cancel in the energy balance, so no information is missing.

b)

Vertical motion, upward positive, with the constant acceleration line of the formula sheet and the quadratic formula: −12.0=v0yt−4.905t2-12.0 = v_{0y}t - 4.905t^{2}.

Stone 2, v0y=−4.5v_{0y} = -4.5 m/s: 4.905t2+4.5t−12.0=04.905t^{2}+4.5t-12.0 = 0 gives t=−4.5+4.52+4(4.905)(12.0)2(4.905)=−4.5+15.999.81=1.17t = \frac{-4.5+\sqrt{4.5^{2}+4(4.905)(12.0)}}{2(4.905)} = \frac{-4.5+15.99}{9.81} = 1.17 s.

Stone 1, v0y=+4.5v_{0y} = +4.5 m/s: 4.905t2−4.5t−12.0=04.905t^{2}-4.5t-12.0 = 0 gives t=4.5+15.999.81=2.09t = \frac{4.5+15.99}{9.81} = 2.09 s.

The difference, 0.920.92 s, is exactly the time stone 1 spends going up and coming back to the level of the bridge, 2v0yg=2(4.5)9.81=0.92\frac{2v_{0y}}{g} = \frac{2(4.5)}{9.81} = 0.92 s.

Pitfall: the same speed at the water does not mean the same time in the air.

Exercise 3: A car pushes a pickup: the third law and the push of the road

A small car of mass 11001100 kg pushes a stalled pickup truck of mass 24002400 kg along a level street, bumper against bumper. The pair is speeding up.

  • a) Compare the force the car exerts on the pickup with the force the pickup exerts on the car.
  • b) What horizontal force does the road exert on the driven tyres of the car?

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  • a) Equal in magnitude and opposite in direction, at every instant (third law)
  • b) A forward force: static friction of the road on the driven tyres
a)

The two forces are the two members of one action-reaction pair: Newton's third law makes them equal in magnitude and opposite in direction at every instant, whatever the masses and whatever the motion.

The pair speeds up because of the forces acting ON it from outside, chiefly the road on the tyres, not because one member of a pair beats the other.

The car pushes harder: this compares two forces that act on different bodies. What decides the acceleration of the pickup is the net force on the pickup alone, the push of the car minus the resistance on the pickup.

The pickup pushes harder: this confuses a force with its effect. The same force gives the heavier pickup the smaller acceleration.

Equal only at constant speed: that is the first law dressed as the third. The third law holds while accelerating too.

b)

The engine turns the wheels; the tread pushes BACKWARD on the road, and the road pushes FORWARD on the tread, by the third law again. That forward push is the only horizontal external force that can speed up the car and the pickup.

The tread does not slip on the road, so the friction is STATIC: whatever is needed, up to μsFN\mu_{s}F_{N} (formula sheet, Dynamics: Ffr,s≤μsFNF_{fr,s} \le \mu_{s}F_{N}).

Pitfall: friction opposes the SLIPPING of the two surfaces, not the motion of the car. That is why it can point forward.

None, the engine pushes: the engine is inside the car, and internal forces cannot accelerate a body. On glare ice the wheels spin and the car stays put.

Kinetic friction would mean the tyres are spinning on the road, which is exactly what a driver avoids.

Exercise 4: Two moons of an exoplanet: Kepler's third law as a ratio

Astronomers follow two moons on circular orbits around the same exoplanet. The inner moon goes round in 2.02.0 days; the radius of the orbit of the outer moon is 4.04.0 times that of the inner moon.

  • a) What is the period of the outer moon?
  • b) How many times faster than the outer moon does the inner moon travel along its orbit?

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  • a) 1616 days
  • b) 2.02.0 times faster
a)

Formula sheet, Circular motion and gravity: T2r3=4π2GM\frac{T^{2}}{r^{3}} = \frac{4\pi^{2}}{GM}. Both moons orbit the same planet, so the right side is the same number for both, and the unknown mass of the planet cancels in a ratio.

(T2T1)2=(r2r1)3=4.03=64\left(\frac{T_{2}}{T_{1}}\right)^{2} = \left(\frac{r_{2}}{r_{1}}\right)^{3} = 4.0^{3} = 64, so T2T1=8.0\frac{T_{2}}{T_{1}} = 8.0 and T2=16T_{2} = 16 days.

8.08.0 days takes T∝rT \propto r; 4.04.0 days takes T∝rT \propto \sqrt{r}; 3232 days takes T∝r2T \propto r^{2}; 128128 days takes T∝r3T \propto r^{3} and forgets the square root of the left side. Only T2∝r3T^{2} \propto r^{3} is on the sheet.

b)

On a circle, speed is circumference over period, v=2πrTv = \frac{2\pi r}{T}.

v1v2=r1r2⋅T2T1=14.0(8.0)=2.0\frac{v_{1}}{v_{2}} = \frac{r_{1}}{r_{2}}\cdot\frac{T_{2}}{T_{1}} = \frac{1}{4.0}(8.0) = 2.0: the inner moon is twice as fast.

Same result from gravity alone: GMmr2=mv2r\frac{GMm}{r^{2}} = \frac{mv^{2}}{r} gives v=GMrv = \sqrt{\frac{GM}{r}}, and 4.0=2.0\sqrt{4.0} = 2.0.

Pitfall: the longer path of the outer moon does not make it faster. It is slower AND has farther to go, which is why its period is eight times longer.

Exercise 5: Lowering a piano at constant speed: who does work, and how much

Two movers lower a 9090 kg piano from a balcony to the street, 6.06.0 m below, with a rope, at a constant slow speed.

  • a) What is the work done by the rope on the piano during the descent?
  • b) What is the net work done on the piano?

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  • a) Wrope=−mgh=−5.30W_{rope} = -mgh = -5.30 kJ
  • b) Zero
a)

Formula sheet, Work and energy: W=F⃗⋅d⃗=Fdcos⁡θW = \vec F\cdot\vec d = Fd\cos\theta. The rope pulls UP while the piano moves DOWN, so θ=180∘\theta = 180^{\circ} and the work is negative.

Constant speed means zero acceleration, so the tension equals the weight: T=mg=90(9.81)=883T = mg = 90(9.81) = 883 N.

Wrope=Tdcos⁡180∘=−883(6.0)=−5.30×103W_{rope} = Td\cos 180^{\circ} = -883(6.0) = -5.30\times 10^{3} J, that is −mgh=−5.30-mgh = -5.30 kJ.

Positive work would mean the rope helps the motion; here it holds the piano back, which is the whole point of the rope.

Zero work confuses the net work with the work of one force: the speed is constant, so the TOTAL is zero, not each term.

Smaller in size than mghmgh would need the piano to speed up on the way down, which it does not.

b)

Formula sheet: Wnet=ΔKEW_{net} = \Delta KE, and the kinetic energy does not change, so Wnet=0W_{net} = 0.

Term by term: gravity does +mgh=+5.30+mgh = +5.30 kJ, the rope −5.30-5.30 kJ, and the sum is zero. The 5.305.30 kJ of potential energy the piano loses end up as heat in the hands of the movers and in the rope rubbing on the railing.

No time is needed: work is a force times a displacement.

Exercise 6: Walking along a canoe: the centre of mass stays put

A 7070 kg paddler stands at the back of a 5050 kg canoe at rest on still water, a few metres from a dock. She walks 3.03.0 m toward the front, measured along the canoe, then stops. Neglect the resistance of the water.

  • a) What does the canoe do during and after her walk?
  • b) How far does the canoe move relative to the water?

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  • a) It moves backward while she walks, and stops when she stops
  • b) 1.751.75 m backward, while she moves 1.251.25 m forward
a)

Paddler and canoe form a system that is isolated horizontally and starts at rest. Formula sheet, Momentum and collisions: p1,i+p2,i=p1,f+p2,fp_{1,i}+p_{2,i} = p_{1,f}+p_{2,f}, so the total momentum stays zero.

While she moves forward, the canoe must move backward with an equal and opposite momentum; when she stops, her momentum is zero, so the canoe's is zero too, and it stops.

It stays put: but she pushes the canoe backward with her feet, and nothing holds it.

It keeps drifting: that would leave a nonzero total momentum, appearing from zero with no external force.

It moves forward: the two momenta would then point the same way, and their sum could not be zero.

b)

A total momentum of zero from rest means the centre of mass does not move: formula sheet, xCOM=m1x1+m2x2m1+m2x_{COM} = \frac{m_{1}x_{1}+m_{2}x_{2}}{m_{1}+m_{2}} keeps its value.

Let the canoe move back a distance ss. Relative to the water she moves forward 3.0−s3.0 - s, and the shifts of the two masses must balance: 70(3.0−s)=50s70(3.0 - s) = 50s.

s=70(3.0)70+50=1.75s = \frac{70(3.0)}{70+50} = 1.75 m, and she moves 3.0−1.75=1.253.0 - 1.75 = 1.25 m relative to the water.

Check: the heavier body moves less, and 70(1.25)=50(1.75)=87.570(1.25) = 50(1.75) = 87.5 kg m.

Pitfall: the 3.03.0 m is measured on the canoe, which is itself moving. Her displacement relative to the water is not 3.03.0 m.

Exercise 7: A diver tucks: angular momentum and kinetic energy

A diver leaves the platform turning at 1.21.2 revolutions per second with her body stretched out, with a moment of inertia of 1212 kg m2^2 about her centre of mass. In the air she pulls into a tight tuck, which brings her moment of inertia down to 4.04.0 kg m2^2.

  • a) What is her rate of rotation in the tuck?
  • b) What happens to her rotational kinetic energy? Give its value in the tuck.

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  • a) 3.63.6 revolutions per second
  • b) It triples, from 341341 J to 10231023 J; the extra energy comes from her muscles
a)

In the air the only external force is her weight, which acts at her centre of mass and has no torque about it. Formula sheet, Rotational motion: τ=ΔLΔt\tau = \frac{\Delta L}{\Delta t}, so with no torque L=IωL = I\omega stays constant.

I1ω1=I2ω2I_{1}\omega_{1} = I_{2}\omega_{2} gives ω2=124.0(1.2)=3.6\omega_{2} = \frac{12}{4.0}(1.2) = 3.6 revolutions per second: three times less inertia, three times faster.

1.21.2 rev/s keeps ω\omega instead of LL; 0.400.40 rev/s divides by the ratio instead of multiplying; 10.810.8 rev/s multiplies by its square, as if LL were Iω2I\omega^{2}.

b)

Formula sheet: KErot=12Iω2KE_{rot} = \frac{1}{2}I\omega^{2}, which can be written L22I\frac{L^{2}}{2I}. With LL fixed, dividing II by three multiplies the energy by three.

Before: ω1=2π(1.2)=7.540\omega_{1} = 2\pi(1.2) = 7.540 rad/s and KE=12(12)(7.540)2=341KE = \frac{1}{2}(12)(7.540)^{2} = 341 J.

After: ω2=2π(3.6)=22.62\omega_{2} = 2\pi(3.6) = 22.62 rad/s and KE=12(4.0)(22.62)2=1023KE = \frac{1}{2}(4.0)(22.62)^{2} = 1023 J, three times as much.

The extra 682682 J come from her muscles: pulling her arms and legs toward the axis while they are turning takes work, done inside the system. Angular momentum is conserved, kinetic energy is not.

Unchanged confuses the two quantities; times nine squares ω\omega but forgets that II shrank; divided by three is the inverse of the truth.

Exercise 8: A spring and a pendulum taken to the Moon

A lunar laboratory kit holds a mass on a spring, hung vertically, and a simple pendulum. On Earth both oscillate with a period of 1.501.50 s. The kit is taken to the Moon, where g=1.62g = 1.62 m/s2^2.

  • a) What happens to the two periods on the Moon?
  • b) Find the period of the pendulum on the Moon.

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  • a) The period of the spring is unchanged, the period of the pendulum gets longer
  • b) 3.693.69 s
a)

Formula sheet, Simple harmonic motion: ωspring=k/m\omega_{spring} = \sqrt{k/m} and ωpendulum=g/L\omega_{pendulum} = \sqrt{g/L}, with T=2πωT = \frac{2\pi}{\omega}.

No gg for the spring: on the Moon it hangs less stretched, but it oscillates about that new equilibrium with the same kk and the same mm, so with the same period.

A gg for the pendulum: its restoring force is a part of the weight, so a weaker gg means a weaker restoring force and a slower swing.

Both longer treats the spring as if gravity drove it. Spring longer and pendulum unchanged swaps the two formulas. Pendulum shorter misreads T∝1gT \propto \frac{1}{\sqrt g}: a smaller gg gives a LONGER period.

b)

At fixed LL, T∝1gT \propto \frac{1}{\sqrt g}, so TMoon=1.509.811.62=1.50(2.461)=3.69T_{Moon} = 1.50\sqrt{\frac{9.81}{1.62}} = 1.50(2.461) = 3.69 s.

Sense check: gg is about six times smaller on the Moon and 6≈2.5\sqrt 6 \approx 2.5, so the period should be about two and a half times longer.

Exercise 9: Earplugs at a concert: what thirty decibels mean

Near the stage of a rock concert the sound level is 112112 dB. A spectator wears foam earplugs that lower the level reaching her eardrum by 3030 dB.

  • a) By what factor do the earplugs divide the sound intensity?
  • b) Find the intensity that reaches her eardrum.

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  • a) By 10001000
  • b) 8282 dB, that is 1.58×10−41.58\times 10^{-4} W/m2^2
a)

Formula sheet, Sound: β=10log⁡10II0\beta = 10\log_{10}\frac{I}{I_{0}}. A difference of two levels is the logarithm of a ratio of intensities: β1−β2=10log⁡10I1I2\beta_{1}-\beta_{2} = 10\log_{10}\frac{I_{1}}{I_{2}}.

30=10log⁡10I1I230 = 10\log_{10}\frac{I_{1}}{I_{2}} gives I1I2=103=1000\frac{I_{1}}{I_{2}} = 10^{3} = 1000.

3030 treats the decibel as a plain unit of intensity; 33 stops at the exponent, 30/1030/10, and forgets the power of ten; 1.41.4 divides the two levels as if they were proportional to the intensities, which a logarithmic scale never is.

The amplitude form of the same line of the sheet, β=20log⁡10AA0\beta = 20\log_{10}\frac{A}{A_{0}}, says that the pressure amplitude is divided by 1030/20=31.610^{30/20} = 31.6: an intensity goes as the square of an amplitude.

b)

112−30=82112 - 30 = 82 dB, so I=I0108.2=(1.0×10−12)(1.585×108)=1.58×10−4I = I_{0}10^{8.2} = (1.0\times 10^{-12})(1.585\times 10^{8}) = 1.58\times 10^{-4} W/m2^2.

Check: at 112112 dB the intensity is 1011.2I0=0.15810^{11.2}I_{0} = 0.158 W/m2^2, and a thousandth of it is the same 1.58×10−41.58\times 10^{-4} W/m2^2.

Exercise 10: Seeing details from orbit: the Rayleigh criterion

The camera of an Earth observation satellite looks straight down from an altitude of 600600 km through a circular aperture 0.500.50 m across. The engineers want it to show finer details on the ground.

  • a) Which change, on its own, improves the finest detail the camera can resolve?
  • b) Imaging at 500500 nm, find the smallest distance between two points on the ground that the camera can still resolve.

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  • a) Imaging in blue light instead of red light
  • b) 0.730.73 m
a)

Formula sheet, Interference and diffraction: Rayleigh criterion θ=1.22λD\theta = 1.22\frac{\lambda}{D}. Two points are resolved when their angular separation is at least θ\theta, so a SMALLER θ\theta is better: a shorter wavelength or a wider aperture.

Blue light has a shorter wavelength than red, so a smaller diffraction disc: this is the answer.

Infrared is LONGER than red: the discs grow and the resolution gets worse, even if haze bothers it less.

More pixels sample the blurred image more finely, but each point is still a disc of angular size 1.22λD1.22\frac{\lambda}{D}: the limit is set by the aperture, not by the detector.

Flying higher keeps the same θ\theta but spreads it over a larger distance on the ground, s=hθs = h\theta: worse.

b)

θ=1.22500×10−90.50=1.22×10−6\theta = 1.22\frac{500\times 10^{-9}}{0.50} = 1.22\times 10^{-6} rad.

Straight below, at a distance hh, the angle is small, so s=hθ=(6.00×105)(1.22×10−6)=0.73s = h\theta = (6.00\times 10^{5})(1.22\times 10^{-6}) = 0.73 m.

Sense check: such a camera can tell two parked cars apart, not two people standing side by side.

Part B: problems (/70)

Exercise 11: Two tugboats and a barge: components, dot products, work and power

Two tugboats tow a barge along a straight canal. Take the xx axis along the canal, in the direction of travel, and the yy axis across it, toward the left bank. Tug 1 pulls on the bow with a force of 4.04.0 kN at 25∘25^{\circ} to the left of the canal axis; tug 2 pulls with 3.03.0 kN at 40∘40^{\circ} to the right of it, as drawn. The barge moves at a constant 1.201.20 m/s along the axis.

The water exerts on the hull a drag along the axis and, through the keel, a sideways push. Nothing else acts horizontally.

bargexF1 = 4.0 kNF2 = 3.0 kN25°40°
  • a) Find the components of each pull and of their sum R⃗\vec R, then the magnitude of R⃗\vec R and its angle with the canal axis.
  • b) Check the magnitude of R⃗\vec R with the line of the formula sheet that gives ∣a⃗+b⃗∣2|\vec a+\vec b|^{2}, naming the angle you use.
  • c) Find the work done by each tug while the barge covers 150150 m, and the total. Which components did no work?
  • d) Find the drag and the sideways push of the water on the hull, then the net work on the barge over the 150150 m.
  • e) Find the power each tug delivers to the barge, and the total.

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  • a) F⃗1=(3.625 ; 1.690)\vec F_{1} = (3.625\,;\,1.690) kN, F⃗2=(2.298 ; −1.928)\vec F_{2} = (2.298\,;\,-1.928) kN, R⃗=(5.923 ; −0.238)\vec R = (5.923\,;\,-0.238) kN, R=5.93R = 5.93 kN at 2.3∘2.3^{\circ} to the right of the axis
  • b) Interior angle 65∘65^{\circ}: R2=4.02+3.02+2(4.0)(3.0)cos⁡65∘R^{2} = 4.0^{2}+3.0^{2}+2(4.0)(3.0)\cos 65^{\circ}, R=5.93R = 5.93 kN
  • c) W1=544W_{1} = 544 kJ, W2=345W_{2} = 345 kJ, total 888888 kJ; the components across the canal do no work
  • d) Drag 5.925.92 kN backward, sideways push 0.240.24 kN toward the left bank, net work zero
  • e) P1=4.35P_{1} = 4.35 kW, P2=2.76P_{2} = 2.76 kW, total 7.117.11 kW
a)

Each pull is resolved on the canal axes, angles measured from +x+x: +25∘+25^{\circ} for tug 1, −40∘-40^{\circ} for tug 2.

F1x=4.0cos⁡25∘=3.625F_{1x} = 4.0\cos 25^{\circ} = 3.625 kN and F1y=4.0sin⁡25∘=1.690F_{1y} = 4.0\sin 25^{\circ} = 1.690 kN.

F2x=3.0cos⁡40∘=2.298F_{2x} = 3.0\cos 40^{\circ} = 2.298 kN and F2y=−3.0sin⁡40∘=−1.928F_{2y} = -3.0\sin 40^{\circ} = -1.928 kN.

Rx=5.923R_{x} = 5.923 kN and Ry=1.690−1.928=−0.238R_{y} = 1.690 - 1.928 = -0.238 kN.

R=5.9232+0.2382=5.93R = \sqrt{5.923^{2}+0.238^{2}} = 5.93 kN, at arctan⁡0.2385.923=2.3∘\arctan\frac{0.238}{5.923} = 2.3^{\circ} to the RIGHT of the axis, since Ry<0R_{y} < 0.

Pitfall: adding the magnitudes, 7.07.0 kN, ignores the fact that the two tugs partly pull against each other across the canal.

b)

Formula sheet, General equations: ∣a⃗+b⃗∣2=a2+b2+2abcos⁡θ|\vec a+\vec b|^{2} = a^{2}+b^{2}+2ab\cos\theta, with θ\theta the interior angle between the two pulls drawn from the bow: 25∘+40∘=65∘25^{\circ}+40^{\circ} = 65^{\circ}.

R2=16.0+9.0+24.0cos⁡65∘=25.0+10.14=35.14R^{2} = 16.0+9.0+24.0\cos 65^{\circ} = 25.0+10.14 = 35.14 kN2^{2}, so R=5.93R = 5.93 kN, as in a).

Using 115∘115^{\circ}, the angle of the head to tail triangle, would give 25.0−10.14=3.85\sqrt{25.0-10.14} = 3.85 kN, less than the larger pull: impossible for two pulls less than 90∘90^{\circ} apart.

c)

Formula sheet, Work and energy: W=F⃗⋅d⃗W = \vec F\cdot\vec d, and the displacement d⃗=(150 ; 0)\vec d = (150\,;\,0) m lies along the axis.

W1=F1x(150)=3625(150)=5.44×105W_{1} = F_{1x}(150) = 3625(150) = 5.44\times 10^{5} J =544= 544 kJ, which is also Fdcos⁡25∘Fd\cos 25^{\circ}.

W2=F2x(150)=2298(150)=3.45×105W_{2} = F_{2x}(150) = 2298(150) = 3.45\times 10^{5} J =345= 345 kJ.

Total: 888888 kJ, equal to R⃗⋅d⃗=5923(150)\vec R\cdot\vec d = 5923(150), as it must be: work adds like the forces.

The yy components, 1.6901.690 kN and 1.9281.928 kN, are perpendicular to the displacement: their dot product with d⃗\vec d is zero, so they do no work. A tug pulling at a steep angle spends most of its effort holding the barge off the bank.

d)

Constant velocity, so the net force is zero (Newton's first law) in each direction.

Along xx: the drag is 5.925.92 kN, pointing backward.

Along yy: the water must push +0.238+0.238 kN, about 0.240.24 kN, toward the left bank, to cancel Ry=−0.238R_{y} = -0.238 kN.

Net work: the drag does −5923(150)=−888-5923(150) = -888 kJ, the sideways push none, so Wnet=888−888=0W_{net} = 888 - 888 = 0, which is the work energy theorem of the sheet, Wnet=ΔKE=0W_{net} = \Delta KE = 0 at constant speed. The 888888 kJ end up as heat and turbulence in the canal.

e)

Formula sheet: power =F⃗⋅v⃗= \vec F\cdot\vec v, with v⃗=(1.20 ; 0)\vec v = (1.20\,;\,0) m/s.

P1=3625(1.20)=4.35×103P_{1} = 3625(1.20) = 4.35\times 10^{3} W and P2=2298(1.20)=2.76×103P_{2} = 2298(1.20) = 2.76\times 10^{3} W, total 7.117.11 kW.

Check with c): the 150150 m take 1501.20=125\frac{150}{1.20} = 125 s, and 888×103125=7.11×103\frac{888\times 10^{3}}{125} = 7.11\times 10^{3} W.

F1F2R = 5.93 kN

Exercise 12: A snowboarder glides up a slope and slides back, solved in letters

A snowboarder reaches the foot of a straight snowy slope inclined at θ=15∘\theta = 15^{\circ} with a speed v0=8.0v_{0} = 8.0 m/s, and glides up it without pushing, then slides back down. Between board and snow, μk=0.080\mu_{k} = 0.080 and μs=0.12\mu_{s} = 0.12. Treat snowboarder and board as one block of mass mm, and neglect air resistance.

Answer each part in letters first, in terms of gg, θ\theta, μk\mu_{k} and v0v_{0}, then with numbers.

θ = 15°v0 = 8.0 m/ssnowboarder
  • a) Draw the free body diagram on the way up, and find the acceleration aupa_{up} in letters, then in numbers.
  • b) Find, in letters, the distance dd she covers up the slope before stopping. Check its dimensions, the limit μk→0\mu_{k} \to 0, and how dd varies with μk\mu_{k}. Then compute dd.
  • c) Does she slide back down? Find her acceleration adowna_{down} on the way down.
  • d) Find, in letters, her speed vbackv_{back} when she is back at the foot of the slope, check the limit μk→0\mu_{k} \to 0, and compute it.
  • e) Find the time up and the time down. Which is longer, and why?

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  • a) aup=g(sin⁡θ+μkcos⁡θ)=3.30a_{up} = g(\sin\theta+\mu_{k}\cos\theta) = 3.30 m/s2^2, down the slope
  • b) d=v022g(sin⁡θ+μkcos⁡θ)=9.71d = \frac{v_{0}^{2}}{2g(\sin\theta+\mu_{k}\cos\theta)} = 9.71 m
  • c) Yes, since tan⁡15∘=0.27>μs\tan 15^{\circ} = 0.27 > \mu_{s}; adown=g(sin⁡θ−μkcos⁡θ)=1.78a_{down} = g(\sin\theta-\mu_{k}\cos\theta) = 1.78 m/s2^2
  • d) vback=v0sin⁡θ−μkcos⁡θsin⁡θ+μkcos⁡θ=5.88v_{back} = v_{0}\sqrt{\frac{\sin\theta-\mu_{k}\cos\theta}{\sin\theta+\mu_{k}\cos\theta}} = 5.88 m/s
  • e) tup=2.43t_{up} = 2.43 s, tdown=3.30t_{down} = 3.30 s: the way down is longer
a)

Axes: xx up the slope, yy perpendicular to it. Three forces: the weight mgmg, straight down; the normal force FNF_{N}, perpendicular to the snow; kinetic friction FfrF_{fr}, DOWN the slope, because the board slides up it.

Along yy, no acceleration: FN=mgcos⁡θF_{N} = mg\cos\theta, so Ffr=μkmgcos⁡θF_{fr} = \mu_{k}mg\cos\theta (formula sheet, Dynamics).

Along xx: −mgsin⁡θ−μkmgcos⁡θ=ma-mg\sin\theta-\mu_{k}mg\cos\theta = ma, so the acceleration points down the slope with magnitude aup=g(sin⁡θ+μkcos⁡θ)a_{up} = g(\sin\theta+\mu_{k}\cos\theta).

aup=9.81(0.2588+0.080×0.9659)=9.81(0.3361)=3.30a_{up} = 9.81(0.2588+0.080\times 0.9659) = 9.81(0.3361) = 3.30 m/s2^2. The mass cancels.

b)

Formula sheet, Kinematics: v2=v02+2a(x−x0)v^{2} = v_{0}^{2}+2a(x-x_{0}) with v=0v = 0 at the highest point and a=−aupa = -a_{up}:

d=v022g(sin⁡θ+μkcos⁡θ)\displaystyle d = \frac{v_{0}^{2}}{2g(\sin\theta+\mu_{k}\cos\theta)}

Dimensions: (m/s)2m/s2=\frac{(\text{m/s})^{2}}{\text{m/s}^{2}} = m, a length, since sines, cosines and μk\mu_{k} have no unit.

Limit μk→0\mu_{k} \to 0: d=v022gsin⁡θd = \frac{v_{0}^{2}}{2g\sin\theta}, so the height gained is dsin⁡θ=v022gd\sin\theta = \frac{v_{0}^{2}}{2g}, all the kinetic energy turned into potential energy, as the energy line of the sheet predicts.

Variation: μk\mu_{k} sits in the denominator, so more friction means a shorter climb, as it should.

d=8.022(3.297)=9.71d = \frac{8.0^{2}}{2(3.297)} = 9.71 m, against 12.612.6 m without friction.

c)

At the top she is momentarily at rest, and static friction could hold her only if mgsin⁡θ≤μsmgcos⁡θmg\sin\theta \le \mu_{s}mg\cos\theta, that is tan⁡θ≤μs\tan\theta \le \mu_{s}.

tan⁡15∘=0.268>0.12\tan 15^{\circ} = 0.268 > 0.12: the slope wins, she slides back.

On the way down friction points UP the slope, against the new sliding: adown=g(sin⁡θ−μkcos⁡θ)=9.81(0.2588−0.0773)=1.78a_{down} = g(\sin\theta-\mu_{k}\cos\theta) = 9.81(0.2588-0.0773) = 1.78 m/s2^2.

Pitfall: keeping friction pointing down the slope after the turn around gives 3.303.30 m/s2^2 again, as if friction helped her slide.

d)

Same line of the sheet, from rest over the distance dd: vback2=2adowndv_{back}^{2} = 2a_{down}d. Replacing dd by its expression from b):

vback=v0sin⁡θ−μkcos⁡θsin⁡θ+μkcos⁡θ\displaystyle v_{back} = v_{0}\sqrt{\frac{\sin\theta-\mu_{k}\cos\theta}{\sin\theta+\mu_{k}\cos\theta}}

Dimensions: a speed times a pure number. Limit μk→0\mu_{k} \to 0: the square root becomes 11 and she comes back at v0v_{0}, the frictionless round trip.

vback=8.00.18150.3361=8.0(0.7350)=5.88v_{back} = 8.0\sqrt{\frac{0.1815}{0.3361}} = 8.0(0.7350) = 5.88 m/s.

Energy check, per kilogram: she loses 12(8.02−5.882)=14.7\frac{1}{2}(8.0^{2}-5.88^{2}) = 14.7 J/kg, and friction takes μkgcos⁡θ(2d)=0.758(19.41)=14.7\mu_{k}g\cos\theta(2d) = 0.758(19.41) = 14.7 J/kg over the round trip.

e)

tup=v0aup=8.03.297=2.43t_{up} = \frac{v_{0}}{a_{up}} = \frac{8.0}{3.297} = 2.43 s, and from rest d=12adownt2d = \frac{1}{2}a_{down}t^{2} gives tdown=2dadown=2(9.71)1.781=3.30t_{down} = \sqrt{\frac{2d}{a_{down}}} = \sqrt{\frac{2(9.71)}{1.781}} = 3.30 s.

In letters, tdowntup=aupadown=1.36\frac{t_{down}}{t_{up}} = \sqrt{\frac{a_{up}}{a_{down}}} = 1.36: the same distance is covered with a smaller acceleration on the way down, because friction adds to gravity going up and subtracts from it coming down.

With μk→0\mu_{k} \to 0 the two accelerations are equal and so are the two times, the symmetry of a frictionless slope.

15°mgFNFfra
On the way up: friction points DOWN the slope, with the weight's component, and the acceleration points down the slope. The friction arrow is drawn at three times its scale.
15°mgFNFfra
On the way down: friction has turned round and points UP the slope; the acceleration still points down the slope but is smaller.

Exercise 13: A toy car on a vertical loop, solved in letters

A toy car of mass m=0.050m = 0.050 kg is released from rest at point A, at a height hh above the bottom of a track that ends in a vertical loop of radius R=0.20R = 0.20 m (figure not to scale). Friction, air resistance and the rotation of the wheels are neglected, so the car is treated as a point that slides.

Work in letters first, in terms of mm, gg, RR and hh, then with numbers.

ARTBh
  • a) Find, in letters, the speed vTv_{T} of the car at the top T of the loop, and the condition on vTv_{T} for the car to stay on the track there.
  • b) Deduce the smallest release height hminh_{min}, in letters and in numbers. Check its dimensions, and say why the mass does not appear.
  • c) The car is released from hminh_{min}. Find the normal force at the bottom B of the loop, in letters and in newtons.
  • d) The car is released from h=0.60h = 0.60 m. Find the normal force at the top.
  • e) A friend releases the car from h=2Rh = 2R, reasoning that this is just enough to reach the top. Show that the car leaves the track before the top, and find the height at which it does.

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  • a) vT2=2g(h−2R)v_{T}^{2} = 2g(h-2R); it stays on the track if vT2≥gRv_{T}^{2} \ge gR
  • b) hmin=5R2=0.50h_{min} = \frac{5R}{2} = 0.50 m
  • c) FN=mg(1+2hR)=6mg=2.94F_{N} = mg\left(1+\frac{2h}{R}\right) = 6mg = 2.94 N
  • d) FN=mg(2hR−5)=mg=0.49F_{N} = mg\left(\frac{2h}{R}-5\right) = mg = 0.49 N
  • e) It leaves where sin⁡α=23\sin\alpha = \frac{2}{3}, at a height 5R3=0.333\frac{5R}{3} = 0.333 m, below the top at 0.400.40 m
a)

Only gravity does work, so KE+PEKE + PE is conserved (formula sheet, extended work energy principle with Wnon−cons.=0W_{non-cons.} = 0): mgh=mg(2R)+12mvT2mgh = mg(2R)+\frac{1}{2}mv_{T}^{2}, which gives vT2=2g(h−2R)v_{T}^{2} = 2g(h-2R).

At T the centre of the loop is BELOW the car, so the net force points down: mg+FN=mvT2Rmg+F_{N} = \frac{mv_{T}^{2}}{R} (formula sheet, a=v2ra = \frac{v^{2}}{r}).

The track can push but never pull, so FN≥0F_{N} \ge 0, that is vT2≥gRv_{T}^{2} \ge gR.

b)

2g(h−2R)≥gR2g(h-2R) \ge gR gives h≥2R+R2h \ge 2R+\frac{R}{2}:

hmin=5R2=2.5(0.20)=0.50h_{min} = \frac{5R}{2} = 2.5(0.20) = 0.50 m

Dimensions: RR is a length, so hminh_{min} is a length.

The mass multiplies every term of the energy balance and of Newton's law, so it cancels: a heavier car needs the same height. Variation: a loop twice as large needs a start twice as high.

Pitfall: h=2Rh = 2R is enough to REACH the height of the top only if the car could arrive there at rest, and at rest it cannot follow a curved path. See e).

c)

At B the centre is ABOVE the car: FN−mg=mvB2RF_{N}-mg = \frac{mv_{B}^{2}}{R}, with vB2=2ghv_{B}^{2} = 2gh from energy, so FN=mg(1+2hR)F_{N} = mg\left(1+\frac{2h}{R}\right).

Limit h→0h \to 0: FN=mgF_{N} = mg, the car at rest at the bottom, as expected.

With h=5R2h = \frac{5R}{2}: FN=mg(1+5)=6mg=6(0.050)(9.81)=2.94F_{N} = mg(1+5) = 6mg = 6(0.050)(9.81) = 2.94 N, six times the weight of the car.

d)

vT2=2(9.81)(0.60−0.40)=3.92v_{T}^{2} = 2(9.81)(0.60-0.40) = 3.92 m2^2/s2^2, and FN=m(vT2R−g)=0.050(19.62−9.81)=0.49F_{N} = m\left(\frac{v_{T}^{2}}{R}-g\right) = 0.050(19.62-9.81) = 0.49 N.

In letters FN=mg(2hR−5)F_{N} = mg\left(\frac{2h}{R}-5\right), and 2(0.60)0.20−5=1\frac{2(0.60)}{0.20}-5 = 1: at the top the track pushes down on the car with exactly its weight.

Check: at h=hminh = h_{min} the same formula gives FN=0F_{N} = 0, the result of b).

e)

Take a point of the upper half of the loop at an angle α\alpha above the horizontal through the centre: its height is R(1+sin⁡α)R(1+\sin\alpha).

Energy from h=2Rh = 2R: v2=2g(2R−R−Rsin⁡α)=2gR(1−sin⁡α)v^{2} = 2g\left(2R-R-R\sin\alpha\right) = 2gR(1-\sin\alpha).

Toward the centre act FNF_{N} and the part mgsin⁡αmg\sin\alpha of the weight: FN+mgsin⁡α=mv2RF_{N}+mg\sin\alpha = \frac{mv^{2}}{R}, so FN=mg(2−3sin⁡α)F_{N} = mg(2-3\sin\alpha).

FNF_{N} reaches zero when sin⁡α=23\sin\alpha = \frac{2}{3}, α=41.8∘\alpha = 41.8^{\circ}, at a height R(1+23)=5R3=0.333R\left(1+\frac{2}{3}\right) = \frac{5R}{3} = 0.333 m, while the top is at 0.400.40 m.

There the car leaves the track still moving, and falls across the inside of the loop as a projectile.

Exercise 14: A fireworks shell that bursts at the top: momentum and the centre of mass

A fireworks shell of mass 1.201.20 kg is fired from ground level at 40.040.0 m/s, 70.0∘70.0^{\circ} above the horizontal. At the top of its path a small charge splits it into two pieces: piece A, 0.4000.400 kg, is left at rest just after the burst, and piece B, 0.8000.800 kg, moves off horizontally. The mass of the charge and air resistance are neglected, and the ground is level.

burst at the top40.0 m/s at 70°x (m)y (m)
  • a) Find the time to reach the top, the height of the top, and its horizontal distance from the launch point.
  • b) Find the velocity of piece B just after the burst.
  • c) Find where each piece lands.
  • d) Find where the centre of mass of the two pieces is when they land, and compare it with the range the shell would have had without the burst.
  • e) Find the kinetic energy just before and just after the burst. Where does the difference come from?

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  • a) t=3.83t = 3.83 s, H=72.0H = 72.0 m, at x=52.4x = 52.4 m
  • b) 20.520.5 m/s, horizontal, forward
  • c) A at 52.452.4 m, B at 131.0131.0 m
  • d) xCOM=104.8x_{COM} = 104.8 m, exactly the range without the burst
  • e) 112.3112.3 J before, 168.4168.4 J after: 56.156.1 J from the chemical energy of the charge
a)

Components: vx=40.0cos⁡70.0∘=13.68v_{x} = 40.0\cos 70.0^{\circ} = 13.68 m/s and vy0=40.0sin⁡70.0∘=37.59v_{y0} = 40.0\sin 70.0^{\circ} = 37.59 m/s.

At the top vy=0v_{y} = 0: t=vy0g=37.599.81=3.83t = \frac{v_{y0}}{g} = \frac{37.59}{9.81} = 3.83 s (formula sheet, v=v0+atv = v_{0}+at).

H=vy022g=37.5922(9.81)=72.0H = \frac{v_{y0}^{2}}{2g} = \frac{37.59^{2}}{2(9.81)} = 72.0 m, and x=vxt=13.68(3.83)=52.4x = v_{x}t = 13.68(3.83) = 52.4 m.

b)

The burst lasts a very short time and its forces are internal, so the horizontal momentum is conserved across it (formula sheet, p1,i+p2,i=p1,f+p2,fp_{1,i}+p_{2,i} = p_{1,f}+p_{2,f}).

Just before, the whole shell moves horizontally at 13.6813.68 m/s: 1.20(13.68)=0.400(0)+0.800 vB1.20(13.68) = 0.400(0)+0.800\,v_{B}, so vB=20.5v_{B} = 20.5 m/s, forward.

In letters vB=MmBvx=1.5vxv_{B} = \frac{M}{m_{B}}v_{x} = 1.5v_{x}.

c)

Both pieces start at 72.072.0 m with no vertical velocity, so both fall for the same 3.833.83 s, the time of the rise, by the symmetry of the vertical motion.

A falls straight down and lands at 52.452.4 m.

B lands at 52.4+20.52(3.83)=52.4+78.6=131.052.4+20.52(3.83) = 52.4+78.6 = 131.0 m.

d)

Formula sheet, xCOM=m1x1+m2x2m1+m2=0.400(52.4)+0.800(131.0)1.20=104.8x_{COM} = \frac{m_{1}x_{1}+m_{2}x_{2}}{m_{1}+m_{2}} = \frac{0.400(52.4)+0.800(131.0)}{1.20} = 104.8 m.

Without the burst, the range equation of the sheet gives R=v2sin⁡2θg=40.02sin⁡140∘9.81=104.8R = \frac{v^{2}\sin 2\theta}{g} = \frac{40.0^{2}\sin 140^{\circ}}{9.81} = 104.8 m: the same point.

The burst is internal; the only external force is gravity, so the centre of mass keeps following the parabola of the unexploded shell. This is visible here because both pieces land at the same instant.

e)

Before: 12(1.20)(13.68)2=112.3\frac{1}{2}(1.20)(13.68)^{2} = 112.3 J. After: 12(0.800)(20.52)2=168.4\frac{1}{2}(0.800)(20.52)^{2} = 168.4 J.

The gain, 56.156.1 J, is chemical energy of the charge turned into kinetic energy: momentum is conserved in the burst, kinetic energy is not. A burst is a perfectly inelastic collision played backward.

Pitfall: conserving kinetic energy instead of momentum would give vB=1.200.800(13.68)=16.8v_{B} = \sqrt{\frac{1.20}{0.800}}(13.68) = 16.8 m/s and a landing point that misses the centre of mass rule.

102030405060708090100110120130140102030405060708090A, 0.400 kgB, 0.800 kg52.4 m131.0 mcentre of mass lands at 104.8 m (open dot)x (m)y (m)

Exercise 15: A cue ball that slides, then rolls: torque, rolling and energy in letters

A cue ball, a uniform solid sphere of mass M=0.170M = 0.170 kg and radius R=2.86R = 2.86 cm, is struck at the height of its centre and leaves the cue sliding at v0=2.80v_{0} = 2.80 m/s without any spin. The coefficient of kinetic friction between ball and cloth is μk=0.20\mu_{k} = 0.20. Given: a uniform solid sphere has I=25MR2I = \frac{2}{5}MR^{2} about its centre.

Answer in letters first, in terms of gg, μk\mu_{k}, v0v_{0} and RR, then with numbers.

v0 = 2.80 m/sno spin at releasecloth
  • a) Name the forces on the sliding ball. Find, in letters, the deceleration aa of its centre and its angular acceleration α\alpha, then their values.
  • b) The ball starts rolling without slipping when v=Rωv = R\omega. Find, in letters, the instant t1t_{1} and the speed v1v_{1} at which this happens. Check the dimensions of t1t_{1} and its limit μk→0\mu_{k} \to 0. Compute both.
  • c) How far does the ball slide before it rolls?
  • d) Find the kinetic energy at the start and once the ball rolls, with the rotational share. Where did the difference go?
  • e) A heavier ball of the same radius is struck at the same speed on the same cloth: is its final rolling speed larger, smaller or the same? And on a cloth with twice the friction?

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  • a) a=μkg=1.96a = \mu_{k}g = 1.96 m/s2^2 backward, α=5μkg2R=171.5\alpha = \frac{5\mu_{k}g}{2R} = 171.5 rad/s2^2, spinning it forward
  • b) t1=2v07μkg=0.408t_{1} = \frac{2v_{0}}{7\mu_{k}g} = 0.408 s, v1=57v0=2.00v_{1} = \frac{5}{7}v_{0} = 2.00 m/s
  • c) d=12v0249μkg=0.979d = \frac{12v_{0}^{2}}{49\mu_{k}g} = 0.979 m
  • d) 0.6660.666 J at the start, 0.4760.476 J rolling, of which 0.1360.136 J, that is 27\frac{2}{7}, is rotational; 0.1900.190 J became heat
  • e) The same 2.002.00 m/s in both cases; with twice the friction it is reached in half the time
a)

Three forces: the weight MgMg at the centre, the normal force FN=MgF_{N} = Mg at the contact point, and kinetic friction μkMg\mu_{k}Mg at the contact point, BACKWARD, because the bottom of the ball slides forward over the cloth.

Translation, Newton's second law: μkMg=Ma\mu_{k}Mg = Ma, so a=μkg=0.20(9.81)=1.96a = \mu_{k}g = 0.20(9.81) = 1.96 m/s2^2, slowing the centre.

Rotation about the centre, formula sheet τ=F⊥r\tau = F_{\perp}r and τ=Iα\tau = I\alpha: the weight and the normal force pass through the centre and have no torque; friction has a lever arm RR, so μkMgR=25MR2α\mu_{k}MgR = \frac{2}{5}MR^{2}\alpha.

α=5μkg2R=5(1.962)2(0.0286)=171.5\alpha = \frac{5\mu_{k}g}{2R} = \frac{5(1.962)}{2(0.0286)} = 171.5 rad/s2^2, in the sense that makes the ball roll forward.

The same force slows the centre and spins the ball up: friction converts sliding into rolling.

b)

Constant accelerations (formula sheet, v=v0+atv = v_{0}+at and ω=ω0+αt\omega = \omega_{0}+\alpha t): v=v0−μkgtv = v_{0}-\mu_{k}gt and Rω=Rαt=52μkgtR\omega = R\alpha t = \frac{5}{2}\mu_{k}gt.

They meet when v0−μkgt=52μkgtv_{0}-\mu_{k}gt = \frac{5}{2}\mu_{k}gt:

t1=2v07μkgt_{1} = \frac{2v_{0}}{7\mu_{k}g} and v1=v0−μkgt1=57v0v_{1} = v_{0}-\mu_{k}gt_{1} = \frac{5}{7}v_{0}

Dimensions: m/sm/s2=\frac{\text{m/s}}{\text{m/s}^{2}} = s. Limit μk→0\mu_{k} \to 0: t1t_{1} grows without bound, a ball on frictionless cloth slides forever and never starts turning. More friction, sooner rolling.

t1=2(2.80)7(0.20)(9.81)=0.408t_{1} = \frac{2(2.80)}{7(0.20)(9.81)} = 0.408 s and v1=57(2.80)=2.00v_{1} = \frac{5}{7}(2.80) = 2.00 m/s, with ω1=2.000.0286=69.9\omega_{1} = \frac{2.00}{0.0286} = 69.9 rad/s, which is indeed αt1\alpha t_{1}.

Once it rolls, the contact point no longer slides, kinetic friction stops, and the ball keeps 2.002.00 m/s (rolling resistance neglected).

c)

Formula sheet: v2=v02+2a(x−x0)v^{2} = v_{0}^{2}+2a(x-x_{0}), so d=v02−v122μkg=12v0249μkgd = \frac{v_{0}^{2}-v_{1}^{2}}{2\mu_{k}g} = \frac{12v_{0}^{2}}{49\mu_{k}g}.

d=2.802−2.0022(1.962)=7.84−4.003.924=0.979d = \frac{2.80^{2}-2.00^{2}}{2(1.962)} = \frac{7.84-4.00}{3.924} = 0.979 m, about half the length of a pool table.

d)

Start: all translational, 12(0.170)(2.80)2=0.666\frac{1}{2}(0.170)(2.80)^{2} = 0.666 J.

Rolling: translational 12Mv12=0.340\frac{1}{2}Mv_{1}^{2} = 0.340 J and rotational 12Iω12=12⋅25MR2v12R2=15Mv12=0.136\frac{1}{2}I\omega_{1}^{2} = \frac{1}{2}\cdot\frac{2}{5}MR^{2}\frac{v_{1}^{2}}{R^{2}} = \frac{1}{5}Mv_{1}^{2} = 0.136 J, total 0.4760.476 J. The rotational share is 1/57/10=27\frac{1/5}{7/10} = \frac{2}{7}, whatever the speed.

The missing 0.1900.190 J were turned into heat by kinetic friction while the contact point slid over the cloth.

e)

v1=57v0v_{1} = \frac{5}{7}v_{0} contains neither MM, nor μk\mu_{k}, nor RR.

A heavier ball: a=μkga = \mu_{k}g and α=5μkg2R\alpha = \frac{5\mu_{k}g}{2R} do not depend on MM, so the motion is identical and the final speed is the same 2.002.00 m/s.

Twice the friction: the same 2.002.00 m/s, reached in half the time, 0.2040.204 s, after half the distance, 0.4890.489 m, since t1t_{1} and dd go as 1μk\frac{1}{\mu_{k}}.

Pitfall: a heavier ball or a rougher cloth does not mean a slower roll; friction only decides how soon the rolling starts.

0.10.20.30.40.50.60.511.522.53v of the centreRωrolling: v = Rω = 2.00 m/st (s)speed (m/s)
Speed of the centre (teal) and RωR\omega (orange) against time: one falls, the other grows, and they meet at 0.4080.408 s, after which the ball rolls at 2.002.00 m/s.

Exercise 16: A tuning fork walked toward a wall: oscillation, Doppler shift and beats

A tuning fork vibrates at f=440f = 440 Hz, and the tip of each prong moves in simple harmonic motion with an amplitude of 0.400.40 mm. Take the speed of sound in the still air of the room as v=330v = 330 m/s.

A student holding the sounding fork walks at a steady u=1.50u = 1.50 m/s straight toward a large flat wall, as drawn. She hears at the same time the sound that comes straight from the fork and its echo from the wall.

fork 440 Hzu = 1.50 m/swall
  • a) Find the maximum speed and the maximum acceleration of a prong tip, and compare the acceleration with gg.
  • b) Find the wavelength of the sound when the student stands still.
  • c) Find, in letters then in numbers, the frequency received by the wall while she walks.
  • d) The wall sends back what it receives. Find, in letters, the frequency fef_{e} of the echo she hears, then the beat frequency between the echo and the direct sound. Check the dimensions and the limit u→0u \to 0, and compute both.
  • e) Walking faster, she counts 6.06.0 beats per second. What is her speed?

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  • a) vmax=1.11v_{max} = 1.11 m/s, amax=3.06×103a_{max} = 3.06\times 10^{3} m/s2^2, about 312g312g
  • b) λ=0.750\lambda = 0.750 m
  • c) fw=fvv−u=442.0f_{w} = f\frac{v}{v-u} = 442.0 Hz
  • d) fe=fv+uv−u=444.0f_{e} = f\frac{v+u}{v-u} = 444.0 Hz; fb=2ufv−u=4.02f_{b} = \frac{2uf}{v-u} = 4.02 Hz
  • e) u=fbv2f+fb=2.23u = \frac{f_{b}v}{2f+f_{b}} = 2.23 m/s
a)

Formula sheet, Simple harmonic motion: vmax=Aωv_{max} = A\omega and amax=Aω2a_{max} = A\omega^{2}, with ω=2πf=2π(440)=2765\omega = 2\pi f = 2\pi(440) = 2765 rad/s.

vmax=(0.40×10−3)(2765)=1.11v_{max} = (0.40\times 10^{-3})(2765) = 1.11 m/s and amax=(0.40×10−3)(2765)2=3.06×103a_{max} = (0.40\times 10^{-3})(2765)^{2} = 3.06\times 10^{3} m/s2^2.

amaxg=30589.81=312\frac{a_{max}}{g} = \frac{3058}{9.81} = 312: a prong tip that moves less than half a millimetre accelerates at over three hundred gg, because the acceleration goes as the SQUARE of the frequency.

b)

Formula sheet, Waves: v=fλv = f\lambda, so λ=330440=0.750\lambda = \frac{330}{440} = 0.750 m.

The fork sets the frequency, the air sets the speed, and the wavelength follows.

c)

The fork is a source moving toward a wall at rest. Formula sheet, Sound, moving source: f′=fvwavevwave±vsourcef' = f\frac{v_{wave}}{v_{wave}\pm v_{source}}, with the minus sign because the source approaches:

fw=fvv−u\displaystyle f_{w} = f\frac{v}{v-u}

fw=440330330−1.50=440330328.5=442.0f_{w} = 440\frac{330}{330-1.50} = 440\frac{330}{328.5} = 442.0 Hz. In front of the walking fork the crests are squeezed to v−uf=0.7466\frac{v-u}{f} = 0.7466 m.

d)

The wall now acts as a source at rest emitting fwf_{w}, and she is an observer moving toward it. Formula sheet, moving observer: f′=fvwave±vobsvwavef' = f\frac{v_{wave}\pm v_{obs}}{v_{wave}}, plus sign since she approaches:

fe=fwv+uv=fv+uv−u\displaystyle f_{e} = f_{w}\frac{v+u}{v} = f\frac{v+u}{v-u}

The direct sound comes from a fork that moves WITH her: no relative motion, she hears 440440 Hz. Formula sheet: fb=∣f1−f2∣f_{b} = |f_{1}-f_{2}|, so

fb=fv+uv−u−f=2ufv−u\displaystyle f_{b} = f\frac{v+u}{v-u}-f = \frac{2uf}{v-u}

Dimensions: (m/s)(Hz)m/s=\frac{(\text{m/s})(\text{Hz})}{\text{m/s}} = Hz. Limit u→0u \to 0: fb=0f_{b} = 0, standing still she hears the echo at 440440 Hz and no beats. Walking faster gives faster beats.

fe=440331.5328.5=444.0f_{e} = 440\frac{331.5}{328.5} = 444.0 Hz and fb=2(1.50)(440)328.5=4.02f_{b} = \frac{2(1.50)(440)}{328.5} = 4.02 Hz.

Pitfall: applying a single Doppler shift gives 2.02.0 beats per second. The wall is first an observer, then a source: the shift happens twice.

e)

Solve fb(v−u)=2uff_{b}(v-u) = 2uf for uu: u=fbv2f+fb=6.0(330)880+6.0=2.23u = \frac{f_{b}v}{2f+f_{b}} = \frac{6.0(330)}{880+6.0} = 2.23 m/s, a brisk walk.

Check with the approximation fb≈2ufvf_{b} \approx \frac{2uf}{v}, fine since uu is tiny next to vv: u≈6.0(330)880=2.25u \approx \frac{6.0(330)}{880} = 2.25 m/s, close.

Exercise 17: Wave optics in three scenes: an insect wing, a CD and a polarized screen

SCENE 1. The transparent wing of an insect is a thin film of chitin, of index n=1.56n = 1.56 and thickness t=400t = 400 nm, with air on both sides. White light, from 400400 to 700700 nm in air, falls on it almost along the normal; the rays of the figure are tilted only so that they can be told apart. A reflection off a medium of HIGHER index turns the wave upside down, a shift of half a wavelength; a reflection off a medium of lower index does not. In the film light travels at v=cnv = \frac{c}{n} (formula sheet), so its wavelength there is λn\frac{\lambda}{n}.

SCENE 2. A compact disc reflects light like a grating whose lines are its tracks, d=1.60d = 1.60 µm apart; a DVD has tracks 0.740.74 µm apart. A green laser pointer, 532532 nm, shines on each at normal incidence.

SCENE 3. A phone screen sends out light that is linearly polarized along its long edge, held vertical. A viewer wears polarizing sunglasses whose transmission axis is vertical when her head is upright. Malus's law, given: I=I0cos⁡2θI = I_{0}\cos^{2}\theta for polarized light meeting a polarizer at an angle θ\theta to its axis.

white light12chitin, n = 1.56airairt = 400 nm
  • a) Scene 1. Count the half wavelength shifts of rays 1 and 2, write the condition for strong reflection, and find the visible wavelength that the wing reflects most strongly.
  • b) Scene 1. Find the visible wavelengths that the wing hardly reflects at all. What colour does the wing show in reflected light?
  • c) Scene 2. Find the angles of the bright spots that the CD sends back, and how many spots there are in all.
  • d) Scene 2. Same questions for the DVD. Which of the two spreads the colours of white light the most?
  • e) Scene 3. She tilts her head by 60∘60^{\circ}. What fraction of the light of the screen reaches her eyes? At what tilt does she receive half of it?

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  • a) One shift between the rays; 2nt=(m+12)λ2nt = \left(m+\frac{1}{2}\right)\lambda; λ=499\lambda = 499 nm
  • b) 2nt=mλ2nt = m\lambda: 624624 nm and 416416 nm are suppressed; the wing looks blue-green
  • c) 19.4∘19.4^{\circ}, 41.7∘41.7^{\circ}, 85.9∘85.9^{\circ} on each side; 77 spots
  • d) Only 46.0∘46.0^{\circ} on each side; 33 spots; the DVD spreads the colours more
  • e) cos⁡260∘=0.25\cos^{2}60^{\circ} = 0.25; half at 45∘45^{\circ}
a)

Ray 1 reflects off the top face, from air onto chitin, a higher index: one half wavelength shift. Ray 2 reflects off the bottom face, from chitin onto air, a lower index: no shift.

The rays thus differ by one half wavelength from the reflections, plus the extra path 2t2t inside the film, where the wavelength is λn\frac{\lambda}{n}. They come back in step, and reflection is strong, when 2t=(m+12)λn2t = \left(m+\frac{1}{2}\right)\frac{\lambda}{n}:

λ=2ntm+12\lambda = \frac{2nt}{m+\frac{1}{2}} with 2nt=2(1.56)(400)=12482nt = 2(1.56)(400) = 1248 nm

m=0m = 0: 24962496 nm; m=1m = 1: 832832 nm; m=2m = 2: 499499 nm; m=3m = 3: 357357 nm. Only 499499 nm falls between 400400 and 700700 nm.

Pitfall: forgetting the half wavelength shift swaps the bright and the dark colours of b).

b)

The rays cancel when 2nt=mλ2nt = m\lambda, that is λ=1248m\lambda = \frac{1248}{m} nm: 12481248, 624624, 416416, 312312 nm. In the visible: 624624 nm, orange red, and 416416 nm, violet.

With red and violet removed and 499499 nm reinforced, the wing shines blue-green.

Pitfall: using λ\lambda instead of λn\frac{\lambda}{n} in the film moves every answer by the factor 1.561.56.

c)

Formula sheet, two slit maxima, which hold for a grating too: dsin⁡θm=mλd\sin\theta_{m} = m\lambda, so sin⁡θm=m532×10−91.60×10−6=0.3325 m\sin\theta_{m} = m\frac{532\times 10^{-9}}{1.60\times 10^{-6}} = 0.3325\,m.

m=1m = 1: 19.4∘19.4^{\circ}; m=2m = 2: sin⁡θ=0.665\sin\theta = 0.665, 41.7∘41.7^{\circ}; m=3m = 3: sin⁡θ=0.9975\sin\theta = 0.9975, 85.9∘85.9^{\circ}, almost along the disc; m=4m = 4 would need sin⁡θ=1.33\sin\theta = 1.33, impossible.

Spots: m=0m = 0 straight back, and m=±1,±2,±3m = \pm 1, \pm 2, \pm 3: 77 in all.

d)

DVD: sin⁡θm=m532×10−90.74×10−6=0.719 m\sin\theta_{m} = m\frac{532\times 10^{-9}}{0.74\times 10^{-6}} = 0.719\,m. m=1m = 1: 46.0∘46.0^{\circ}; m=2m = 2 would need 1.441.44: impossible. Spots: m=0,±1m = 0, \pm 1, so 33.

Closer tracks, larger angles: at first order, 450450 nm and 650650 nm leave the CD at 16.3∘16.3^{\circ} and 24.0∘24.0^{\circ}, 7.6∘7.6^{\circ} apart, and the DVD at 37.5∘37.5^{\circ} and 61.4∘61.4^{\circ}, 24.0∘24.0^{\circ} apart. The DVD spreads the colours about three times more.

e)

The light of the screen is already polarized, so Malus's law applies directly: II0=cos⁡260∘=0.25\frac{I}{I_{0}} = \cos^{2}60^{\circ} = 0.25.

Half: cos⁡2θ=12\cos^{2}\theta = \frac{1}{2}, cos⁡θ=0.707\cos\theta = 0.707, θ=45∘\theta = 45^{\circ}.

Pitfall: cos⁡60∘=0.5\cos 60^{\circ} = 0.5 forgets the square; the law is in intensity, and intensity goes as the square of the field.

Unpolarized light, such as daylight, would lose half whatever the tilt: tilting matters here only because the screen sends polarized light.

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