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)0.6 s

A 3.7 kg mass on a spring with k = 50 N/m is pulled 13 cm in the positive direction and released from rest at t = 0. Find its displacement x from equilibrium at t = 0.6 s (with sign).

m = 3.7 kgk = 50 N/mA = 13 cmt = 0.6 s
x = cm
2.Springs & pendulumsHard
t (s)x (cm)t = ?9.6

A body oscillates in simple harmonic motion with period 2 s and amplitude 12 cm. What is the shortest time t it needs to move from equilibrium to a displacement of 9.6 cm?

T = 2 sA = 12 cmx = 9.6 cm
t = s
3.Waves, sound & opticsMedium
FF1 cmdo​ = 30 cmf = 10 cm

An object 1 cm tall stands 30 cm in front of a thin converging lens with a focal length of 10 cm. Find the image height hi (negative for an inverted image).

ho = 1 cmdo = 30 cmf = 10 cm
hi = cm
4.Waves, sound & opticsHard
θa​ = ?n1​ = 1.5n2​ = 1.49n0​ = 1.00

An optical fibre has a core with n₁ = 1.5 and a cladding with n₂ = 1.49. Find the largest angle θa to the fibre axis at which light from air can enter the end of the fibre and still be guided by total internal reflection.

n1 = 1.5n2 = 1.49n0 = 1.00
θa = °

3Solutions

1.Springs & pendulums

Answer: x = −7.71 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 = √(50/3.7) = 3.676 rad/s
ω·t = 3.676·0.6 = 2.206 rad

Displacement

x = A·cos(ω·t) = 13·cos(2.206) = −7.71 cm

Answer

x = −7.71 cm
2.Springs & pendulums

Answer: t = 0.2952 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 = 2π/T = 2π/2 = 3.142 rad/s

Solve for the time

0.8 = sin(ω·t) → ω·t = arcsin(0.8) = 0.9273 rad
t = 0.9273/3.142 = 0.2952 s

Answer

t = 0.2952 s
3.Waves, sound & optics

Answer: hi = −0.5 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.

Thin-lens equation

1/di = 1/f − 1/do = 1/10 − 1/30
di = 15 cm
FF30 cmf = 10 cm

Magnification and height

m = −15/30 = −0.5
hi = −0.5·1 = −0.5 cm

Answer

hi = −0.5 cm
4.Waves, sound & optics

Answer: θa = 9.957 °

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.

Critical angle at the cladding

sin θc = 1.49/1.5 = 0.9933 → θc = 83.38°

Numerical aperture

NA = √(1.5² − 1.49²) = 0.1729

Acceptance angle

θa = arcsin(0.1729) = 9.957°

Answer

θa = 9.957°

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