Skip to content
Marlbridge

Flashcards · IB Diploma Programme Physics · Topic 3

C. Wave behaviour flashcards

41 cards on Topic 3, subtopics C.1 to C.5. Pick a subtopic or study them all.

Study mode needs JavaScript. Every card is listed below, so you can still cover the answers and test yourself.

All 41 cards

For a quick read-through or printing. Cover the right-hand side to test yourself.

C.1 Simple harmonic motion

Conditions for simple harmonic motion, and its defining equation
The net force acts towards equilibrium and is proportional to displacement (F = −kx). a = −ω²x.
Period, frequency and angular frequency
T = 1/f = 2π/ω, with ω = 2πf in rad s⁻¹.
Periods of a mass–spring system and a simple pendulum
T = 2π√(m/k) T = 2π√(l/g) (small angles) Neither depends on the amplitude.
A 0.50 kg mass on a spring with k = 200 N m⁻¹. Period and ω?
T = 2π√(0.50/200) = 0.314 s; ω = 2π/T = 20 rad s⁻¹
Where in SHM are the speed and the acceleration greatest?
Speed is greatest at equilibrium, where acceleration is zero. Acceleration is greatest at the turning points, where speed is zero.
Energy changes during one oscillation (no damping)
Kinetic energy is maximum at equilibrium and zero at the turning points; potential energy does the opposite; the total stays constant.
Displacement and velocity as functions of time in SHM
x = x₀ sin(ωt + φ) v = ωx₀ cos(ωt + φ) (HL only)
Speed at displacement x, and total energy, in SHM
v = ±ω√(x₀² − x²) E_T = ½mω²x₀² (HL only)
ω = 10 rad s⁻¹, amplitude 0.030 m. Speed at x = 0.020 m?
v = 10 × √(0.030² − 0.020²) = 0.224 m s⁻¹ (HL only)

C.2 Wave model

Travelling wave
A disturbance that transfers energy through a medium or space without the medium as a whole being shifted.
Transverse vs longitudinal waves
Transverse: particles oscillate at right angles to the direction of travel. Longitudinal: particles oscillate along it, forming compressions and rarefactions.
Wavelength, and the wave equation
Wavelength: the distance between neighbouring points in phase. v = fλ = λ/T.
Sound vs electromagnetic waves
Sound: longitudinal, needs a medium, speed depends on the medium. EM: transverse (perpendicular electric and magnetic fields), needs no medium, all travel at c in a vacuum.
A wave has period 0.125 s and wavelength 0.90 m. Speed and frequency?
v = 0.90 ÷ 0.125 = 7.2 m s⁻¹; f = 1/T = 8.0 Hz
Electromagnetic spectrum, long wavelength to short
Radio, microwave, infrared, visible (about 4 to 7 × 10⁻⁷ m), ultraviolet, X-ray, gamma. Frequency increases in that order.
On a longitudinal wave’s displacement graph, where is a compression?
At a point of zero displacement where the particles on either side are displaced towards it (a rarefaction: displaced away from it).

C.3 Wave phenomena

Wavefront and ray
Wavefront: a line or surface joining points at the same phase. Ray: the direction of travel and energy transfer, perpendicular to the wavefronts.
Snell’s law and refractive index
n₁ sin θ₁ = n₂ sin θ₂, i.e. n₁/n₂ = sin θ₂/sin θ₁ = v₂/v₁. n = c/v.
What changes at a boundary when a wave refracts?
Speed and wavelength change (and usually direction). Frequency stays the same.
Critical angle from n = 1.45 into n = 1.20?
sin C = 1.20 ÷ 1.45 = 0.8276, so C = 55.9°. Total internal reflection if the angle of incidence exceeds C.
When is diffraction significant?
When the gap or obstacle is about the same size as the wavelength or smaller. Speed, wavelength and frequency do not change.
Principle of superposition
Where waves meet, the resultant displacement is the sum of the individual displacements, signs included.
Conditions for constructive and destructive interference (coherent sources in phase)
Constructive: path difference = nλ. Destructive: path difference = (n + ½)λ. Coherent: same frequency, constant phase difference.
Young’s double slit: λ = 589 nm, d = 0.45 mm, D = 1.35 m. Fringe separation?
s = λD/d = 589 × 10⁻⁹ × 1.35 ÷ 0.45 × 10⁻³ = 1.77 × 10⁻³ m
Single-slit diffraction: angle of the first minimum
θ = λ/b (radians), b the slit width. A narrower slit gives a wider, dimmer central maximum. (HL only)
Diffraction grating equation, with an example
nλ = d sin θ. 700 lines per mm gives d = 1.43 × 10⁻⁶ m; a second order at 40.0° gives λ = d sin θ / 2 = 459 nm. (HL only)

C.4 Standing waves and resonance

Standing wave, node and antinode
The superposition of two matching waves travelling in opposite directions; no net energy is carried along. Node: permanently zero amplitude. Antinode: maximum amplitude.
Distances in a standing wave
Node to adjacent node: λ/2. Node to adjacent antinode: λ/4.
Allowed frequencies for a string fixed at both ends and a pipe open at both ends
f = nv/2L, all harmonics n = 1, 2, 3, …
Allowed frequencies for a pipe closed at one end
f = nv/4L, odd harmonics only (n = 1, 3, 5, …).
A string of length 0.80 m has wave speed 240 m s⁻¹. First harmonic?
f₁ = 240 ÷ (2 × 0.80) = 150 Hz
Resonance
A large-amplitude response when the driving frequency is at or very near a natural frequency of the system.
Light, critical and heavy damping
Light: several oscillations of decreasing amplitude. Critical: fastest return to equilibrium with no overshoot. Heavy: no oscillation, but a slower return than critical.
Effect of increasing damping on a resonance curve
Lower peak amplitude, a broader peak, and the peak moves slightly below the natural frequency.

C.5 Doppler effect

Doppler effect
The change in observed frequency (and wavelength) when the source and observer are in relative motion.
Moving source vs moving observer
Moving source: wavefronts bunch up in front (shorter λ, higher f) and spread out behind. Moving observer: λ is unchanged, but wavefronts are met more or less often.
Doppler shift for light (v much less than c)
Δf/f = Δλ/λ ≈ v/c. A positive Δλ (redshift) means recession; blueshift means approach.
Doppler formula for sound from a moving source
f′ = f v / (v ± us): minus when the source moves towards the observer, plus when it moves away. (HL only)
A 300 Hz source recedes at 17 m s⁻¹ (v = 340 m s⁻¹). Observed frequency?
f′ = 300 × 340 ÷ (340 + 17) = 286 Hz (HL only)
Doppler formula for sound with a moving observer
f′ = f (v ± uo) / v: plus when moving towards the source, minus when moving away. (HL only)
Two applications of the Doppler effect
Doppler ultrasound: the shifted echo from moving blood gives its speed and direction. Radar speed checks: microwaves reflected from a moving vehicle are shifted.