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

Corrected exercises: lab measurements, uncertainties and graphical analysis (203-SN3-RE)

Here are fifteen corrected exercises on measurement and uncertainty in the waves and modern physics lab, course 203-SN3-RE (formerly 203-NYC) of the revised Natural Science program (200.B1). The program prescribes this experimental component in all three physics courses, but it is practised on the setups of each one: here, the goniometer, the diffraction grating, the sound tube, the polarizers, the radioactivity counter and the spectral lamp.

Part A lays down the rules for the quantities of this course: the vernier, the angle measured on both sides of the beam, fractional exponents, the extreme-values method and the differential method with its angles in radians. Part B processes the data: counting statistics, regressions and linearizations, extreme lines. Part C revisits what recurs from one lab to the next and ends on the two faces of one problem, a small difference that a setup can measure directly, and another that has to be wrested from the noise by patience.

The thread of the set: in this course, almost every interesting quantity is either tiny, a wavelength or a frequency shift, or random by nature, a count of decays. Two consequences. First, the uncertainty is no longer read off the instrument, it is PREDICTED, by the square root of the number of counts or by the derivative of a sine. Second, you never get a small quantity by subtracting two large ones: you measure it directly, or you count long enough for it to emerge from the noise.

15 corrected exercises • 150 points • 225 minutes

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

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Course recap

  • • Vernier: the smallest readable division is the gap between one vernier division and one division of the main scale. For a fiftieths vernier it is 0.020.02 mm; on a goniometer with thirty divisions, the arcminute.
  • • Writing a result: x=(xˉ±Δx)x=(\bar x\pm\Delta x) unit; the uncertainty to one significant figure, two if it starts with 11, and the value rounded to the same decimal place.
  • • Sum or difference: Δ(x±y)=Δx+Δy\Delta(x\pm y)=\Delta x+\Delta y, ABSOLUTE uncertainties. A difference is only dangerous if its result is SMALL compared with the terms.
  • • Product, quotient, power: Δzz=∣a∣Δxx+∣b∣Δyy\dfrac{\Delta z}{z}=|a|\dfrac{\Delta x}{x}+|b|\dfrac{\Delta y}{y} for z=kxaybz=kx^{a}y^{b}. A square doubles the relative uncertainty, a square root halves it.
  • • Differential method: Δz≈∣∂z∂x∣Δx+…\Delta z\approx\left|\dfrac{\partial z}{\partial x}\right|\Delta x+\ldots, and any ANGULAR uncertainty is converted to RADIANS first.
  • • Counting: the uncertainty of a count of NN events is N\sqrt{N}, so the relative uncertainty is 1N\dfrac{1}{\sqrt{N}}. It is predicted without repeating, and it takes four times as many counts to halve it.
  • • Background: a SYSTEMATIC error, which is subtracted and not averaged. On a semi-logarithmic plot, an upward curvature betrays a forgotten additive term.
  • • Grating: dsin⁡θ=mλd\sin\theta=m\lambda; resolving power R=λΔλmin=mNR=\dfrac{\lambda}{\Delta\lambda_{min}}=mN with NN the number of ILLUMINATED lines. Separating two lines and locating a line are two different qualities.
  • • Linearizing: u=U0e−t/τu=U_{0}e^{-t/\tau} gives ln⁡u\ln u linear in tt; I=I0cos⁡2θI=I_{0}\cos^{2}\theta gives II linear in cos⁡2θ\cos^{2}\theta; eVs=hcλeV_{s}=\dfrac{hc}{\lambda} gives VsV_{s} linear in 1λ\dfrac{1}{\lambda}.
  • • Consistency: two values are consistent when their intervals overlap. A gap is expressed as a NUMBER OF UNCERTAINTIES, never as “it is close”.

Part A: the basics (/50)

Exercise 1: Reading a vernier and a goniometer, then writing the result

A VERNIER divides the smallest graduation of the main scale into equal parts: you read the vernier line that best lines up with a line of the main scale. A vernier caliper graduated to fiftieths gives 150\dfrac{1}{50} of a millimetre, that is 0.020.02 mm.

A spectrometer GONIOMETER has a circle graduated in half-degrees and a vernier with thirty divisions, so it reads to the arcminute. The diagram below shows the graduated circle and its vernier.

40°42°44°46°48°50°52°54°56°0′10′20′30′circle graduated in half-degreesvernier: 30 divisions on 29 half-degrees
  • a) What is the reading uncertainty of a vernier caliper graduated to fiftieths, in mm?
  • b) The goniometer vernier has thirty divisions spanning twenty-nine half-degrees. What is the smallest readable division, in arcminutes?
  • c) Convert 40∘54′40^{\circ}54' to decimal degrees, and 2′2' to degrees and then to radians.
  • d) A calculation gives λ=545.6173\lambda=545.6173 nm with an uncertainty of 1.27581.2758 nm. Write the result correctly.
  • e) Why build a vernier instead of engraving graduations fifty times finer?

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  • a) 0.020.02 mm
  • b) 1′1', that is one arcminute
  • c) 40.90∘40.90^{\circ}; 2′=0.0333∘=5.82×10−42'=0.0333^{\circ}=5.82\times 10^{-4} rad
  • d) λ=(545.6±1.3)\lambda=(545.6\pm 1.3) nm
  • e) Lines fifty times closer together would be unreadable to the eye and would blur into one another
a)

A vernier caliper graduated to fiftieths has fifty vernier divisions spanning forty-nine millimetres of the main scale. Each vernier division is therefore worth 4950=0.98\dfrac{49}{50}=0.98 mm, which is 0.020.02 mm less than a millimetre: the offset builds up from one division to the next, and the line that lines up tells you the number of hundredths. The reading uncertainty is the smallest readable division, 0.020.02 mm. Unlike a graduated ruler, you do NOT take half: a vernier gives a clean reading, not an interpolation by eye.

b)

Thirty divisions span twenty-nine half-degrees, that is 29×30′=870′29\times 30'=870'. Each vernier division is worth 87030=29′\dfrac{870}{30}=29', against 30′30' for a division of the circle: the difference is 1′1' per division. The smallest readable division is therefore ONE ARCMINUTE, that is 160\dfrac{1}{60} of a degree. A goniometer in an optics lab thus reads thirty times more finely than its circle is engraved.

c)

54′=5460=0.90∘54'=\dfrac{54}{60}=0.90^{\circ}, so 40∘54′=40.90∘40^{\circ}54'=40.90^{\circ}. For the uncertainty: 2′=260=0.03333∘2'=\dfrac{2}{60}=0.03333^{\circ}, and in radians 0.03333×π180=5.82×10−40.03333\times\dfrac{\pi}{180}=5.82\times 10^{-4} rad. The conversion to radians is not cosmetic: any propagation through the derivative of a sine or a cosine requires it, and forgetting it multiplies the result by fifty-seven.

d)

The uncertainty is rounded to TWO significant figures when it starts with a 11, so Δλ=1.3\Delta\lambda=1.3 nm. The value is aligned on the same decimal place, the tenth of a nanometre: λ=(545.6±1.3)\lambda=(545.6\pm 1.3) nm. The four decimals from the calculator are calculation noise; writing them would suggest a measurement ten thousand times better than it is.

e)

Because the eye cannot separate two lines closer than about a tenth of a millimetre, and because an engraving fifty times finer would be both impossible to make cleanly and unreadable without a microscope. The vernier gets around the problem: it engraves nothing finer, it converts a small DISTANCE into a COINCIDENCE, and the eye is excellent at judging whether two lines are aligned. It is the same principle as the Wheatstone bridge in electricity or the zero of a beam balance: a difficult absolute reading is replaced by an easy comparison.

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Exercise 2: Measuring an angle on both sides: the difference that cancels the zero

On a grating spectrometer, a line appears on both sides of the direct beam. Its position on the graduated circle is read on the LEFT and then on the RIGHT, and the deflection angle is HALF THE DIFFERENCE of the two readings.

Readings: θL=(139∘12′±2′)\theta_{L}=(139^{\circ}12'\pm 2') and θR=(221∘00′±2′)\theta_{R}=(221^{\circ}00'\pm 2'). The diagram below shows the spectrometer seen from above.

collimatorgratingdirect beamθR = (221°00′ ± 2′)θL = (139°12′ ± 2′)θθ
  • a) Calculate the difference of the two readings, in degrees and arcminutes.
  • b) Deduce the deflection angle θ\theta, in decimal degrees.
  • c) Calculate the uncertainty on θ\theta, in arcminutes and then in degrees.
  • d) The graduated circle is badly set: its zero is offset by +15′+15'. Show that this method still gives the correct angle.
  • e) Why do we divide a difference by two, when a difference normally adds the uncertainties?

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  • a) 81∘48′81^{\circ}48'
  • b) θ=40.90∘\theta=40.90^{\circ}
  • c) Δθ=2′=0.0333∘\Delta\theta=2'=0.0333^{\circ}
  • d) The offset is added to BOTH readings and disappears in the difference
  • e) The sum 2′+2′=4′2'+2'=4' is then divided by two, like the quantity itself
a)

221∘00′−139∘12′221^{\circ}00'-139^{\circ}12'. The arcminutes cannot be subtracted directly, since 00′−12′00'-12' is negative: you BORROW 60′60' from the degrees, exactly as you borrow 6060 seconds from a minute. So you calculate 220∘60′−139∘12′220^{\circ}60'-139^{\circ}12', which gives 48′48' and 220−139=81220-139=81 degrees: the difference is 81∘48′81^{\circ}48'.

b)

The difference of the two readings is 2θ2\theta, since the line is deflected by θ\theta on one side and by θ\theta on the other. So θ=81∘48′2=40∘54′=40.90∘\theta=\dfrac{81^{\circ}48'}{2}=40^{\circ}54'=40.90^{\circ}.

c)

The two readings are independent and each carries 2′2': a difference adds the absolute uncertainties, Δ(2θ)=2′+2′=4′\Delta(2\theta)=2'+2'=4'. Dividing by two, Δθ=4′2=2′\Delta\theta=\dfrac{4'}{2}=2', that is 0.0333∘0.0333^{\circ}, or 5.82×10−45.82\times 10^{-4} rad. Result: θ=(40.900±0.033)∘\theta=(40.900\pm 0.033)^{\circ}, a relative uncertainty of only 0.08 %0.08\,\%.

d)

With the zero offset by +15′+15', the two readings become 139∘27′139^{\circ}27' and 221∘15′221^{\circ}15'. Their difference: 221∘15′−139∘27′=81∘48′221^{\circ}15'-139^{\circ}27'=81^{\circ}48', unchanged, so θ=40.90∘\theta=40.90^{\circ} again. The offset is added to BOTH readings and disappears in the subtraction. That is the whole point of the method: a SYSTEMATIC setting error, which no amount of repetition would have corrected, is eliminated by the geometry of the measurement itself. Measuring on one side only, assuming the zero is right, would have given 41∘15′41^{\circ}15', that is 0.35∘0.35^{\circ} too much, ten times the stated uncertainty.

e)

Because the division by two applies to EVERYTHING, to the quantity as well as to its uncertainty. The difference did add the uncertainties, 4′4' instead of 2′2', but it also DOUBLED the measured quantity, which is 2θ2\theta and not θ\theta: the relative uncertainty has not moved. The classic trap of the chapter, a difference of two nearby quantities, does not apply here: the two readings are very FAR apart, 8282 degrees, so the subtraction destroys nothing. Remember the exact wording: a difference is dangerous when its result is SMALL compared with the terms, not simply because it is a difference.

Exercise 3: The square root halves the uncertainty: wave speed on a string

The speed of a transverse wave on a stretched string is v=Tμv=\sqrt{\dfrac{T}{\mu}}, where μ=mL\mu=\dfrac{m}{L} is the linear mass density.

Measurements: tension T=(12.00±0.05)T=(12.00\pm 0.05) N, mass of the string m=(2.50±0.01)m=(2.50\pm 0.01) g, length L=(1.200±0.002)L=(1.200\pm 0.002) m.

Reminder: in z=kxaybz=kx^{a}y^{b}, each exponent MULTIPLIES the corresponding relative uncertainty. A square doubles it; a square root, which is the exponent 12\dfrac{1}{2}, halves it. The diagram below shows the stretched string.

vibratorT = (12.00 ± 0.05) Nstring tensionL = (1.200 ± 0.002) mstring: m = (2.50 ± 0.01) g
  • a) Calculate the linear mass density and its relative uncertainty, in %.
  • b) Calculate the wave speed, in m/s.
  • c) Calculate the relative uncertainty on the wave speed, in %, detailing the three contributions.
  • d) Write the result with its uncertainty, in m/s.
  • e) What would the relative uncertainty be if the law were v=Tμv=\dfrac{T}{\mu} instead of v=Tμv=\sqrt{\dfrac{T}{\mu}}? What should you take from this?

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  • a) μ=2.083×10−3\mu=2.083\times 10^{-3} kg/m, with 0.57 %0.57\,\%
  • b) v≈75.9v\approx 75.9 m/s
  • c) 0.49 %0.49\,\%: 0.21+0.20+0.080.21+0.20+0.08
  • d) v=(75.9±0.4)v=(75.9\pm 0.4) m/s
  • e) 0.98 %0.98\,\%, which is double: the square root halves the uncertainty
a)

μ=mL=2.50×10−31.200=2.083×10−3\mu=\dfrac{m}{L}=\dfrac{2.50\times 10^{-3}}{1.200}=2.083\times 10^{-3} kg/m. This is a quotient, so the relative uncertainties add: 0.012.50=0.40 %\dfrac{0.01}{2.50}=0.40\,\% for the mass and 0.0021.200=0.17 %\dfrac{0.002}{1.200}=0.17\,\% for the length, that is 0.57 %0.57\,\% in all.

b)

v=12.002.083×10−3=5760=75.89v=\sqrt{\dfrac{12.00}{2.083\times 10^{-3}}}=\sqrt{5760}=75.89 m/s. Order-of-magnitude check: a sonometer string stretched by about ten newtons carries waves at a few tens of metres per second, more slowly than sound in air, 343343 m/s; the two speeds are unrelated anyway, since the speed on the string depends only on its tension and its linear mass density. The figure is plausible.

c)

The exponent of TT is +12+\dfrac{1}{2} and that of μ\mu is −12-\dfrac{1}{2}, so each relative uncertainty is HALVED: Δvv=12ΔTT+12Δμμ\dfrac{\Delta v}{v}=\dfrac{1}{2}\dfrac{\Delta T}{T}+\dfrac{1}{2}\dfrac{\Delta\mu}{\mu}. In detail: the tension contributes 12×0.0512.00=0.21 %\dfrac{1}{2}\times\dfrac{0.05}{12.00}=0.21\,\%, the mass 12×0.40=0.20 %\dfrac{1}{2}\times 0.40=0.20\,\% and the length 12×0.17=0.08 %\dfrac{1}{2}\times 0.17=0.08\,\%. Total: 0.49 %0.49\,\%. None of the three dominates, and that is precisely the effect of the root: it has flattened the differences between the contributions.

d)

Δv=75.89×0.0049=0.37\Delta v=75.89\times 0.0049=0.37 m/s, rounded to 0.40.4 m/s. Result: v=(75.9±0.4)v=(75.9\pm 0.4) m/s.

e)

Without the root, the three relative uncertainties would enter in full: 0.42+0.40+0.17=0.98 %0.42+0.40+0.17=0.98\,\%, exactly DOUBLE. What to take from this fits in one sentence: an exponent is an amplifier of uncertainty, in both directions. A square doubles, a cube triples, a square root halves, a cube root divides by three. That is why a quantity obtained through a root is, for equal measurements, more reliable than one obtained through a product; and it is why a squared diameter, in a wire cross-section or a beam area, is almost always the dominant term in an uncertainty budget.

Exercise 4: The extreme-values method on a refractive index

A goniometer is used to measure the angle of incidence and the angle of refraction of a ray entering a glass block, then Snell's law is applied, n=sin⁡isin⁡rn=\dfrac{\sin i}{\sin r}, with air taken as n=1n=1.

Measurements: i=(60.0±0.5)∘i=(60.0\pm 0.5)^{\circ} and r=(35.0±0.5)∘r=(35.0\pm 0.5)^{\circ}. The diagram below shows the ray.

iri = (60.0 ± 0.5)°r = (35.0 ± 0.5)°airglass
  • a) Calculate the refractive index.
  • b) To obtain nmaxn_{max}, should you take rr at its maximum or at its minimum? Justify without calculating.
  • c) Calculate nmaxn_{max} and nminn_{min}.
  • d) Calculate Δn\Delta n and write the result.
  • e) Crown glass is tabulated at n=1.52n=1.52 and acrylic at n=1.49n=1.49. Does this measurement allow you to tell them apart?

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  • a) n≈1.510n\approx 1.510
  • b) rr at its MINIMUM, because sin⁡r\sin r is in the denominator and the sine increases on [0,90∘][0, 90^{\circ}]
  • c) nmax≈1.537n_{max}\approx 1.537 and nmin≈1.484n_{min}\approx 1.484
  • d) Δn≈0.03\Delta n\approx 0.03, so n=(1.51±0.03)n=(1.51\pm 0.03)
  • e) No: both tabulated values lie inside the interval
a)

n=sin⁡60.0∘sin⁡35.0∘=0.86600.5736=1.510n=\dfrac{\sin 60.0^{\circ}}{\sin 35.0^{\circ}}=\dfrac{0.8660}{0.5736}=1.510. Check: the ray bends toward the normal on entering, so the second medium is the more refractive one and n>1n>1. If the calculation had given 0.660.66, the quotient would have been inverted.

b)

The sine is INCREASING on [0,90∘][0, 90^{\circ}], so sin⁡r\sin r grows with rr. Since sin⁡r\sin r is in the DENOMINATOR, the index is largest when sin⁡r\sin r is smallest, that is for rr at its MINIMUM, 34.5∘34.5^{\circ}, and simultaneously for ii at its maximum, 60.5∘60.5^{\circ}. The argument rests on the monotonicity of the sine: over a range containing 90∘90^{\circ} it would no longer hold.

c)

nmax=sin⁡60.5∘sin⁡34.5∘=0.87040.5664=1.537n_{max}=\dfrac{\sin 60.5^{\circ}}{\sin 34.5^{\circ}}=\dfrac{0.8704}{0.5664}=1.537 and nmin=sin⁡59.5∘sin⁡35.5∘=0.86160.5807=1.484n_{min}=\dfrac{\sin 59.5^{\circ}}{\sin 35.5^{\circ}}=\dfrac{0.8616}{0.5807}=1.484. The central value 1.5101.510 does lie between the two.

d)

Δn=1.537−1.4842=0.0532=0.026\Delta n=\dfrac{1.537-1.484}{2}=\dfrac{0.053}{2}=0.026, rounded to 0.030.03. Result: n=(1.51±0.03)n=(1.51\pm 0.03), a relative uncertainty of 1.8 %1.8\,\%. The refractive index is a number with NO UNIT: write nothing after it, neither a degree sign nor an invented unit.

e)

No. The interval [1.48,1.54][1.48, 1.54] contains both 1.521.52 and 1.491.49: both materials are CONSISTENT with the measurement, so the experiment does not decide. That is the right conclusion to write, and not “it is crown glass since 1.511.51 is closer to 1.521.52”: comparing central values when the intervals overlap has no value as proof. To tell them apart you would have to bring the uncertainty below 0.0150.015, therefore divide Δi\Delta i and Δr\Delta r by two at least, that is read the angles to a quarter of a degree or better, which is precisely what a vernier goniometer does.

Exercise 5: The differential method on a diffraction grating

A grating has 600600 lines per millimetre, with an uncertainty of one line per millimetre on this ruling. The grating spacing is d=1600d=\dfrac{1}{600} mm.

Order 22 of a green line is observed at θ=(40.90±0.03)∘\theta=(40.90\pm 0.03)^{\circ}, the angle coming from the two-sided measurement of exercise 2.

The grating formula is dsin⁡θ=mλd\sin\theta=m\lambda, so λ=dsin⁡θm\lambda=\dfrac{d\sin\theta}{m}, with m=2m=2 exact. The diagram below shows the grating and the observed line.

θorder 2order 0θ = (40.90 ± 0.03)°green linegrating: 600 lines per mm,to within one line
  • a) Calculate the grating spacing, in µm, then the wavelength, in nm.
  • b) Calculate the contribution of the angle, ∣∂λ∂θ∣Δθ\left|\dfrac{\partial\lambda}{\partial\theta}\right|\Delta\theta, in nm.
  • c) Calculate the contribution of the grating spacing, in nm.
  • d) Write the result. The green mercury line is at 546.1546.1 nm: is it consistent?
  • e) Which quantity now limits the measurement? And why is order 22 observed rather than order 11?

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  • a) d=1.667d=1.667 µm and λ≈545.6\lambda\approx 545.6 nm
  • b) 0.370.37 nm
  • c) 0.910.91 nm
  • d) λ=(545.6±1.3)\lambda=(545.6\pm 1.3) nm, consistent with 546.1546.1 nm
  • e) The NUMBER OF LINES of the grating; order 2 doubles the angle and improves the measurement
a)

d=1600d=\dfrac{1}{600} mm =1.667×10−3=1.667\times 10^{-3} mm =1.667=1.667 µm =1.6667×10−6=1.6667\times 10^{-6} m. Then λ=1.6667×10−6×sin⁡40.90∘2=1.6667×10−6×0.65472=5.456×10−7\lambda=\dfrac{1.6667\times 10^{-6}\times\sin 40.90^{\circ}}{2}=\dfrac{1.6667\times 10^{-6}\times 0.6547}{2}=5.456\times 10^{-7} m, that is 545.6545.6 nm. The order-of-magnitude check is immediate: a visible wavelength lies between 400400 and 700700 nm, and 545545 nm is indeed in the green.

b)

∂λ∂θ=dcos⁡θm=1.6667×10−6×0.75592=6.299×10−7\dfrac{\partial\lambda}{\partial\theta}=\dfrac{d\cos\theta}{m}=\dfrac{1.6667\times 10^{-6}\times 0.7559}{2}=6.299\times 10^{-7} m/rad. The uncertainty MUST be in radians: Δθ=0.03333∘=5.818×10−4\Delta\theta=0.03333^{\circ}=5.818\times 10^{-4} rad. Contribution: 6.299×10−7×5.818×10−4=3.66×10−106.299\times 10^{-7}\times 5.818\times 10^{-4}=3.66\times 10^{-10} m, that is 0.370.37 nm. Keeping degrees would have given 2121 nm, fifty-seven times too much: this is the costliest error of the whole chapter, because the result stays plausible.

c)

The spacing dd enters to the power 11, so its relative contribution passes through unchanged: Δdd=1600=0.167 %\dfrac{\Delta d}{d}=\dfrac{1}{600}=0.167\,\%, since an uncertainty of one line out of six hundred carries over identically to their spacing. Contribution: 545.6×0.00167=0.91545.6\times 0.00167=0.91 nm.

d)

Δλ=0.37+0.91=1.28\Delta\lambda=0.37+0.91=1.28 nm, rounded to 1.31.3 nm. Result: λ=(545.6±1.3)\lambda=(545.6\pm 1.3) nm, interval [544.3,546.9][544.3, 546.9] nm. The green mercury line, 546.1546.1 nm, lies inside it: the measurement is CONSISTENT, and the experiment identifies the line correctly.

e)

It is now the GRATING that limits: its contribution, 0.910.91 nm, is two and a half times that of the angle. Reading the angles even more finely would hardly help; you would need a grating whose spacing is better known, or to calibrate it on a line of known wavelength, which is standard practice. As for the order: going from m=1m=1 to m=2m=2 doubles sin⁡θ\sin\theta, so it takes the angle from 19∘19^{\circ} to 41∘41^{\circ}, where the cosine is smaller. Now ∂λ∂θ\dfrac{\partial\lambda}{\partial\theta} is proportional to cos⁡θm\dfrac{\cos\theta}{m}: the two effects work in the same direction and divide the contribution of the angle by about 2.52.5. Higher orders are therefore more precise, until sin⁡θ\sin\theta exceeds 11 and the line disappears.

Part B: problems and reasoning (/50)

Exercise 6: Radioactive counting: the uncertainty you predict before measuring

A decay is a RANDOM phenomenon: two counts of the same duration on the same source do not give the same number. Statistics says that the scatter of a count of NN events is N\sqrt{N}, without any need to repeat anything.

Eight successive ten-second counts on a teaching-lab source give, in counts: 4747; 5252; 3939; 4545; 5858; 4343; 5050; 4242. The graph below plots the eight counts.

1234567893035404550556065count numbercounts in 10 s
  • a) Calculate the mean number of counts per ten seconds.
  • b) Calculate the sample standard deviation of these eight counts.
  • c) Calculate Nˉ\sqrt{\bar N} and compare it with b). What do you conclude?
  • d) Calculate the uncertainty on the mean, then the corresponding relative uncertainty, in %.
  • e) A single 8080 s count would give about 376376 counts. What would its relative uncertainty be? Compare with the eight ten-second counts.

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  • a) Nˉ=47.0\bar N=47.0 counts
  • b) s≈6.14s\approx 6.14 counts
  • c) 47≈6.86\sqrt{47}\approx 6.86: very close, the square-root law is confirmed
  • d) s8≈2.17\dfrac{s}{\sqrt{8}}\approx 2.17 counts, that is 4.6 %4.6\,\%
  • e) 376≈19.4\sqrt{376}\approx 19.4 counts out of 376376, that is 5.2 %5.2\,\%: practically the same
a)

The sum is 376376 counts, so Nˉ=3768=47.0\bar N=\dfrac{376}{8}=47.0 counts per ten seconds.

b)

The deviations from the mean are 00; +5+5; −8-8; −2-2; +11+11; −4-4; +3+3; −5-5, which sum to zero. The sum of squares is 0+25+64+4+121+16+9+25=2640+25+64+4+121+16+9+25=264, so s=2647=37.71=6.14s=\sqrt{\dfrac{264}{7}}=\sqrt{37.71}=6.14 counts.

c)

Nˉ=47.0=6.86\sqrt{\bar N}=\sqrt{47.0}=6.86 counts. The measured standard deviation, 6.146.14, is within 10 %10\,\% of it, which is all you can hope for with only eight values: the uncertainty on a standard deviation estimated from NN values is of the order of 12(N−1)\dfrac{1}{\sqrt{2(N-1)}}, that is 27 %27\,\% here. The conclusion is a strong one: the observed scatter is the one predicted by the root-NN law, SO YOU DO NOT NEED TO REPEAT to know the uncertainty of a count. This is a unique situation in the whole chapter: elsewhere, only repetition reveals the scatter.

d)

s8=6.142.828=2.17\dfrac{s}{\sqrt{8}}=\dfrac{6.14}{2.828}=2.17 counts, that is 2.1747.0=4.6 %\dfrac{2.17}{47.0}=4.6\,\%. You would write Nˉ=(47.0±2.2)\bar N=(47.0\pm 2.2) counts per ten seconds.

e)

A single 8080 s count accumulates the same decays: about 376376 counts, whose uncertainty is 376=19.4\sqrt{376}=19.4 counts, that is 19.4376=5.2 %\dfrac{19.4}{376}=5.2\,\%. This is PRACTICALLY THE SAME result as the eight separate counts, and it is no accident: what fixes the precision of a count is the TOTAL NUMBER OF COUNTS ACCUMULATED, not the way they are split into sessions. The only thing the eight counts bring in addition is the check in c), that is, the proof that the source is stable and the counter does not drift. Practical rule: to halve the relative uncertainty, you need FOUR times as many counts, hence four times as much time.

1234567891011123035404550556065mean 47+ √N− √Ncount number

Exercise 7: Linearizing the resonance of a tube: the end correction is in the intercept

A tube closed at one end resonates when its length equals an ODD number of quarter-wavelengths. In reality, the displacement antinode forms slightly outside the tube, which adds an END CORRECTION ee: Ln=(2n−1)λ4−eL_{n}=(2n-1)\dfrac{\lambda}{4}-e.

A 512512 Hz tuning fork excites a tube 2.02.0 cm in diameter whose air column is lengthened. The first four resonances are observed at L=0.155L=0.155; 0.4900.490; 0.8250.825; 1.1601.160 m. The diagram below shows the tube and the tuning fork.

tuning fork, 512 HzLair columnlengthenedwatertube diameter: 2.0 cm
  • a) What should be plotted on the horizontal axis to obtain a straight line? What are then the slope and the intercept?
  • b) Calculate the slope of the regression, in m, then the wavelength, in m.
  • c) Calculate the speed of sound, in m/s.
  • d) Calculate the intercept, then the end correction, in cm. Compare with the theoretical value e≈0.6 de\approx 0.6\,d.
  • e) The speed of sound in air is v≈331+0.6 θv\approx 331+0.6\,\theta with θ\theta in degrees Celsius. What temperature does the measurement indicate? What does this check validate?

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  • a) (2n−1)(2n-1) on the horizontal axis; slope λ4\dfrac{\lambda}{4}, intercept −e-e
  • b) Slope 0.16750.1675 m, so λ=0.670\lambda=0.670 m
  • c) v≈343.0v\approx 343.0 m/s
  • d) Intercept −0.0125-0.0125 m, so e=1.25e=1.25 cm, against 1.21.2 cm expected
  • e) θ≈20\theta\approx 20 °C: the value is that of the room, the setup is consistent
a)

You plot (2n−1)(2n-1) on the horizontal axis, that is 11, 33, 55, 77, and the length LL on the vertical axis. The relation L=(2n−1)λ4−eL=(2n-1)\dfrac{\lambda}{4}-e is then of the form Y=aX+bY=aX+b with a=λ4a=\dfrac{\lambda}{4} and b=−eb=-e. Plotting simply nn would also work, but the slope would be λ2\dfrac{\lambda}{2} and the intercept −e−λ4-e-\dfrac{\lambda}{4}: the two unknowns would be mixed, whereas the choice of (2n−1)(2n-1) separates them cleanly.

b)

With Xˉ=4\bar X=4 and Lˉ=0.6575\bar L=0.6575 m, we form ∑(Xi−Xˉ)(Li−Lˉ)=3.35\sum(X_{i}-\bar X)(L_{i}-\bar L)=3.35 and ∑(Xi−Xˉ)2=20\sum(X_{i}-\bar X)^{2}=20, so a=3.3520=0.1675a=\dfrac{3.35}{20}=0.1675 m. Hence λ=4a=0.670\lambda=4a=0.670 m. Immediate check: the gaps between successive resonances are all 0.3350.335 m, that is HALF a wavelength, which gives λ=0.670\lambda=0.670 m again.

c)

v=λf=0.670×512=343.0v=\lambda f=0.670\times 512=343.0 m/s. This is exactly the value expected in a room at ambient temperature.

d)

b=Lˉ−aXˉ=0.6575−0.1675×4=0.6575−0.6700=−0.0125b=\bar L-a\bar X=0.6575-0.1675\times 4=0.6575-0.6700=-0.0125 m. Since b=−eb=-e, the end correction is e=0.0125e=0.0125 m =1.25=1.25 cm. Theory gives e≈0.6 d=0.6×2.0=1.2e\approx 0.6\,d=0.6\times 2.0=1.2 cm: the agreement is excellent. The intercept is therefore NOT here a mere check that you hope will be zero, it is a PHYSICAL RESULT, and this is the only way to obtain it. A student who had forced the line through the origin would have distorted the slope, hence the speed of sound, while thinking they were doing the right thing.

e)

θ=343.0−3310.6=20.0\theta=\dfrac{343.0-331}{0.6}=20.0 °C, the temperature of a lab room. This check does not measure the temperature, it VALIDATES the measurement chain: it verifies that the frequency of the tuning fork, the reading of the lengths and the graphical processing are consistent with one another. Had it given −40-40 °C or 9595 °C, you would have had to look for the error, for example a misidentified tuning fork or a skipped resonance. A good lab report always ends with a check of this kind, which confronts the result with something known independently.

123456780.20.40.60.811.21.42n − 1L (m)intercept = −e

Exercise 8: Five statements to correct

Each of the following five sentences was overheard in a waves and modern physics lab. Say what is wrong with it, then write the correct version. Naming the rule that is broken earns half the marks.

  • a) “The counter shows 4747 counts, a whole number, so this measurement is exact.”
  • b) “The angle is known to 0.030.03 degree, so we write Δθ=0.03\Delta\theta=0.03 in the propagation formula.”
  • c) “If we repeat the background count often enough, we end up eliminating it.”
  • d) “The measured wavelength is 545.6545.6 nm and the mercury line is 546.1546.1 nm: the experiment failed.”
  • e) “To improve the measurement of the wave speed v=T/μv=\sqrt{T/\mu}, you must first measure the tension better, since it is in the numerator.”

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  • a) False: the number is a whole number but the phenomenon is random, ΔN=N\Delta N=\sqrt{N}
  • b) False: the derivative of a sine requires RADIANS
  • c) False: the background is SUBTRACTED, it does not average to zero
  • d) False: 546.1546.1 lies in [544.3,546.9][544.3, 546.9], so it is consistent
  • e) False: the three contributions are comparable, none dominates
a)

FALSE. The counter counts exactly, but what it counts FLUCTUATES: decay is random, and a second count of the same duration will give a different integer. The uncertainty is N=47=6.9\sqrt{N}=\sqrt{47}=6.9 counts, that is 15 %15\,\%. Correct version: “the count is exact, the quantity is not; the uncertainty of a count is the square root of the number of counts, and it is predicted without repeating”.

b)

FALSE, and this is the costliest error of the chapter because the result stays plausible. A derivative such as ∂λ∂θ=dcos⁡θm\dfrac{\partial\lambda}{\partial\theta}=\dfrac{d\cos\theta}{m} is valid only in RADIANS, since the derivative of the sine equals the cosine only in that unit. You must therefore convert: 0.03333∘=5.818×10−40.03333^{\circ}=5.818\times 10^{-4} rad. Keeping degrees multiplies the contribution by 180π=57.3\dfrac{180}{\pi}=57.3. Correct version: “any angular uncertainty entering a propagation through a derivative is first converted to radians”.

c)

FALSE. The background, cosmic rays and ambient radioactivity, is present all the time and ALWAYS in the same direction: it is a systematic error by excess. Averaging it only measures it more precisely, it does not remove it. It is SUBTRACTED, and that subtraction has a cost, since it adds the uncertainties of the two counts. Correct version: “the background is measured with the source removed, then subtracted from the total count; repeating only improves the knowledge of the background, never its absence”.

d)

FALSE. The gap, 0.50.5 nm, is SMALLER than the uncertainty, 1.31.3 nm: the tabulated value lies inside the interval [544.3,546.9][544.3, 546.9] nm, so the measurement is CONSISTENT and the experiment succeeded. Declaring a failure because two numbers differ is ignoring what an uncertainty means. Correct version: “two values are consistent when their intervals overlap; the 0.50.5 nm gap is 0.40.4 times the uncertainty, an excellent agreement”.

e)

FALSE. The square root halves each relative contribution, which flattens the differences: the tension contributes 0.21 %0.21\,\%, the mass 0.20 %0.20\,\% and the length 0.08 %0.08\,\%. None dominates, and improving the tension alone would gain at best a fifth of the budget. Correct version: “you find the dominant contribution by calculation, not by the place of the quantity in the formula; and when none dominates, you must improve several measurements at once or change method”.

Exercise 9: Problem: Planck's constant measured with five light-emitting diodes

A light-emitting diode only lights above a threshold voltage VsV_{s}: electrons must receive enough energy to emit a photon, so eVs=hcλeV_{s}=\dfrac{hc}{\lambda}.

The threshold voltage of five diodes of different colours is read with a voltmeter:

λ\lambda (nm): 635635; 585585; 525525; 470470; 405405. VsV_{s} (V): 1.851.85; 2.042.04; 2.272.27; 2.562.56; 3.003.00. The diagram below shows the setup.

threshold voltage VsrheostatLEDfive LEDs: 635, 585, 525, 470 and 405 nmGV
  • a) What should be plotted on the horizontal axis to obtain a straight line, and what is then the slope?
  • b) Calculate the slope of the regression, in V·µm.
  • c) Deduce Planck's constant, in J·s. Take e=1.602×10−19e=1.602\times 10^{-19} C and c=3.00×108c=3.00\times 10^{8} m/s.
  • d) The accepted value is 6.626×10−346.626\times 10^{-34} J·s. Calculate the relative deviation, in %.
  • e) The extreme lines have slopes of 1.241.24 and 1.321.32 V·µm. Give hh with its uncertainty, then conclude about the method.

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  • a) 1λ\dfrac{1}{\lambda} on the horizontal axis; the slope is hce\dfrac{hc}{e}
  • b) Slope ≈1.278\approx 1.278 V·µm
  • c) h≈6.83×10−34h\approx 6.83\times 10^{-34} J·s
  • d) +3.1 %+3.1\,\%
  • e) h=(6.83±0.21)×10−34h=(6.83\pm 0.21)\times 10^{-34} J·s: consistent, despite a known upward bias
a)

Isolating the voltage: Vs=hce⋅1λV_{s}=\dfrac{hc}{e}\cdot\dfrac{1}{\lambda}. This is of the form Y=aXY=aX with X=1λX=\dfrac{1}{\lambda} and Y=VsY=V_{s}, so you plot the INVERSE OF THE WAVELENGTH on the horizontal axis and the SLOPE IS hce\dfrac{hc}{e}. Plotting λ\lambda directly would give a hyperbola, from which no tangent can be read with a ruler.

b)

Expressing 1λ\dfrac{1}{\lambda} in µm−1^{-1}: 1.57481.5748; 1.70941.7094; 1.90481.9048; 2.12772.1277; 2.46912.4691. The regression gives Xˉ=1.9572\bar X=1.9572 µm−1^{-1}, Vˉ=2.344\bar V=2.344 V, and a=1.278a=1.278 V·µm. Rough check with the two extreme points: 3.00−1.852.4691−1.5748=1.150.8943=1.286\dfrac{3.00-1.85}{2.4691-1.5748}=\dfrac{1.15}{0.8943}=1.286, the right order.

c)

a=hcea=\dfrac{hc}{e}, so h=aech=\dfrac{ae}{c}. Converting the slope to volt-metres, a=1.278×10−6a=1.278\times 10^{-6} V·m: h=1.278×10−6×1.602×10−193.00×108=6.83×10−34h=\dfrac{1.278\times 10^{-6}\times 1.602\times 10^{-19}}{3.00\times 10^{8}}=6.83\times 10^{-34} J·s. The conversion of micrometres to metres is the only delicate step: forgetting it gives 10−2810^{-28}, a million times too much.

d)

6.83−6.6266.626=0.031\dfrac{6.83-6.626}{6.626}=0.031, that is +3.1 %+3.1\,\%. The deviation is POSITIVE, and it always is with this method.

e)

Δa=1.32−1.242=0.04\Delta a=\dfrac{1.32-1.24}{2}=0.04 V·µm, a relative uncertainty of 0.041.278=3.1 %\dfrac{0.04}{1.278}=3.1\,\% on the slope, hence on hh: Δh=6.83×0.031=0.21\Delta h=6.83\times 0.031=0.21, and h=(6.83±0.21)×10−34h=(6.83\pm 0.21)\times 10^{-34} J·s. The interval [6.62,7.04]×10−34[6.62, 7.04]\times 10^{-34} contains the accepted value, just barely: the measurement is CONSISTENT. What to conclude is more interesting than the verdict. The diode method carries a SYSTEMATIC BIAS upward, because the “threshold” is not a sharp point: the diode already emits a little below it, and the eye or the voltmeter declares it lit a little too late; the ohmic drop in the junction adds to this. The bias here is three percent, and it happens to be of the same order as the uncertainty, which makes it invisible. An honest uncertainty therefore saved the conclusion, but did not prove it: if you really wanted to measure hh, you would need a method without a fuzzy threshold, such as the photoelectric effect with a stopping potential.

0.511.522.530.511.522.533.51/λ (µm⁻¹)Vs (V)slope = hc/e

Exercise 10: Problem: the half-life by semi-logarithmic regression, background included

The activity of a freshly eluted source of metastable barium 137 is followed. The counter totals the counts for thirty seconds, every minute. The background, measured with the source removed, is 2020 counts per thirty seconds.

tt (s): 00; 6060; 120120; 180180; 240240. Total count: 820820; 630630; 484484; 374374; 290290 counts.

The decay follows N=N0e−λtN=N_{0}e^{-\lambda t}, with t1/2=ln⁡2λt_{1/2}=\dfrac{\ln 2}{\lambda}. The graph below shows the total counts.

60120180240300100200300400500600700800900background: 20 countst (s)counts in 30 s
  • a) List the NET counts, and say why the background is subtracted before taking the logarithm and not after.
  • b) Calculate the slope of the regression of ln⁡N\ln N against tt, in s−1^{-1}.
  • c) Deduce the half-life, in seconds and then in minutes. The tabulated value is 2.552.55 min.
  • d) A student forgets the subtraction and regresses on the TOTAL counts. They obtain a slope of −4.334×10−3-4.334\times 10^{-3} s−1^{-1}. What half-life do they find, and by how much are they wrong?
  • e) On the student's semi-logarithmic plot, the sequence of points is slightly CURVED. Explain why, and say what this signal is for.

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  • a) 800800; 610610; 464464; 354354; 270270; the logarithm is not linear, ln⁡(a−b)≠ln⁡a−ln⁡b\ln(a-b)\neq\ln a-\ln b
  • b) Slope ≈−4.528×10−3\approx -4.528\times 10^{-3} s−1^{-1}
  • c) t1/2≈153t_{1/2}\approx 153 s, that is 2.552.55 min: exact agreement
  • d) 160160 s, that is 2.672.67 min: 4.5 %4.5\,\% too much
  • e) A constant background becomes relatively heavier as the source decays: the curve flattens
a)

You subtract 2020 counts from each count: 800800; 610610; 464464; 354354; 270270. The subtraction is done BEFORE the logarithm because the logarithm is not a linear operation: ln⁡(Ntot−Nbg)\ln(N_{tot}-N_{bg}) has nothing to do with ln⁡Ntot−ln⁡Nbg\ln N_{tot}-\ln N_{bg}, which equals ln⁡NtotNbg\ln\dfrac{N_{tot}}{N_{bg}}. More deeply, the exponential law describes the SOURCE alone; the background is a constant additive term laid on top of it, and it has to be removed to recover the quantity the law describes.

b)

The logarithms are 6.68466.6846; 6.41356.4135; 6.13996.1399; 5.86935.8693; 5.59845.5984. Their successive differences, −0.2711-0.2711; −0.2736-0.2736; −0.2706-0.2706; −0.2709-0.2709, are practically constant: the decay is indeed exponential, and this is the check to make before any calculation. The regression gives tˉ=120\bar t=120 s, ln⁡N‾=6.1411\overline{\ln N}=6.1411, ∑(ti−tˉ)(ln⁡Ni−ln⁡N‾)=−163.0\sum(t_{i}-\bar t)(\ln N_{i}-\overline{\ln N})=-163.0 and ∑(ti−tˉ)2=36,000\sum(t_{i}-\bar t)^{2}=36{,}000, so λ=−a=4.528×10−3\lambda=-a=4.528\times 10^{-3} s−1^{-1}.

c)

t1/2=ln⁡2λ=0.69314.528×10−3=153.1t_{1/2}=\dfrac{\ln 2}{\lambda}=\dfrac{0.6931}{4.528\times 10^{-3}}=153.1 s, that is 153.160=2.55\dfrac{153.1}{60}=2.55 min. The agreement with the tabulated value is exact to the hundredth of a minute.

d)

t1/2=0.69314.334×10−3=159.9t_{1/2}=\dfrac{0.6931}{4.334\times 10^{-3}}=159.9 s, that is 2.672.67 min. The relative deviation is 2.67−2.552.55=4.5 %\dfrac{2.67-2.55}{2.55}=4.5\,\%, and it is POSITIVE: forgetting the background always makes the source look slower than it is. This is not a random error that repetition would correct, it is a systematic bias, of the same kind as the offset zero of a goniometer.

e)

A constant background of 2020 counts represents 2.4 %2.4\,\% of the first count but 6.9 %6.9\,\% of the last: its RELATIVE weight grows as the source dies away. The curve of totals therefore falls less and less quickly on a logarithmic scale, it flattens, and would tend to the horizontal once the source was exhausted, since only the background would remain. It is a valuable signal: ON A SEMI-LOGARITHMIC PLOT, AN UPWARD CURVATURE BETRAYS A FORGOTTEN ADDITIVE TERM. The same diagnosis applies elsewhere: a background of stray light in an absorption measurement, a dark current in a photodiode, a leak in parallel on a capacitor. And the opposite curvature, downward, generally betrays the presence of a second isotope with a shorter life.

5010015020025030055.566.57t (s)ln Nsquares: uncorrected totals

Part C: the classics (/50)

Exercise 11: Separating is not measuring: the resolving power of a grating

The RESOLVING POWER of a grating tells you the smallest wavelength difference Δλ\Delta\lambda it can still SEPARATE into two distinct lines: R=λΔλmin=mNR=\dfrac{\lambda}{\Delta\lambda_{min}}=mN, where mm is the order and NN the number of lines ACTUALLY ILLUMINATED by the beam.

Take the grating of exercise 5, 600600 lines per millimetre, observed at order 22 and illuminated by a beam 5.05.0 mm wide, around λ=545.6\lambda=545.6 nm. The diagram below shows the illuminated grating.

beam: 5.0 mm widegrating seen from the front: 600 lines per mm (lines not to scale)
  • a) How many lines does the beam illuminate?
  • b) Calculate the resolving power at order 22.
  • c) Calculate the smallest separable wavelength difference, in nm.
  • d) The sodium yellow doublet is at 589.0589.0 and 589.6589.6 nm. What resolving power is needed to separate it? Does this grating manage it?
  • e) Compare the result of c) with the uncertainty Δλ=1.3\Delta\lambda=1.3 nm of exercise 5. What should you conclude about the meaning of the words “resolution” and “accuracy”?

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  • a) N=3000N=3000 lines
  • b) R=6000R=6000
  • c) Δλmin≈0.091\Delta\lambda_{min}\approx 0.091 nm
  • d) R≈982R\approx 982 is enough: the grating separates the doublet with room to spare
  • e) It SEPARATES fourteen times more finely than it LOCATES: two different qualities
a)

N=600 lines/mm×5.0 mm=3000N=600\ \text{lines/mm}\times 5.0\ \text{mm}=3000 lines. What matters is NOT the total number of lines engraved on the grating, but the number of lines the beam touches: masking the grating with a diaphragm degrades the resolution, even if the plate is huge.

b)

R=mN=2×3000=6000R=mN=2\times 3000=6000. The resolving power is a number with NO UNIT: it is a ratio of two wavelengths.

c)

Δλmin=λR=545.66000=0.0909\Delta\lambda_{min}=\dfrac{\lambda}{R}=\dfrac{545.6}{6000}=0.0909 nm, or about 0.0910.091 nm. The grating therefore distinguishes two lines a tenth of a nanometre apart.

d)

You need R=λΔλ=589.00.6=982R=\dfrac{\lambda}{\Delta\lambda}=\dfrac{589.0}{0.6}=982. The grating offers 60006000, six times more: it separates the sodium doublet without difficulty, and two distinct yellow lines are clearly seen. At order 11 it would still offer 30003000, plenty. With a beam reduced to 11 mm, only R=1200R=1200 would remain at order 22: the two lines would still be separated, but only just.

e)

The two numbers do not measure the same thing, and that is the whole lesson. The RESOLUTION, 0.0910.091 nm, tells you how finely the instrument SEPARATES two neighbouring lines: it is a question of discriminating power. The ACCURACY, 1.31.3 nm, tells you how precisely it LOCATES a line on the wavelength scale: it is a question of calibration. Here the instrument separates fourteen times more finely than it locates, which is the normal case for a spectrometer: it sees perfectly well that two lines are different, but it can only say where they are to within 1.31.3 nm, because of the uncertainty on the grating spacing. Immediate practical consequence: to improve the accuracy you calibrate, with a line of known wavelength; to improve the resolution you widen the beam or go up in order. Confusing the two leads to buying the wrong instrument.

Exercise 12: Identifying a line: which hydrogen transition does the measurement point to?

A hydrogen lamp is observed with the spectrometer of exercise 5, and a blue-green line is measured at λ=(485.5±1.5)\lambda=(485.5\pm 1.5) nm.

The visible lines of hydrogen form the Balmer series, whose wavelengths obey 1λ=RH(122−1n2)\dfrac{1}{\lambda}=R_{H}\left(\dfrac{1}{2^{2}}-\dfrac{1}{n^{2}}\right) with RH=1.0974×107R_{H}=1.0974\times 10^{7} m−1^{-1} and n≥3n\geq 3. The diagram below shows the measured line.

400450500550600650700λ (nm)λ = (485.5 ± 1.5) nmblue-green line of the hydrogen lamp
  • a) Calculate the wavelength predicted for n=4n=4, in nm.
  • b) Calculate the wavelength predicted for n=5n=5, in nm.
  • c) Which of the two is consistent with the measurement? Justify with the intervals.
  • d) Calculate the gap expressed as a number of uncertainties, ∣λ−λth∣Δλ\dfrac{|\lambda-\lambda_{th}|}{\Delta\lambda}. Comment on the quality of the agreement.
  • e) Deuterium emits the same line shifted by 0.130.13 nm toward the blue. Does this experiment allow hydrogen to be distinguished from deuterium?

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  • a) λ4≈486.0\lambda_{4}\approx 486.0 nm
  • b) λ5≈433.9\lambda_{5}\approx 433.9 nm
  • c) n=4n=4: 486.0486.0 lies in [484.0,487.0][484.0, 487.0], 433.9433.9 is far outside it
  • d) 0.330.33 uncertainty: excellent agreement
  • e) No: 0.130.13 nm is eleven times smaller than the uncertainty
a)

1λ=1.0974×107(14−116)=1.0974×107×0.1875=2.0576×106\dfrac{1}{\lambda}=1.0974\times 10^{7}\left(\dfrac{1}{4}-\dfrac{1}{16}\right)=1.0974\times 10^{7}\times 0.1875=2.0576\times 10^{6} m−1^{-1}, so λ=12.0576×106=4.860×10−7\lambda=\dfrac{1}{2.0576\times 10^{6}}=4.860\times 10^{-7} m =486.0=486.0 nm. This is the HβH_{\beta} line. Watch the final inversion: the formula gives the inverse of the wavelength, and forgetting to invert the result produces a number in inverse metres that gets mistaken for nanometres.

b)

1λ=1.0974×107(14−125)=1.0974×107×0.21=2.3045×106\dfrac{1}{\lambda}=1.0974\times 10^{7}\left(\dfrac{1}{4}-\dfrac{1}{25}\right)=1.0974\times 10^{7}\times 0.21=2.3045\times 10^{6} m−1^{-1}, so λ=433.9\lambda=433.9 nm, the HγH_{\gamma} line, violet.

c)

The measurement covers [484.0,487.0][484.0, 487.0] nm. The n=4n=4 line, at 486.0486.0 nm, lies inside it: CONSISTENT. The n=5n=5 line, at 433.9433.9 nm, is more than fifty nanometres away, thirty-five times the uncertainty: ruled out without hesitation. The observed transition is therefore the one from level 44 to level 22.

d)

∣485.5−486.0∣1.5=0.51.5=0.33\dfrac{|485.5-486.0|}{1.5}=\dfrac{0.5}{1.5}=0.33. The gap is a third of an uncertainty, which is an EXCELLENT agreement: statistically, you expect a gap of the order of one uncertainty, and finding three times less is even a little lucky. The sentence to write in a report is “the measurement is consistent with the theoretical value, the gap being 0.330.33 uncertainty”, never “the measurement is right”.

e)

No. The isotopic shift, 0.130.13 nm, is ELEVEN TIMES smaller than the uncertainty of 1.51.5 nm: the two lines would fall in the same place, at the precision of this setup. Be careful not to confuse this with exercise 11: the grating SEPARATES 0.0910.091 nm, so it would indeed show two distinct lines if both isotopes were present together, since the 0.130.13 nm gap exceeds its resolving power. What it cannot do is say which of the two it is looking at when there is only one, because that requires LOCATING the line to better than 0.130.13 nm, eleven times better than the calibration allows. Separating and locating, once again, are not the same thing. To manage it, you would have to calibrate the spectrometer on known lines, which would bring the uncertainty down to the level of the resolution.

430440450460470480490λ (nm)measurement: [484.0, 487.0]n = 4 : 486.0 nmn = 5 : 433.9 nm

Exercise 13: Linearizing Malus's law: what the intercept exposes

Two polarizers face each other, the second rotated by an angle θ\theta relative to the first. Malus's law predicts I=I0cos⁡2θI=I_{0}\cos^{2}\theta.

A photodiode measures the transmitted intensity, in microwatts:

θ\theta: 0∘0^{\circ}; 30∘30^{\circ}; 45∘45^{\circ}; 60∘60^{\circ}; 90∘90^{\circ}. II (µW): 2.462.46; 1.901.90; 1.341.34; 0.780.78; 0.220.22. The diagram below shows the setup.

polarizer 1polarizer 2rotated by θphotodiodeI (µW)lamp
  • a) What should be plotted on the horizontal axis to obtain a straight line? List the abscissas.
  • b) Calculate the slope of the regression, in µW.
  • c) Calculate the intercept, in µW. What should it be if Malus's law alone were at work?
  • d) A student measured only 0∘0^{\circ} and 90∘90^{\circ} and concludes that crossed polarizers let through 9 %9\,\% of the light. What does the complete graph tell them?
  • e) Correct the five measurements, then check that Malus's law is then obeyed exactly.

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  • a) cos⁡2θ\cos^{2}\theta: 11; 0.750.75; 0.500.50; 0.250.25; 00
  • b) Slope I0=2.24I_{0}=2.24 µW
  • c) Intercept 0.220.22 µW; it should be zero
  • d) The 0.220.22 µW is CONSTANT, therefore instrumental, not optical
  • e) 2.242.24; 1.681.68; 1.121.12; 0.560.56; 00, which is exactly I0cos⁡2θI_{0}\cos^{2}\theta
a)

You plot cos⁡2θ\cos^{2}\theta on the horizontal axis: the law becomes I=I0XI=I_{0}X, a line through the origin. The abscissas are cos⁡20∘=1\cos^{2}0^{\circ}=1; cos⁡230∘=(32)2=0.75\cos^{2}30^{\circ}=\left(\dfrac{\sqrt{3}}{2}\right)^{2}=0.75; cos⁡245∘=0.50\cos^{2}45^{\circ}=0.50; cos⁡260∘=0.25\cos^{2}60^{\circ}=0.25; cos⁡290∘=0\cos^{2}90^{\circ}=0. Plotting θ\theta directly would give a bell-shaped curve from which you can get nothing with a ruler; plotting cos⁡θ\cos\theta would give a parabola, hardly better.

b)

With Xˉ=0.50\bar X=0.50 and Iˉ=1.34\bar I=1.34 µW, the regression gives a slope of 2.242.24 µW. Check: the successive differences between the measurements are all 0.560.56 µW for an abscissa step of 0.250.25, a slope of 0.560.25=2.24\dfrac{0.56}{0.25}=2.24 µW. The points are therefore perfectly aligned.

c)

b=Iˉ−aXˉ=1.34−2.24×0.50=1.34−1.12=0.22b=\bar I-a\bar X=1.34-2.24\times 0.50=1.34-1.12=0.22 µW. It SHOULD be zero: at cos⁡2θ=0\cos^{2}\theta=0, that is crossed polarizers, Malus's law predicts total extinction. The 0.220.22 µW measured therefore comes from something else: ambient light entering the detector, the dark current of the photodiode, or stray reflections in the setup.

d)

The complete graph shows that these 0.220.22 µW are present at ALL ANGLES, and not only at 90∘90^{\circ}: it is a CONSTANT ADDITIVE term, not a fraction of the incident light. A student who measures only the two extremes cannot tell the difference between “the polarizers let through 9 %9\,\%” and “the detector sees 0.220.22 µW of stray signal all the time”: both hypotheses give the same two points. You need at least three points to tell them apart, and five to do it comfortably. This is the same argument as in exercises 7 and 10: two points can never contradict a model, because a line always passes through two points.

e)

You subtract 0.220.22 µW from each measurement: 2.242.24; 1.681.68; 1.121.12; 0.560.56; 00 µW. The ratio to the first value gives 11; 0.750.75; 0.500.50; 0.250.25; 00, exactly cos⁡2θ\cos^{2}\theta: Malus's law is verified without the slightest gap, and the extinction at 90∘90^{\circ} is TOTAL. The setup was fine, it was the measurement that carried an offset. That is what a linearization is really for: not to obtain a pretty line, but to SEPARATE what is proportional from what is constant, that is, the physics from the artefact.

0.20.40.60.811.20.511.522.53cos² θI (µW)intercept 0.22: stray light

Exercise 14: The Doppler radar: measuring a difference without ever subtracting

A traffic radar emits a wave at f0=24.125f_{0}=24.125 GHz. The wave returned by an approaching vehicle comes back shifted by Δf=2vf0c\Delta f=\dfrac{2vf_{0}}{c}, the factor 22 coming from the round trip.

Take c=2.998×108c=2.998\times 10^{8} m/s and consider a vehicle at 100100 km/h. The diagram below shows the situation.

radarv = 100 km/hemitted: f₀ = 24.125 GHzreturned: f₀ + Δf
  • a) Calculate the frequency shift, in Hz.
  • b) Calculate the RELATIVE shift Δff0\dfrac{\Delta f}{f_{0}}.
  • c) To know the speed to within 11 km/h, to how many significant figures would each of the two frequencies have to be known, if they were measured separately and subtracted?
  • d) The instrument instead mixes the two signals and counts the BEAT for one second, to within ±1\pm 1 Hz. What uncertainty does that give on the speed, in km/h?
  • e) State the general rule this example illustrates, and name another setup in this course that applies it.

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  • a) Δf≈4.47\Delta f\approx 4.47 kHz
  • b) 1.85×10−71.85\times 10^{-7}
  • c) Ten significant figures on each frequency
  • d) ±0.022\pm 0.022 km/h
  • e) A small difference is MEASURED, never computed; the Wheatstone bridge does the same
a)

v=100v=100 km/h =1003.6=27.78=\dfrac{100}{3.6}=27.78 m/s. Δf=2×27.78×24.125×1092.998×108=4.47×103\Delta f=\dfrac{2\times 27.78\times 24.125\times 10^{9}}{2.998\times 10^{8}}=4.47\times 10^{3} Hz, that is about 4.474.47 kHz: an AUDIBLE frequency, which is no accident, since the first radars let the operator listen to it.

b)

Δff0=4.47×10324.125×109=1.85×10−7\dfrac{\Delta f}{f_{0}}=\dfrac{4.47\times 10^{3}}{24.125\times 10^{9}}=1.85\times 10^{-7}, less than two ten-millionths. The quantity sought is thus buried very deep in the decimals of the two frequencies.

c)

A speed of 11 km/h corresponds to 4470100=44.7\dfrac{4470}{100}=44.7 Hz. For the DIFFERENCE of two frequencies to be known to within 44.744.7 Hz, each must be known to better than 2222 Hz, out of 24.125×10924.125\times 10^{9} Hz: that is a relative uncertainty of 9×10−109\times 10^{-10}, so TEN significant figures on each measurement. No ordinary lab counter gives that many, and the radar oscillator would moreover have to be stable at that level during the measurement. The subtraction method is therefore out of reach, not by a little, but by several orders of magnitude.

d)

The beat is measured to ±1\pm 1 Hz, and 44.744.7 Hz is worth 11 km/h: the uncertainty on the speed is 144.7=0.022\dfrac{1}{44.7}=0.022 km/h. The instrument thus knows the speed to a hundredth of a kilometre per hour, although it would be unable to measure either frequency to better than a few kilohertz. The difference was never calculated: it was PHYSICALLY MANUFACTURED by the mixer, then measured directly.

e)

The rule: A SMALL DIFFERENCE OF TWO LARGE QUANTITIES IS NOT CALCULATED, IT IS MEASURED. Whenever a setup can produce the difference itself, a beat, an imbalance, an interference, prefer it, because the uncertainty then falls on the small quantity and not on the large ones. The Wheatstone bridge of the electricity course is the twin example: it does not measure two voltages to subtract them, it nulls their difference and reads a length. In this course, the Michelson interferometer does the same with two nearly equal optical paths, and exercise 15 shows what it costs when no setup of this kind is available.

Exercise 15: Problem: a weak source, when the difference drowns in the noise

We want to know whether a rock sample is radioactive. With the counter in place and the sample present, 520520 counts are totalled in 300300 s; with the sample removed, the background gives 480480 counts in 300300 s.

Reminder from exercise 6: the uncertainty of a count of NN events is N\sqrt{N}. The diagram below shows the two counts.

520 countsGeiger tubesample presentin 300 s480 countsGeiger tubesample removedin 300 s
  • a) Calculate the net count and its absolute uncertainty.
  • b) Calculate the ratio netΔ\dfrac{\text{net}}{\Delta}, often called the signal-to-noise ratio.
  • c) Can we claim that the sample is radioactive? Write the conclusion.
  • d) The measurement is repeated, counting for 30003000 s: 52005200 counts with the sample, 48004800 without. Redo a) and b).
  • e) How long would you have to count to reach a ratio of 33, starting from the first measurement? State the law that governs this progression.

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  • a) Net =40=40 counts, Δ≈45\Delta\approx 45 counts
  • b) 0.890.89
  • c) No: the gap is smaller than its uncertainty, nothing is demonstrated
  • d) Net =400=400 counts, Δ≈141\Delta\approx 141 counts, ratio 2.832.83
  • e) About 34003400 s, that is 5757 min; the ratio grows as the SQUARE ROOT of the time
a)

Net =520−480=40=520-480=40 counts. The two counts are independent and each carries its own uncertainty: 520=22.8\sqrt{520}=22.8 and 480=21.9\sqrt{480}=21.9 counts. A difference adds the absolute uncertainties, so Δ=22.8+21.9=44.7\Delta=22.8+21.9=44.7, about 4545 counts. Result: net =(40±45)=(40\pm 45) counts.

b)

4044.7=0.89\dfrac{40}{44.7}=0.89. The signal being sought is SMALLER than its uncertainty.

c)

No, nothing can be claimed. The interval of the net, [−5,85][-5, 85] counts, contains ZERO: a perfectly inert sample could very well have given these numbers. The correct conclusion is written: “the net count is (40±45)(40\pm 45) counts; it is consistent with zero, so this measurement shows no radioactivity. Nor does it prove that the sample is inert: it is simply too short to decide.” Writing “the sample is weakly radioactive since we counted 4040 more” is the mistake to avoid, and it is exactly the reasoning that manufactures false discoveries.

d)

Net =5200−4800=400=5200-4800=400 counts. Uncertainties: 5200=72.1\sqrt{5200}=72.1 and 4800=69.3\sqrt{4800}=69.3, so Δ=141.4\Delta=141.4 counts. Net =(400±141)=(400\pm 141) counts, and the ratio is 400141.4=2.83\dfrac{400}{141.4}=2.83. The interval, [259,541][259, 541], no longer contains zero: this time the sample is indeed active. Notice what happened: counting ten times longer multiplied the net by 1010 but its uncertainty only by 10=3.16\sqrt{10}=3.16.

e)

The ratio grows as t\sqrt{t}: going from 0.890.89 to 33 requires multiplying the time by (30.894)2=11.3\left(\dfrac{3}{0.894}\right)^{2}=11.3, that is 300×11.3=3400300\times 11.3=3400 s, about 5757 minutes. THE LAW: the net count grows in proportion to the time, its uncertainty only as the square root of the time, so the signal-to-noise ratio grows as the square root of the time. Two practical consequences. First, in principle there is no such thing as a source that is “too weak”, only measurements that are too short, and this is what makes carbon 1414 dating possible on almost extinct samples. Second, the price is brutal: gaining a factor of ten in sensitivity costs ONE HUNDRED times more time. That is why, when possible, you always prefer to reduce the background, with a lead shield or a buried detector, rather than count longer: when the background dominates the noise, dividing it by four is worth as much as counting four times longer.

−1000100200300400500600net (counts)3,000 s: (400 ± 141) counts300 s: (40 ± 45) countszero net
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