Waves and Optics: cram pack

Formula sheets, the key method steps for every topic and 4 practice problems, with full solutions at the back.

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1Formulas and methods

Springs & pendulums

Mass on a spring
T = 2π·√(m/k)
Pendulum
T = 2π·√(L/g)
Angular frequency
ω = √(k/m) = 2π/T
Maximum speed and acceleration
vmax = A·ω, amax = A·ω²
Energy
E = ½·k·A²

Waves, sound & optics

Wave speed
v = fλ, T = 1/f
String
v = √(T/μ), μ = m/L
Sound level
β = 10·log10(I/I0), I0 = 10⁻¹² W/m²
Point source
I = P/(4πr²)
Standing waves
string or open pipe fn = n·v/(2L); closed pipe fn = n·v/(4L), n odd
Doppler effect
f′ = f·(v ± vo)/(v ∓ vs)
Refractive index
n = c/v, λ = λ0/n
Snell’s law
n1sin θ1 = n2sin θ2
Critical angle
sin θc = n2/n1
Optical fibre
NA = sin θa = √(n1² − n2²)
Lenses and mirrors
1/f = 1/do + 1/di, m = −di/do, mirror f = R/2
Double slit
d·sin θ = mλ, ym = mλL/d
Grating
d = 1/N, d·sin θ = mλ, mmax ≤ d/λ
Single slit
a·sin θ = mλ (dark), w = 2λL/a

Method

  1. Identify the kind of problem: wave speed, sound level, standing wave, Doppler, refraction, lens or mirror, or interference.
  2. Write the relation first: v = fλ, β = 10·log(I/I₀), fₙ = n·v/(2L) or n·v/(4L), f′ = f(v ± vo)/(v ∓ vs), n₁sin θ₁ = n₂sin θ₂, 1/f = 1/d₀ + 1/dᵢ, d·sin θ = mλ.
  3. Convert units: nm, mm and cm to m, and check whether angles are measured from the normal.
  4. Check signs and plausibility: a virtual image has dᵢ < 0, an approaching source sounds higher, a closed pipe has only odd harmonics.

2Practice problems

1.Springs & pendulumsMedium
L = 2.9 m

A simple pendulum has a length of 2.9 m. Use g = 9.81 m/s². Find its period T for small swings.

L = 2.9 mg = 9.81 m/s²
T = s
2.Springs & pendulumsHard
3.8 kgk = 420 N/mA = 2 cm

A 3.8 kg mass on a spring with k = 420 N/m is pulled 2 cm from equilibrium and released. Find its maximum speed vmax.

m = 3.8 kgk = 420 N/mA = 2 cm
vmax = m/s
3.Waves, sound & opticsMedium
S34 m/sOf = 400 Hz

A source of 400 Hz moves at 34 m/s away from a stationary observer. The speed of sound is 343 m/s. Find the frequency f′ that the observer hears.

f = 400 Hzv = 343 m/svs = 34 m/s
f′ = Hz
4.Waves, sound & opticsHard
f1​ = 15 cmf2​ = −10 cm30 cm60 cm

Two thin lenses share an axis, 60 cm apart: lens 1 with f₁ = 15 cm and lens 2 with f₂ = −10 cm. An object stands 30 cm in front of lens 1. Find the position di2 of the final image measured from lens 2 (positive beyond lens 2, real-is-positive convention).

f1 = 15 cmf2 = −10 cms = 60 cmdo = 30 cm
di2 = cm

3Solutions

1.Springs & pendulums

Answer: T = 3.416 s

Simple harmonic motion: a mass m on a spring of stiffness k oscillates with angular frequency ω = √(k/m) and period T = 2π/ω = 2π·√(m/k). A simple pendulum of length L has T = 2π·√(L/g). With amplitude A, the largest speed is A·ω, the largest acceleration A·ω² and the energy ½·k·A².

Pendulum period

T = 2π·√(2.9/9.81) = 3.416 s

Answer

T = 3.416 s
2.Springs & pendulums

Answer: vmax = 0.2103 m/s

Simple harmonic motion: a mass m on a spring of stiffness k oscillates with angular frequency ω = √(k/m) and period T = 2π/ω = 2π·√(m/k). A simple pendulum of length L has T = 2π·√(L/g). With amplitude A, the largest speed is A·ω, the largest acceleration A·ω² and the energy ½·k·A².

Angular frequency

ω = √(420/3.8) = 10.51 rad/s

Maximum speed

vmax = A·ω = 0.02·10.51 = 0.2103 m/s

Answer

vmax = 0.2103 m/s
3.Waves, sound & optics

Answer: f′ = 363.9 Hz

Standing waves and the Doppler effect: a string fixed at both ends, or a pipe open at both ends, fits whole half-wavelengths: L = nλ/2, fn = n·v/(2L), n = 1, 2, 3, … A pipe closed at one end has a node at the closed end and an antinode at the open end: L = nλ/4 with odd n only, fn = n·v/(4L). When source or observer move along the line between them, f′ = f·(v ± vo)/(v ∓ vs): use the upper signs for motion towards each other. Two waves of nearly equal frequency beat at |f₁ − f₂|.

Doppler formula

f′ = f·(v − vo)/(v + vs) = 400·(343 − 0)/(343 + 34)
f′ = 363.9 Hz

Answer

f′ = 363.9 Hz
4.Waves, sound & optics

Answer: di2 = −7.5 cm

Geometric optics: at a boundary, n₁·sin θ₁ = n₂·sin θ₂ (Snell's law), with angles measured from the normal and n = c/v. Going into a slower medium the ray bends towards the normal. From a denser medium (n₁ > n₂) beyond the critical angle θc = arcsin(n₂/n₁) all light is reflected: total internal reflection. Thin lenses and spherical mirrors obey 1/f = 1/do + 1/di with the magnification m = −di/do. Sign convention: f > 0 for a converging lens and a concave mirror (f = R/2), f < 0 for a diverging lens and a convex mirror; di > 0 for a real image, di < 0 for a virtual one, and m < 0 for an inverted image.

Image of lens 1

1/di1 = 1/15 − 1/30 → di1 = 30 cm

Object for lens 2

do2 = 60 − 30 = 30 cm

Final image

1/di2 = 1/(−10) − 1/30 → di2 = −7.5 cm

Answer

di2 = −7.5 cm

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