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 = 0.9 m

A simple pendulum has a length of 0.9 m. Use g = 9.81 m/s². Find its period T for small swings.

L = 0.9 mg = 9.81 m/s²
T = s
2.Springs & pendulumsHard
0.9 kgk = 250 N/m

A 0.9 kg mass is attached to the lower end of an unstretched vertical spring with k = 250 N/m and released from rest. Use g = 9.81 m/s². Find the greatest speed vmax of the mass.

m = 0.9 kgk = 250 N/mg = 9.81 m/s²
vmax = m/s
3.Waves, sound & opticsMedium
Pβ = ?r = 1 m

A small loudspeaker radiates 2 W of sound power equally in all directions. Find the sound intensity level β at 1 m.

P = 2 Wr = 1 mI0 = 10⁻¹² W/m²
β = dB
4.Waves, sound & opticsHard
θa​ = ?n1​ = 1.48n2​ = 1.38n0​ = 1.00

An optical fibre has a core with n₁ = 1.48 and a cladding with n₂ = 1.38. 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 = 1.48n2 = 1.38n0 = 1.00
θa = °

3Solutions

1.Springs & pendulums

Answer: T = 1.903 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·√(0.9/9.81) = 1.903 s

Answer

T = 1.903 s
2.Springs & pendulums

Answer: vmax = 0.5886 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.

Equilibrium and amplitude

x₀ = m·g/k = 0.9·9.81/250 = 0.03532 m = A

Greatest speed

The speed is largest at equilibrium.

ω = √(250/0.9) = 16.67 rad/s
vmax = A·ω = 0.03532·16.67 = 0.5886 m/s

Answer

vmax = 0.5886 m/s
3.Waves, sound & optics

Answer: β = 112 dB

Waves: a periodic wave moves one wavelength in one period, so v = fλ with T = 1/f. On a stretched string v = √(T/μ), with T the tension and μ = m/L the mass per metre. Sound in air travels at about 343 m/s at 20 °C, light in vacuum at c = 3.00 × 10⁸ m/s. Loudness is measured on a logarithmic scale: β = 10·log₁₀(I/I₀) dB with I₀ = 10⁻¹² W/m², so 10 times the intensity adds 10 dB. A point source spreads its power P over a sphere: I = P/(4πr²).

Intensity

I = P/(4πr²) = 0.1592 W/m²

Level

β = 10·log₁₀(0.1592/10⁻¹²) = 112 dB

Answer

β = 112 dB
4.Waves, sound & optics

Answer: θa = 32.33 °

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 = 1.38/1.48 = 0.9324 → θc = 68.82°

Numerical aperture

NA = √(1.48² − 1.38²) = 0.5348

Acceptance angle

θa = arcsin(0.5348) = 32.33°

Answer

θa = 32.33°

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