Amplitude: A wave’s maximum displacement from the equilibrium position
Frequency (f): The number of complete oscillations passing through a point per second
Period (T): The time taken for one full oscillation
Speed (v): The distance travelled by the wave per unit time
Wavelength (λ): The length of one whole oscillation (e.g. the distance between successive peaks/troughs)
Wave equation:
The speed (v) of a wave is equal to the wave’s frequency multiplied by its wavelength
λv = f
Longitudinal waves:
In longitudinal waves, the oscillation of particles is parallel to the direction of energy transfer
Made up of compressions and rarefactions and can’t travel in a vacuum
Transverse waves:
In transverse waves, the oscillations of particles (or fields)are perpendicular to the direction of energy transfer
All electromagnetic (EM) waves are transverse and travel at 3 x 10^8 ms^-1 in a vacuum
Graphs of transverse and longitudinal waves:
Displacement-distance graphs show how the displacement of a particle varies with the distance of wave travel and can be used to measure wavelength
Displacement-time graphs show how the displacement of a particle varies with time and can be used to measure the period of a wave
Further definitions:
Phase: The position of a certain point on a wave cycle
Phase difference: How much a particle/wave lags behind another particle/wave
Path difference: The difference in the distance travelled by two waves
Superposition: Where the displacements of two waves are combined as they pass each other
Coherence: A coherent light source has the same frequency and wavelength and a fixed phase difference
Wavefront: A surface representing points of a wave with the same phase
Interference:
Constructive interference occurs when two waves are in phase and their displacements are added
Destructive interference occurs when waves are completely out of phase and their displacements are subtracted
Phase difference and path difference:
Two waves are in phase if they have the same frequency and wavelength and their phase difference is an integer multiple of 360° (2π radians)
Two waves are completely out of phase if they have the same frequency and wavelength and their phase difference is an odd integer multiple of 180° (π radians)
Stationary waves:
Formed from the superposition of 2 progressive waves travelling in opposite directions with the same frequency, wavelength, and amplitude
No energy is transferred by a stationary wave
In phase - constructive interference occurs forming antinodes
Completely out of phase - destructive interference occurs forming nodes
Speed of a transverse wave on a string:
Speed (v) = √(T/μ) where T is the tension in the string and μ is the mass per unit length of the string
Intensity of radiation:
Intensity is the power per unit area and can be calculated using I = P/A where P is power and A is the area
Refractive index and Snell’s law:
Refractive index (n) measures how much light slows down passing through a material
n = c/v where c is the speed of light in a vacuum and v is the speed of light in the substance
Refraction occurs when a wave enters a different medium, causing it to change direction
Snell’s law: sinθ1/n1 = sinθ2/n2
Critical angle:
The critical angle (C) is reached when the angle of refraction is exactly 90° and light is refracted along the boundary
Total internal reflection:
Total internal reflection occurs when the angle of incidence is greater than the critical angle and the incident refractive index is greater than the material's refractive index at the boundary
The power of a lens is measured by finding the reciprocal of the focal length:
Power = 1 / focal length
Power is positive in converging lenses and negative in diverging lenses
For thin lenses used in combination, the power of the combination is the sum of the powers of the individual lenses:
Power of combination = Power1 + Power2 + ...
A real image can be projected onto a screen, while a virtual image cannot be projected onto a screen
The magnification of a lens is the ratio of the size of the image to the size of the object:
Magnification = image height / object height = u / v
Where u is the distance between the object and the lens axis, v is the distance between the lens axis and the image, and f is the focal length
A polarised wave oscillates in only one plane, and only transverse waves can be polarised
Diffraction is the spreading out of waves when they pass through or around a gap
The diffraction grating equation is:
sin θ = nλ / d
Where d is the distance between the slits, θ is the angle to the normal, n is the order, and λ is the wavelength
Electron diffraction experiments show the wave nature of electrons:
Electrons interact with small gaps between atoms in a crystal lattice and form an interference pattern on a screen
De Broglie hypothesis states that all particles have a wave nature and a particle nature
De Broglie wavelength (λ) can be found using the equation: λ = ph, where h is the Planck constant and p is the momentum of the particle
Pulse-echo technique is used with ultrasound waves for imaging objects, relies on waves being reflected at boundaries between different materials
In the photon model of electromagnetic radiation, EM waves travel in discrete packets called photons, with energy directly proportional to their frequency (E = hf)
Photon energy is directlyproportional to frequency, described by the equation: E = hf
Threshold frequency is the minimum frequency of light required to emit photoelectrons, work function is the minimum energy required for electrons to be emitted from the surface of a metal
Photoelectric equation shows the relationship between work function, frequency of light, and maximum kinetic energy of emitted photoelectrons: hf = Φ + KE(max)
Electronvolt (eV) is a unit of energy, used to express small energies, where 1 eV is equal to the kinetic energy of an electron accelerated across a potential difference of 1 V or 1.6 x 10^-19 J
Photoelectric effect demonstrates evidence for the particle nature of electromagnetic radiation
Atomic line spectra show that electrons in atoms can only exist in discrete energy levels, and transitions between these levels result in the emission or absorption of photons
Energy difference between two energy levels is equal to a specific photon energy emitted or absorbed, calculated using the formula: EΔ = E1 - E2
Photon frequency can be found using the equation: f = (E1 - E2) / h, where f is the photon frequency and h is the Planck constant