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
t (s)x (cm)1 s

A 3.7 kg mass on a spring with k = 30 N/m is pulled 10 cm in the positive direction and released from rest at t = 0. Find its displacement x from equilibrium at t = 1 s (with sign).

m = 3.7 kgk = 30 N/mA = 10 cmt = 1 s
x = cm
2.Springs & pendulumsHard
mk = 130 N/mA = 17 cmx = 5 cm

A mass on a spring with k = 130 N/m oscillates on a frictionless surface with an amplitude of 17 cm. Find its kinetic energy K when it is 5 cm from equilibrium.

k = 130 N/mA = 17 cmx = 5 cm
K = J
3.Waves, sound & opticsMedium
FFdo​ = 10 cmf = 8 cm

An object stands 10 cm in front of a thin converging lens with a focal length of 8 cm. Find the image distance di. Use the sign convention 1/f = 1/do + 1/di (f < 0 for a diverging lens, di < 0 for a virtual image).

do = 10 cmf = 8 cm
di = cm
4.Waves, sound & opticsHard
f1​ = 10 cmf2​ = 15 cm25 cm20 cm

Two thin lenses share an axis, 20 cm apart: lens 1 with f₁ = 10 cm and lens 2 with f₂ = 15 cm. An object stands 25 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 = 10 cmf2 = 15 cms = 20 cmdo = 25 cm
di2 = cm

3Solutions

1.Springs & pendulums

Answer: x = −9.571 cm

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 = √(30/3.7) = 2.847 rad/s
ω·t = 2.847·1 = 2.847 rad

Displacement

x = A·cos(ω·t) = 10·cos(2.847) = −9.571 cm

Answer

x = −9.571 cm
2.Springs & pendulums

Answer: K = 1.716 J

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.

Total energy

E = ½·k·A² = ½·130·0.17² = 1.879 J

Spring energy at x

U = ½·k·x² = ½·130·0.05² = 0.1625 J

Kinetic energy

K = 1.879 − 0.1625 = 1.716 J

Answer

K = 1.716 J
3.Waves, sound & optics

Answer: di = 40 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.

Thin-lens equation

1/di = 1/f − 1/do = 1/8 − 1/10
di = 40 cm
FF10 cmf = 8 cm

Ray diagram

real, on the far side of the lens

Answer

di = 40 cm
4.Waves, sound & optics

Answer: di2 = −4.286 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 = 1/10 − 1/25 → di1 = 16.67 cm

Object for lens 2

do2 = 20 − 16.67 = 3.333 cm

Final image

1/di2 = 1/15 − 1/3.333 → di2 = −4.286 cm

Answer

di2 = −4.286 cm

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