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Chapter 32:
• 8: a) 100 mSv, b) 80 mSv, c) 15-30 mSv, depending on α energy
• 10: 2-4 Gy depending on the RBE of the α used.
• 16: Using RBE=20, we get 7.44 x 108 nuclei
• 48: a) Z=90, N=142, b) product is 90233Th, c) two β decays produce 91233Pa, and 92233U successively, d) the U has N=141, e) half life is 1590 years, plenty long to have a bomb sit around for a while before you use it. NOTE: There may be a typo in the parenthetical statement, which should say, (much as 238 U is bred into 239 Pu)
• 49: Thermal output is 2570 MW, b) 8.04 x 1019 fissions/sec, which is 2.53 x 1027 fissions/year, a total mass of U of 990 kg has fissioned
• 52: 46 grams
• 54: 4.67 x 1012 kWh, b) 4.67 x 1011 dollars

Chapter 31:
• 9: a) 4.6 fm, b) 0.61
• 10: Using E=mc2, 1 u gives 1.4924 x 10-10 J, which is 931.5 MeV
• 18: produces 2040Ca and an anti-neutrino (but I don't care much about neutrinos)
• 20: produces 2552Mn
• 24: 226Ra → 24α + 86222Rn
• 34: a) 82208Pb, b) energy released = 33.05 MeV
• 45: a) 0.50 mCi, b) this is 3 half lives, = 15.81 years
• 56: it decayed to 0.7 of its initial activity, which takes 2.71 years

Chapter 29:
• 21: FM radio 90 MHz, a) 5.96 x 10-26 J, = 3.72 x 10-7 eV, b) at 50 kW of power this is 8.38 x 1029 photons/sec
• 26: IR photon: a) E= 0.0827 eV, b) say 5 eV to break a molecule, this will take about 60 photons, c) γ-ray: 1.24 MeV, d) will break 250,000 molecules
• 35: at 650 kHz a 50kW radio station emits 1.16 x 1032 photons/sec. Spread out over a sphere with one photon per cm2 per second, the sphere will have a radius of 3.04 x 1013 m, which is much less than a light year (which is about 1016 m), and the nearest star is about 4 light years away, and stars that may have alien civilizations are likely much farther away than that.
• 38: a) 1.67 x 10-32 kg m/s
• 39: a) 6.63 x 10-23 kg m/s, b) 0.124 MeV
• 50: not relativity, too slow, so λ = 8.08 x 10-11 m
• 58: a) v = 728 m/s

Chapter 28:
• 1: γ = 1.033 and 1.15
• 3: 5.96 x 10-8 s
• 6: v = 0.90 c
• 8: 0.24 c
• 16: Time as seen by us = 4.302 years. time as seen by astronaut = 0.143 years. The ratio is γ
• 36: 1.35 x 10-21 kg m/s
• 40: 2.0 x 108 m/s
• 44: 1.50 x 10-10 J = 939 MeV
• 46: 1.4 x 1020 stars can be formed if half of the total energy available is converted to mass.
• 47: a) mass lost = 1.11 x 1027 kg, which is, b) 5.56 x 10-5 of the original mass
• 67: for 1000 MW of electric output produced at 35% efficiency, a total power of 2.86 x 109 W is needed to be produced from the reactor. For an entire year, this amounts to a total energy output of 9.0 x 1016 J, which has a mass equivalent of 1 kg. So only 1 kg of mass was converted to energy. Hard to notice 1 kg missing out of 10,000 kg.

Chapter 27:
• 2: for visible range of 400nm - 700nm, λ in crown glass is 263nm - 460nm, for 380-760 nm it is 250-500 nm in crown glass
• 8: d = 1.22 μm
• 11: 577 nm
• 13: m=62 (set Sinθ=1, solve for m=62.5, but the biggest integer value of m=62)
• 23: 8990 lines/cm (solve for d, which is meters/line, convert to cm/line, and invert for lines/cm)
• 25: 5000 lines/cm gives d = 2.00 μm, λ = 707 nm
• 45: a) D=1.35 μm, b) θ=69.7o
• 51: a) You can't use the small angle approximation, because the angles are 17.1306o and 17.1455o, 0.0150o different, b) And you cannot use the small angle approx to determine the separation, because it depends on the angles themselves. Find each y-value, then take the difference to get 0.273 mm
• 58: 107 m
• 62: a) 2.237 x 10-4 radians, which is 0.0128o, b)5.8 km, c) 179 μm d) that is narrower than a pencil line, about the width of two hairs.
• 86: 0.046 W/m2
• 89: Final intensity is 1/4 the original intensity. If middle polarizer is removed, final intensity is zero.

Chapter 26:
• 2: 50.3 diopters
• 4: calculate the magnification, get 5.3 x 10-6, then calc the distance = 3.75 km
• 6: 2.0 m
• 9: Original power = 51 diopters. so 51 = 1/x + 1/0.02, giving x = 1.0 m
• 16: -5 diopters is the prescription for contacts
• 17: -5.4 diopters is the prescription for glasses. (-5.6 D for glasses at 2 cm from eye)

Chapter 25:
• 2: Show that the change of direction equals 180 degrees
• 5: 2.25 x 108 m/s and 2.04 x 108 m/s
• 8: ice, n=1.31
• 13: n=1.457, so probably fused quartz (which is a fairly commonly used material)
• 14: the time delay for two trips through the atmosphere is 5.86 x 10-8 s, which is 2.29 x 10-6% of the round trip time.
• 22: 66.3o
• 29: θred = 46.5o, θviolet = 46.0o
• 36: 20.0 diopters
• 41: Screen is 3.43 m away. Mag = 33.3, so image is 80 cm x 120 cm.
• 42: a) -135 cm, that is, 135 cm from lens on the same side as the mole, b) m = 10, c) 50.0 mm image size
• 57: f = 36.0 cm
• 59: a) m = 0.111, b)image distance = -0.334 cm (behind the cornea), c) f = -0.376 cm, so R =2f = -0.752 cm

Chapter 24:
• 1: yup, you get the speed of light
• 3: 1.50 x 105 V/m
• 7: a) wavelengths from 188 to 556 m for AM, and 2.78 to 3.41 m for FM
• 12: λ = 0.25 μm, which is about the size of the smallest detail you could see with the UV microscope.
• 18: a) 9.46 x 1015 m, b) 1.9 x 1022 m, c) 1.1 x 1026 m
• 23: a) 193 nm has f = 1.55 x 1015 Hz, the resolution ratio will be the ratio of the wavelengths, so for 400 nm light, 400/193 ≈2 two times better resolution.
• 26: in 0.1 ns light goes 3 cm, which is the round trip uncertainty. Half of that is 1.5 cm, the uncertainty of the distance to the moon. b) 3.9 x 10-9 percent
• 32: Intensity, I = Power/area, 318 W/m2, b) B = 1.6 μT, c) E = 490 V/m
• 42: a) 1.50 μm IR light, 200 W, in a 25.0 cm dia circle on your shoulder. Intensity, I=P/A = 4074 W/m2, b) E = 1750 V/m, c) B = 5.84 x 10-6 T, d) to heat 4.00 kg of shoulder requires 2.78 x 104 J, and power = energy/time, so t = E/P = 139 seconds.

Chapter 23:
• 4: a) ccw, b) cw c) cw
• 9: a) 3.04 mV, b) pretty low power, not much temperature increase. Even if R = 0.001 Ω the power is only 9 mW for a short time.
• 12: B = 0.425 T
• 17: 0.63 V, not much
• 27: a) I=0, b) I = cw, c) I = 0, d) I = ccw, e) I=0
• 44: a) 30 turns, (b) 97.5 mA
• 50: a) 2.24, b) 0.447 (which is 1/2.24), c) loss is 20% of what it was before (0.447 squared)
• 67: L = 200 H, b) temperature increases by 5oC

Chapter 22:
• 2: a) right, b) Perp. out of page, c) down, to bottom of page, d) 0, e) left, f) up, to top of page
• 3: a) right, b) perp. into page, c) down, to bottom of page
• 10: 10.1o or 169.9o
• 14: 0.261 T, easily achieved even by permanent magnets.
• 32: a) left, b) perp. out of page, c) up to top of page
• 37: B = 1.80 T
• 48: τ = 0.471 N m, viewed from above, rotation will be cw.
• 57: F = 7.5 x 10-5 N toward the bottom of the page, in line with the right side of the square.
• 68: Need I2 going down. I1/I2 = 1/π
• 84: need FB = mg, so you need to figure out m. I looked up the density of copper, which I won't tell you so you also have the pride of that accomplishment. Ultimately, I got I = 1730 A. If earth contributes a field of 3 x 10-5 T, this is 11% of the field contributed by the lower wire, so decrease its current by 11% to 1540 A.

Chapter 21:
• 3: Series gives the max Rs=786 Ω, parallel gives the min,Rp=20.3 Ω
• 6: a) I=0.400 A, P24=3.84 W, P96=15.4 W, b) Rp=19.2 Ω, I=2.50 A, 2.0 A through R24 and 0.5 A through R96, P24=96 W, P96=24 W
• 16: 2.9994 V
• 23: a) 200 A, b) 10.0 V, c) 2000 W, d) 80 A, Vmot = 4.0 V, Pmot = 320 W
• 26: b) 1.67 A, c) 27.9 kW, d) 20 MΩ
The additional problems handed out, calling the circuits (A), (B) and (C) clockwise from the top
For Resistors
(A) Req=8.75 Ω total power P=9.26 W, I=1.03 A
Note: R2 and R3 are parallel, then R23 is series with R1
(B) Req=3.58 Ω total power P=22.6 W, I=2.52 A
Note: R3, R2, R4 are parallel , then R324is series with R2 ...
(C) Req=3.27 Ω total power P=24.8 W, I=2.75 A

(A) Ceq=3.81 μF, Q=34.3 μC, E=1.54 x 10-4 J
(B) Ceq=12.06 μF, Q=108 μC, E=4.88 x 10-4 J
(C) Ceq=12.8 μF, Q=115 μC, E=5.2 x 10-4 J

Chapter 20:
• 4: 4.00 mA
• 9: 0.12 C, 7.5 x 1017 electrons
• 23: 0.20 mA
• 25: 0.322 Ω
• 27: the Al will be 1.24 times the diameter of the Cu wire
• 40: P = 2 x 1012 W. But not for very long.
• 49: beam power is 1500 W
• 56: \$3.94 billion
• 69: a) = 2.08 x 105 A, for that current, b) the waste heat will be I2R= 4.3 x 1010 W. c) but that is greater than the power output of the generator! So it cannot happen. d) Don't confuse the idea of how much power you want to get to the destination with how much power you need to produce at the source.
• 73: 480 V
• 76: R = 576 Ω, power during melt down is 100 W.

Chapter 19:
• 2: eV=1/2 mv2, so v=1.2 x 108 m/s
• 5: 1940 V
• 7: a) 2 GJ, b) 765 kg of water can evaporate (mcΔT + mLf... remember?)
• 13: yup, they are equivalent
• 17: a) E=2.5 MV/m (mega volts/meter), so no breakdown (no spark), b) at d=1.7 mm you get a big enough E-field.
• 29: Q = +0.833 μC
• 38: sketch so equipotentials are perp to E-field. Higher potential is in direction opposite the arrows of E-field
• 50: 20,000 V
• 61: Cnet = 11.4 μF. (a couple of intermediate combinations give 2.06 and 1.37 μF)
• 66: series: 14.2 μC and 63.8 μJ, parallel: 84.6 μC and 381 μJ

Chapter 18:
• 1: a) 1.25 x 1010 electrons b) 3.13 x 1012 electrons
• 6: a) 1.88 x 106 electrons short of a full load, b) 1.88 x 10-10
• 16: 14.4 N away from Qa, (or in 1 sig fig, 10 N)
• 17: 3.45 x 1016 m/s2
• 20: 1.04 nC
• 25: 85.9 cm right of negative charge, or, if both positive 10.9 cm left of +3 μC
• 30: 69.4 nC and 6.25 N/C
• 43: a) 4 x 107N/C, b) 7 cm, in the middle, c)No, there is no suitable place 0-8 cm, d) The net charge in fig (a) is zero, but the net charge in fig (b) is +1, so E goes to zero faster in the case of fig. (a), and e) Add the electric fields due to the three charges for some point right of 11 cm. This is ugly algebra, which is why they suggest looking at the graph of the sum of the E-fields (if you have some way to make a graph of a function), then the graph of the sum of the E-fields crosses the zero at x=30.6 cm
• 48: Vector addition! All the x-components cancel, and the net vector is 0.102 N in the negative y-direction
• 57: remember circular motion? F=ma=mv2/r, and v=rω, but F=kqQ/r2, put it all together and get ω = 4.12 x 1016 rad/sec (and from v=rω get v=2.2 x 106 m/s, if you are interested)

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