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IB Physics HL/Notes/C.3 Wave phenomena

IB Physics HLC.3 Wave phenomenaNotes

Model Wavefronts and rays

Use wavefronts and rays as two linked representations of the same travelling wave. The wavefront marks equal phase; the ray points in the propagation direction and must meet the wavefront at 90 degrees. When a wave enters a slower medium, frequency remains set by the source, so wavelength and wavefront spacing decrease. A correct IB refraction sketch therefore shows the refracted ray bent toward the normal and the refracted wavefronts closer together.

A wavefront is a line in 2D or a surface in 3D joining points that oscillate in phase, such as adjacent crests in the same wave cycle.
A ray is drawn perpendicular to wavefronts and shows the direction of wave travel or energy transfer.
Plane wavefronts have parallel rays; a point source produces circular wavefronts in 2D or spherical wavefronts in 3D with diverging rays.
At a boundary, reflection, refraction, and transmission can be represented with rays; wavefront spacing changes when wave speed and wavelength change.
Angles of incidence, reflection, and refraction are measured between the ray and the normal, not between the ray and the surface.

Match each wavefront/ray representation to the meaning it carries in a C.3 diagram.

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A plane wave enters a slower medium at an angle. Describe how to sketch the transmitted ray and transmitted wavefronts.

Drawing the ray bending correctly but not changing the transmitted wavefront spacing, or measuring angles from the surface instead of the normal.

A plane wave enters a slower medium at an angle. Describe how to sketch the transmitted ray and transmitted wavefronts.

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Model Snell’s law

Snell’s law is a direction rule for refraction. First label the incident medium as 1 and the refracting medium as 2, then measure each angle from the normal. If the second medium has a larger refractive index, light travels more slowly there and the refracted ray is closer to the normal. The wave frequency does not change at the boundary; the wavelength changes because the wave speed changes.

Snell’s law relates the directions of a ray in two media: n1 sin theta1 = n2 sin theta2.
theta1 and theta2 are measured between the ray and the normal to the boundary.
A larger refractive index means a smaller wave speed in that medium, so the ray bends toward the normal when entering the larger-n medium.
At a boundary the source fixes frequency; speed and wavelength change together according to v = f lambda.
Reflection, refraction, and transmission can occur at the same boundary, but Snell’s law describes the transmitted/refracted direction.

Build Snell’s law for a ray crossing from medium 1 into medium 2, then state the angle convention.

Formula
Target formula n1 sin theta1 = n2 sin theta2
n1
refractive index of the incident medium
theta1
angle between the incident ray and the normal
degrees or radians
n2
refractive index of the refracting medium
theta2
angle between the refracted ray and the normal
degrees or radians
1Label the incident and refracting media before choosing variables.medium 1 -> n1, theta1; medium 2 -> n2, theta2
2Place each refractive index with the sine of its own ray angle.n1 sin theta1 = n2 sin theta2
3Check the angle convention before substituting.theta is measured from the normal, not from the surface
4Use the indices to predict the bend direction.larger n -> smaller speed -> ray closer to normal

Light passes from air into glass. Explain why the ray bends toward the normal and write the equation needed to calculate the refracted angle.

Using the angle to the surface, or explaining refraction by saying frequency changes at the boundary.

Light passes from air into glass. Explain why the ray bends toward the normal and write the equation needed to calculate the refracted angle.

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Refractive index

Refractive index is a speed ratio, not a new unit. In vacuum light travels at c, so any material with n greater than 1 gives a lower speed v = c/n. When light enters the material, the source still drives the same frequency. Since v = f lambda, the wavelength decreases when the speed decreases. This is the physical reason a ray bends toward the normal when it enters a higher-index medium.

Refractive index is defined by n = c / v, where c is the speed of light in vacuum and v is the speed of light in the medium.
n has no unit; a larger refractive index means light travels more slowly in that medium.
Rearrange to v = c / n when calculating the speed of light in a transparent medium.
At a boundary, frequency is unchanged because it is fixed by the source; wavelength changes because v = f lambda.
Refractive index is the quantity in Snell’s law that predicts how much a ray bends.

Build the refractive-index formula and rearrange it to find light speed in a medium.

Formula
Target formula n = c / v; v = c / n
n
refractive index of the medium
c
speed of light in vacuum
m s^-1
v
speed of light in the medium
m s^-1
1Start from the definition of refractive index.n = c / v
2Rearrange for the speed in the medium.v = c / n
3Interpret a larger refractive index physically.larger n -> smaller v
4Connect speed change to wavelength at a boundary.frequency unchanged, so lambda changes with v

A transparent material has refractive index 1.60. Calculate the speed of light in the material and state what happens to wavelength when light enters it from air.

Using n = v/c, giving refractive index a unit, or saying frequency changes when light enters the material.

A transparent material has refractive index 1.60. Calculate the speed of light in the material and state what happens to wavelength when light enters it from air.

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Total internal reflection

TIR is a limiting case of refraction. As light travels from a higher refractive index medium into a lower refractive index medium, the refracted ray bends away from the normal. Increasing the incident angle eventually makes the refracted angle 90 degrees; this defines the critical angle. Any larger incident angle gives total internal reflection, so no refracted ray carries energy away into the second medium in the ray model.

The critical angle theta_c is the incident angle in the higher-index medium for which the refracted ray is at 90 degrees to the normal, along the boundary.
For n1 > n2, sin theta_c = n2 / n1.
Total internal reflection occurs only when the incident wave is in the higher-index medium and theta_i > theta_c.
For theta_i < theta_c, some light is transmitted into the second medium; for theta_i = theta_c, the refracted ray travels along the boundary.
In TIR, the wave is reflected back into the original medium and follows the law of reflection.

Spot and repair the incorrect statements about critical angle and total internal reflection.

Spot Errors

Light travels from glass, n = 1.50, into air. Calculate the critical angle and state what happens for an incident angle of 50 degrees.

Forgetting to check that the light starts in the higher-index medium, or reversing the ratio in sin theta_c = n2/n1.

Light travels from glass, n = 1.50, into air. Calculate the critical angle and state what happens for an incident angle of 50 degrees.

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Superposition

Superposition is a local rule. At one instant and one position, read each wave displacement from equilibrium and add the signed values. The rule explains both pulse diagrams and later interference patterns: maxima occur where waves arrive in phase and minima occur where opposite displacements reduce the resultant. The waves are not used up by the overlap in the ideal model.

The principle of superposition states that when waves overlap, the resultant displacement is the sum of the individual displacements at each point.
Displacements above equilibrium can be treated as positive and below equilibrium as negative when adding pulses.
Constructive interference occurs when displacements have the same sign and the resultant magnitude increases.
Destructive interference occurs when displacements have opposite signs; complete cancellation requires equal magnitudes.
After overlap, ideal linear waves continue through each other with their original shape and speed.

Repair the incorrect statements about superposition of overlapping waves.

Spot Errors

Two pulses overlap at a point with displacements +4.0 cm and -1.5 cm. State the resultant displacement and identify whether the overlap is constructive or destructive.

Adding magnitudes only and ignoring that displacement has sign relative to equilibrium.

Two pulses overlap at a point with displacements +4.0 cm and -1.5 cm. State the resultant displacement and identify whether the overlap is constructive or destructive.

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Coherence

Coherence is the condition that makes interference observable as a stable pattern. If the phase difference between two sources drifts, a point on the screen alternates between constructive and destructive conditions and the pattern washes out over time. IB answers should state both parts of the condition: same frequency and constant phase difference.

Two waves are coherent if they have the same frequency and a constant phase difference.
A constant phase difference can be zero or non-zero; coherence does not require the waves to be exactly in phase.
Stable interference patterns require coherence so that maxima and minima remain in fixed positions.
Two independent light sources are usually not coherent because their relative phase changes randomly.
In Young’s double-slit experiment, coherent secondary sources are made by splitting light from the same source.

Repair the incorrect statements about coherence and stable interference.

Spot Errors

State the condition for two sources to be coherent and explain why coherence is needed in a double-source interference experiment.

Writing only “same phase” or “same wavelength” without stating constant phase difference.

State the condition for two sources to be coherent and explain why coherence is needed in a double-source interference experiment.

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Path difference

Path difference turns geometry into interference. If one wave travels an extra whole number of wavelengths, crests still meet crests and the result is constructive. If one wave travels an extra half-integer number of wavelengths, crests meet troughs and the result is destructive. In diagrams, measure both paths to the same observation point before subtracting.

Path difference is delta L = |L1 - L2| for two waves travelling from their sources to the same observation point.
Constructive interference occurs when delta L = m lambda, where m is an integer, so the waves arrive in phase.
Destructive interference occurs when delta L = (m + 1/2) lambda, so the waves arrive in antiphase.
The related phase difference is delta phi = 2 pi delta L / lambda for waves in the same medium.
A bright or dark point in an interference pattern is explained by path difference plus superposition.

Spot and repair errors in these path-difference statements.

Spot Errors

Two coherent waves reach a point with path lengths 4.20 m and 3.90 m. The wavelength is 0.20 m. Determine the type of interference.

Comparing wavelength with one path length instead of the path difference between the two paths.

Two coherent waves reach a point with path lengths 4.20 m and 3.90 m. The wavelength is 0.20 m. Determine the type of interference.

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Model Two-source interference

Two-source interference combines the previous three ideas. Coherence keeps the relative phase fixed, path difference tells whether a point receives waves in phase or antiphase, and superposition gives the resultant displacement. The visible pattern is a map of maxima and minima, not a set of new waves travelling along the nodal lines.

A stable two-source interference pattern requires coherent sources: same frequency and constant phase difference.
The waves must overlap in the same region so superposition can occur.
Antinodal lines are positions of constructive interference where delta L = m lambda.
Nodal lines are positions of destructive interference where delta L = (m + 1/2) lambda.
For two in-phase sources, the central line has zero path difference and is an antinodal line.

Repair the incorrect reasoning in these two-source interference statements.

Spot Errors

Describe the conditions needed to observe a stable two-source interference pattern and explain why the central line is bright for two in-phase sources.

Stating only “waves meet” without mentioning coherent sources or using path difference to justify maxima and minima.

Describe the conditions needed to observe a stable two-source interference pattern and explain why the central line is bright for two in-phase sources.

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Young double-slit equation

Practice

Young’s experiment converts two-source interference into a measurable pattern. The two slits act as coherent secondary sources. Bright fringes occur where path difference is a whole number of wavelengths, and the small-angle geometry gives an approximately constant fringe spacing s = lambda D / d. Use the formula only after identifying which distance is on the screen and which is between the slits.

Young’s double-slit equation is s = lambda D / d.
s is the spacing between adjacent bright fringes or adjacent dark fringes on the screen.
lambda is the wavelength of the light, D is the slit-to-screen distance, and d is the separation between the two slits.
The formula is used for coherent monochromatic light with small angles, typically D much larger than d.
Increasing lambda or D increases fringe spacing; increasing d decreases fringe spacing.
Young’s double-slit experiment is significant because a stable interference pattern is evidence for the wave behaviour of light.

Build Young’s double-slit equation and state how each variable changes the fringe spacing.

Formula
Target formula s = lambda D / d
s
spacing between adjacent bright fringes or adjacent dark fringes
m
lambda
wavelength of the light
m
D
distance from slits to screen
m
d
separation between the two slits
m
1Identify the three distances in the setup before substituting.s on screen; D slits-to-screen; d between slits
2Put wavelength and screen distance in the numerator and slit separation in the denominator.s = lambda D / d
3State the conditions for using the relation.coherent monochromatic light, small angles, D much greater than d
4Predict how the pattern changes.s increases with lambda and D; s decreases as d increases

In a Young double-slit experiment, lambda = 6.0 × 10^-7 m, D = 1.8 m, and d = 0.30 mm. Calculate the fringe spacing and state what happens if d is doubled.

Using millimetres without converting to metres, or using the slit separation as the fringe spacing.

In a Young double-slit experiment, lambda = 6.0 × 10^-7 m, D = 1.8 m, and d = 0.30 mm. Calculate the fringe spacing and state what happens if d is doubled.

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Model Diffraction through apertures and around obstacles

Diffraction is a wavefront effect. When a wave meets an edge or passes through a gap, the wavefront spreads into the region beyond the edge. The comparison that matters is wavelength against the size of the aperture or obstacle. If the gap is much larger than the wavelength, spreading is small. If the gap is about one wavelength wide, the outgoing wavefronts spread strongly.

Diffraction is the spreading of a wave when it passes through an aperture or around an obstacle.
The effect is most noticeable when the aperture or obstacle size is similar to the wavelength.
A narrow gap produces strongly curved outgoing wavefronts; a wide gap gives little spreading and the wave continues almost straight ahead.
Longer wavelengths diffract more for the same aperture size, which is why sound can bend around everyday obstacles more easily than visible light.
Diffraction changes the shape of the wavefront pattern; it does not require the wave speed or frequency to change.

Label the diffraction sketch so each wavefront pattern matches the aperture or obstacle condition.

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Plane water waves pass through a gap. Sketch and explain the difference between the pattern when the gap is about one wavelength wide and when the gap is much wider than the wavelength.

Saying only “waves bend” without comparing aperture size with wavelength, or drawing the same spreading for narrow and wide gaps.

Plane water waves pass through a gap. Sketch and explain the difference between the pattern when the gap is about one wavelength wide and when the gap is much wider than the wavelength.

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Model Double-slit intensity graphs

In an HL double-slit graph, there are two scales to read. The repeating bright and dark fringes are the two-slit interference pattern. Their separation depends on lambda D / d, so larger slit separation gives closer fringes. The slow rise and fall of the fringe heights is the diffraction envelope from the finite width of each slit. A narrower slit produces a wider envelope, so more interference fringes fit under the central envelope.

A double-slit intensity graph plots brightness or intensity against position on the screen.
The closely spaced maxima and minima come from interference between light from the two slits.
The broad envelope comes from diffraction by each individual slit and controls the overall height of the fringes.
Increasing slit separation d decreases the spacing between adjacent interference fringes.
Decreasing individual slit width makes the diffraction envelope wider.
Graph interpretation questions often ask which parameter changed: wavelength, screen distance, slit separation, or slit width.

Interpret a double-slit intensity graph by separating fringe spacing from envelope width.

Graph

The graph plots intensity I against screen position x. Narrow, regularly spaced maxima sit underneath a broad central diffraction envelope with smaller side envelopes.

1Identify the small-scale feature that changed.
2State whether the change points to slit separation or individual slit width.
3Explain the direction of the change using s = lambda D / d.

Two double-slit intensity graphs use the same wavelength and screen distance. In graph B the fringes are closer together, but the broad envelope has the same width. Explain what changed in the apparatus.

Saying the slit width changed when only fringe spacing changed, or ignoring the envelope entirely.

Two double-slit intensity graphs use the same wavelength and screen distance. In graph B the fringes are closer together, but the broad envelope has the same width. Explain what changed in the apparatus.

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Model Single-slit diffraction

Single-slit diffraction is not just “light spreading”; HL expects the intensity pattern. The strongest feature is the broad central maximum. The first dark minima occur where the path difference across the slit produces cancellation, summarized by sin theta = lambda/a for m = 1. If a decreases, lambda/a increases, so the first minima move farther from the centre and the central maximum widens.

Monochromatic light through a single slit forms a broad central maximum with weaker side maxima separated by dark minima.
For slit width a, minima occur at sin theta = m lambda / a, where m = 1, 2, 3, ... on either side of the centre.
The first minima at m = 1 define the angular half-width of the central maximum.
A narrower slit gives larger theta for the first minima, so the central maximum becomes wider.
A longer wavelength also produces a wider diffraction pattern for the same slit width.

Build the single-slit minima condition and use it to predict the diffraction width.

Formula
Target formula sin theta = m lambda / a
theta
angle from the central axis to a diffraction minimum
degrees or radians
m
order number of the minimum, m = 1, 2, 3, ...
lambda
wavelength of the light
m
a
single-slit width
m
1Identify that the pattern is from one slit, not two slits.single slit -> use slit width a
2Write the minima condition.sin theta = m lambda / a
3Use m = 1 for the first minimum and central maximum half-width.sin theta_1 = lambda / a
4Predict the effect of slit width.smaller a -> larger theta_1 -> wider central maximum

Monochromatic light of wavelength 5.0 × 10^-7 m passes through a single slit of width 2.0 × 10^-5 m. Estimate the angle to the first minimum and state how the pattern changes if the slit is narrowed.

Using the double-slit equation or identifying a maximum when the formula locates minima.

Monochromatic light of wavelength 5.0 × 10^-7 m passes through a single slit of width 2.0 × 10^-5 m. Estimate the angle to the first minimum and state how the pattern changes if the slit is narrowed.

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Model Diffraction envelope

A double-slit pattern has two layers. The separation between the two slits controls the closely spaced interference maxima. The finite width of each slit controls the broad diffraction envelope that changes the heights of those maxima. Where the envelope is zero, a possible interference maximum is missing because the single-slit diffraction from each slit contributes no intensity at that angle.

The fine, regularly spaced fringes in a double-slit pattern come from interference between the two slits.
Because each slit has finite width, each slit also produces a single-slit diffraction pattern.
The observed intensity is the two-slit interference pattern modulated by the single-slit diffraction envelope.
An interference maximum can be suppressed if it occurs at an angle where the single-slit envelope has a minimum.
Slit separation d controls fringe spacing; slit width a controls the envelope width.

Repair the incorrect statements about double-slit diffraction envelopes.

Spot Errors

A double-slit intensity graph shows regularly spaced bright fringes, but one expected bright fringe is absent at a position where the broad envelope is zero. Explain this observation.

Explaining a missing maximum only with two-source path difference and ignoring the single-slit envelope.

A double-slit intensity graph shows regularly spaced bright fringes, but one expected bright fringe is absent at a position where the broad envelope is zero. Explain this observation.

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Model Diffraction gratings

A grating is a many-source interference system. For a bright principal maximum, light from neighbouring slits must arrive in phase, so their path difference d sin theta must equal an integer number of wavelengths. More slits narrow the maxima because off-condition angles cancel more strongly. Before calculating an angle, convert line density into slit spacing if necessary and check that the requested order is possible.

A diffraction grating has many equally spaced slits or lines separated by distance d.
Principal maxima occur when n lambda = d sin theta, where n is the order number 0, 1, 2, ...
The central maximum is n = 0; higher orders appear symmetrically on both sides for normal incidence.
If the grating has N lines per metre, the slit spacing is d = 1/N.
Only orders with n lambda <= d are possible because sin theta cannot be greater than 1.
Many slits make maxima sharper and brighter, which helps precise wavelength measurement.

Build the diffraction grating equation and check whether a requested order is possible.

Formula
Target formula n lambda = d sin theta
n
diffraction order number, n = 0, 1, 2, ...
lambda
wavelength of the light
m
d
spacing between adjacent grating lines or slits
m
theta
angle from the central maximum to the order
degrees or radians
1Identify the adjacent-slit path difference.path difference = d sin theta
2Set that path difference equal to an integer number of wavelengths.d sin theta = n lambda
3Convert line density to slit spacing if needed.d = 1 / (lines per metre)
4Check that the order can exist.n lambda <= d because sin theta <= 1

A grating has 500 lines per mm and is illuminated with light of wavelength 600 nm. Calculate the angle of the first-order maximum and determine whether a fourth order is possible.

Using 500 as d, failing to convert mm to m, or forgetting to check sin theta <= 1 for high orders.

A grating has 500 lines per mm and is illuminated with light of wavelength 600 nm. Calculate the angle of the first-order maximum and determine whether a fourth order is possible.

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Retrieve the Core C.3 Wave phenomena Model

Review

Core C.3 is secure when the student can move from a wave diagram to the correct physical rule. Wavefronts and rays set the geometry. Refraction changes speed and wavelength but not frequency. TIR requires a direction condition before a critical-angle calculation. Diffraction depends on size compared with wavelength. Interference then builds from superposition, coherence, and path difference, ending with Young’s measurable fringe spacing.

Wavefronts join points in phase; rays are perpendicular to wavefronts and show propagation direction.
Refraction uses n = c/v and n1 sin theta1 = n2 sin theta2, with angles measured from the normal and frequency unchanged at a boundary.
Total internal reflection requires higher-index to lower-index travel and theta_i greater than theta_c, where sin theta_c = n2/n1.
Diffraction is strongest when an aperture or obstacle size is comparable to wavelength.
Superposition adds displacements; coherence and path difference decide stable constructive or destructive interference.
Young’s double-slit formula s = lambda D/d links fringe spacing to wavelength, screen distance, and slit separation.

Match each C.3 core cue to the physics response it should trigger.

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Retrieve the HL C.3 Wave phenomena Model

Review

HL C.3 is mostly about choosing the right scale. Single-slit diffraction uses slit width a to find minima and envelope width. Double-slit interference uses slit separation d to find fine fringe spacing, while the finite slit width creates the broad envelope. A grating uses adjacent-line spacing d and integer order n to locate sharp principal maxima. The same symbols can appear in different models, so the diagram or graph feature must be identified before choosing an equation.

Double-slit intensity graphs contain regularly spaced interference fringes under a broader diffraction envelope.
Single-slit dark minima satisfy sin theta = m lambda/a, where a is the slit width and m is a non-zero integer.
Narrowing a single slit makes the central maximum wider because the first minima move to larger angles.
The diffraction envelope is caused by the finite width of each slit; slit separation controls the fine fringe spacing.
A missing or suppressed double-slit maximum occurs when a possible interference maximum lies at an envelope minimum.
Diffraction grating principal maxima satisfy n lambda = d sin theta, with possible orders limited by n lambda <= d.

Match each HL C.3 cue to the graph feature, parameter, or equation it should trigger.

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