C. Wave behaviour
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C.1 Simple harmonic motion
C.1.1—Conditions for SHM
• Conditions that lead to simple harmonic motion.
C.1.2—SHM defining equation
• SHM defining equation: a = -ω^2x.
C.1.3—SHM quantities
• Describe SHM using T, f, ω, amplitude, equilibrium position and displacement.
C.1.4—Period, frequency and angular frequency
• Oscillation period relations: T=1/f=2π/ω.
C.1.5—Mass–spring period
• The time period of a mass–spring system is T=2π√(m/k).
C.1.6—Simple pendulum period
• The time period of a simple pendulum in the small-angle approximation is T=2π√(l/g).
C.1.7—Qualitative energy changes in SHM
• Describe qualitatively how kinetic and potential energy change during one cycle of an oscillation; total mechanical energy remains constant for an ideal oscillator.
C.2 Wave model
C.2.1—Transverse and longitudinal travelling waves
• Distinguish transverse and longitudinal travelling waves by comparing particle or field oscillation with the direction of propagation and energy transfer. • Describe the motion of particles in a medium using displacement with position and with time.
C.2.2—Wave quantities and wave equation
• Apply wavelength λ, frequency f, time period T and wave speed v to wave motion using v=fλ=λ/T.
C.2.3—Nature of sound waves
• Explain sound as a mechanical longitudinal wave, including particle oscillations, compressions and rarefactions, and energy transfer through a medium.
C.2.4—Nature of electromagnetic waves
• Explain electromagnetic waves as transverse oscillating electric and magnetic fields that can propagate through a vacuum. • Use the approximate wavelength orders of magnitude in the Physics data booklet without treating them as sharp boundaries.
C.2.5—Mechanical and electromagnetic wave models
• Compare mechanical waves, which require a medium, with electromagnetic waves, which can travel through a vacuum. • Travelling waves transfer energy even when there is no resultant displacement of the medium. • Apply the wave model to both mechanical and electromagnetic waves.
C.3 Wave phenomena
C.3.1—Wavefronts and rays
• Waves travelling in two and three dimensions can be described through the concepts of wavefronts and rays.
C.3.2—Snell’s law
• Snell’s law: n1 sinθ1 = n2 sinθ2.
C.3.3—Refractive index
• Refractive index: n=c/v.
C.3.4—Total internal reflection
• Total internal reflection condition uses critical angle: sinθc=n2/n1.
C.3.5—Superposition
• Superposition adds displacements where waves overlap.
C.3.6—Coherence
• Coherence requires constant phase difference between waves.
C.3.7—Path difference
• Path difference determines constructive or destructive interference.
C.3.8—Two-source interference
• Two-source interference depends on path difference and wavelength.
C.3.9—Young double-slit equation
• Young double-slit spacing: s = λD/d.
C.3.10—Reflection, refraction and transmission at boundaries
• Explain wave behaviour at boundaries in terms of reflection, refraction and transmission. • Sketch and interpret incident, reflected and transmitted wavefronts and rays at normal or oblique incidence within the syllabus guidance.
C.3.11—Diffraction around bodies and through apertures
• Explain diffraction around a body and through an aperture. • Use wavefront–ray diagrams to represent diffraction, and relate greater spreading qualitatively to wavelength and aperture size.
C.4 Standing waves and resonance
C.4.1—Standing wave formation
• Standing waves form by superposition of identical opposite-travelling waves.
C.4.2—Nodes and antinodes
• Identify nodes, antinodes, amplitude and phase along standing waves. • Include relative amplitude and phase difference along the standing wave.
C.4.3—Strings and pipes
• Know standing-wave patterns in strings and pipes.
C.4.4—Resonance
• Resonance relates driving frequency, natural frequency and amplitude.
C.4.5—Damping and resonance
• Damping reduces maximum amplitude and shifts resonant frequency.
C.4.6—Types of damping
• Compare light, critical and heavy damping effects.
C.5 Doppler effect
C.5.1—Doppler effect
• Nature of the Doppler effect for sound waves and electromagnetic waves.
C.5.2—Doppler wavefront diagrams
• Represent Doppler effect with wavefront diagrams for moving source or observer.
C.5.3—Light Doppler approximation
• For light at low relative speed: Δf/f = Δλ/λ ≈ v/c.
C.5.4—Spectral line shifts
• Spectral line shifts reveal motion of stars and galaxies.