Q: What do these H2 Physics quantum notes cover? A: They cover photoelectric effect, de Broglie wavelength, wavefunctions, Heisenberg uncertainty, particle in a box, and spectra for A-Level 9478.
TL;DR These A-Level quantum physics notes cover the photoelectric effect, de Broglie matter waves, wavefunctions, uncertainty, particle-in-a-box energy ladders, and line spectra for H2 Physics 9478. Master wave-particle duality, ψ-algebra, uncertainty maths, and spectra links to move faster in Paper 1 MCQ, Paper 2 explanations, and Modern Physics revision.
Concrete example: how to use this page
If a photoelectric question changes intensity, think number of photons. If it changes frequency, think photon energy. Keeping those two levers separate makes the explanation much shorter.
Revisit the Modern Physics sequence (photoelectric effect → quantum → nuclear) via the H2 Physics notes hub so each derivation here links straight to the nuclear/particle follow-ups. For the full topic map and paper weightings, see our H2 Physics Syllabus 2026-27 overview.
A-Level quantum physics notes: start here, then route
Use this page as the Topic 19 owner for a level quantum physics, quantum physics a level, quantum physics a level notes
queries. Do not start with the formula sheet alone. The SEAB 9478 topic tests model selection: photon energy, de Broglie wavelength, wavefunction probability, uncertainty, particle-in-a-box energy, and spectra.
Search clue
First owner
Next route
a level quantum physics or quantum physics a level
This page
Use the route-selection map below before choosing an equation.
quantum physics a level notes or quantum physics notes
This page
Read the top route map, then jump to the subtopic that matches the question stem.
Use tuition for feedback on explanation structure, spectra, and timed Paper 2 or 3 work.
When Quantum Physics needs marked feedback
Use the notes first if the mistake is recall: the photon equations, de Broglie route, wavefunction language, uncertainty relation, or particle-in-a-box energy formula. Move to A-Level Physics tuition only when the error repeats after self-study.
Repeated script signal
What feedback should target
Next route
You can quote E=hf, but the explanation mixes intensity and frequency.
Separate photon count from photon energy in timed sentences.
Attempt two photoelectric explanations, then get marked feedback if the wording still drifts.
You know λ=h/p, but choose the wrong momentum route.
Decide whether the particle is a photon, electron with speed, or electron with kinetic energy.
Rework the de Broglie checkpoint, then use tuition only if the route choice remains inconsistent.
You can calculate energy levels, but cannot explain spectra or transitions.
Link the energy difference, photon frequency, and emission or absorption direction.
Use the spectra section, then bring a marked Paper 2 or Paper 3 script for diagnosis.
Quantum route-selection map
Use this map before substituting constants. Quantum questions often share the same constants, so the main challenge is deciding which physical model is being tested.
What the question changes or shows
First move
Main route
Misconception check
Light intensity or frequency in the photoelectric effect
Separate photon count from photon energy.
Use E=hf, then compare with the work function and stopping potential if needed.
Higher intensity below threshold still gives no photoelectrons.
Massive particle with momentum or speed
Check whether the particle is massive or a photon.
Use de Broglie wavelength λ=h/p for matter waves.
Do not use p=E/c for a non-relativistic electron in ordinary H2 questions.
A wavefunction or probability density
Identify whether the question asks for amplitude, normalisation, or probability.
Square the wavefunction magnitude and integrate over the allowed region.
ψ is not the probability; ∣ψ∣2 is the probability density.
Localisation or confinement
Look for Δx, Δp, or a box width.
Use uncertainty reasoning or the particle-in-a-box energy ladder.
Smaller confinement does not lower energy; it increases momentum spread and energy spacing.
Atomic or box transition
Find the two energy levels first.
Use ΔE=hf=hc/λ after computing the energy difference.
Emission means the final level is lower; absorption means the final level is higher.
1 Particle nature of light
1.1 Photoelectric effect
Threshold frequency: No electrons emerge when incident light has a frequency below a critical threshold f0; intensity alone cannot compensate. This contradicts classical wave theory and signals discrete packets of energy.
Photon energy: Each packet carries E=hf. Memorise h=6.63×10−34J⋅s.
Photon momentum: Even though m=0, a photon steers a solar sail via
p=cE=λh.
Photoelectric lever checkpoint
When a question changes the light or the metal, name the lever before writing an equation.
Change in the question
What changes physically
What to calculate
Common trap
Increase intensity, same frequency above threshold
More photons arrive each second.
Emission rate or photocurrent increases.
Saying each electron leaves with more kinetic energy.
Increase frequency, same intensity
Each photon carries more energy.
Kmax=hf−ϕ and eVs=Kmax.
Treating frequency as a photon-count change.
Frequency below threshold
Each photon has too little energy to free one electron.
No emission, even if intensity is high.
Adding many low-energy photons together for one electron.
Use a metal with larger work function
More energy is needed before emission starts.
Threshold frequency increases because hf0=ϕ.
Assuming all metals share the same threshold.
Worked check: if hf=5.0eV and ϕ=2.0eV, then Kmax=3.0eV and Vs=3.0V. Doubling the intensity at the same frequency gives more emitted electrons, not 6.0eV electrons.
Misconception check: one photon interacts with one electron in the basic H2 model. Intensity changes the number of attempts per second; frequency changes the energy per attempt.
Mini-drill
Ready to practise beyond the photoelectric effect? Try 10 Quantum Physics questions, covering photons, matter waves and energy levels.
Calculate the momentum of a 500nm photon.
p=λh=5.00×10−76.63×10−34=1.33×10−27kg⋅m⋅s−1.
2 Wave nature of matter
2.1 Electron diffraction
The Davisson-Germer nickel crystal experiment produced concentric rings identical to X-ray patterns, confirming electron wavelengths.
2.2 Firing single particles at a double-slit
Fire electrons one by one: the screen still builds an interference fringe, proving every particle's wavefunction passes through both slits until detected.
2.3 de Broglie formula
λ=ph=mvh.(1)
Use Eq. (1) to explain why soccer balls never show diffraction - their λ is <10−34m.
de Broglie route checkpoint
Before substituting into λ=h/p, decide how the question gives momentum. Most errors come from using a photon formula for an electron, or from forgetting to convert energy into joules before finding momentum.
Given information
First momentum move
Then use
Common trap
Massive particle speed is given
Use p=mv.
λ=h/(mv).
Using p=E/c for an electron moving well below relativistic speeds.
Kinetic energy is given
Use K=p2/(2m), so p=2mK
Electron accelerated through p.d. V
Use K=eV, then p=2meV
Photon wavelength or energy is given
Use photon momentum p=h/λ or p=E/c.
Do not also use p=mv
Worked check: an electron accelerated through 150V gains kinetic energy K=eV=150eV. Convert this to joules before using p=2mK, then substitute into λ=h/p.
Misconception check: de Broglie wavelength belongs to matter waves, but the route to p depends on the data given. The formula λ=h/p is shared; the momentum step is not.
3 Wavefunctions & probability
A particle's state is ψ(x,t); ∣ψ∣2 yields a probability density that integrates to 1 after normalisation.
Superposition lets us add legitimate ψ functions. Sum two slits and you recover the interference pattern in §2.2, or clamp endpoints to get standing waves in a box.
Quick normalisation hack For ψ=Asin(Lnπx) in [0,L]:
∫0L∣ψ∣2dx=A22L=1⇒A=L2.
4 Heisenberg uncertainty
Localising a particle into Δx demands a spread of momenta Δp. Their product obeys
ΔxΔp≳h.
Tight boxes (↓Δx) force high kinetic energy (↑Δp).
Exam cue: the SEAB syllabus uses the order-of-h form above; when you need the full textbook constant, swap in ΔxΔp≥4πh=2ℏ.
5 Particle in a box
Solving the 1-D Schrödinger equation with ψ(0)=ψ(L)=0 yields
En=8mL2h2n2(n=1,2,3,…).(2)
Zero-point energy: even at n=1, the electron cannot be at rest.
Energy gaps widen with smaller L - reason organic dyes with shorter conjugation lengths absorb bluer light (box model for π electrons).
Particle-in-a-box energy checkpoint
Before substituting into En=8mL2h2n2, decide whether the question is asking for a single level, an energy change, or a trend. The square terms make small changes easy to misread.
Question cue
First move
What changes
Common trap
"Find the energy of level n"
Substitute the stated n into n2.
Energy is proportional to n2.
Treating the levels as equally spaced.
"Transition from ni to nf"
Calculate ΔE=Ei−Ef
"Box width is smaller"
Compare the 1/L2 factor.
All levels and gaps increase when L decreases.
Saying a smaller box gives lower energy because there is less space.
"Particle has larger mass"
Compare the 1/m factor.
Levels and gaps decrease for larger mass.
Forgetting that the same n can mean different energies for different particles.
Worked check: if a particle drops from n=3 to n=1, the emitted photon has energy E3−E1=(9−1)8mL2h2=88mL2h2. The gap is eight base units, not three base units.
Misconception check: the quantum number labels the standing-wave mode. It is not the energy itself, so changing from n=1 to n=2 makes the energy four times larger, not twice as large.
6 Quantised atoms & spectra
Electrons in hydrogen occupy discrete orbits. Transitions release/absorb photons that match energy differences, giving line spectra.
Emission lines appear when excited electrons drop to lower levels; absorption lines appear when ground-state electrons jump up, leaving dark gaps in a continuous spectrum. James Webb's spectrographs use the same principle to fingerprint exoplanet atmospheres.
Problem type
A 656nm photon (Balmer H-α) is emitted. Find the energy gap. E=λhc=3.03×10−19J. Identify initial and final n via the Rydberg table.
7 WA timing rules (modern-paper edition)
List givens under every quantum problem before manipulating equations - avoids dropping h or c.
Box problems: write Eq. (2) once, then plug numbers; do not derive under exam pressure.
Convert wavelengths to energy first; the rest is simple bookkeeping.
Need structured practice on Quantum Physics? Our H2 Physics tuition programme covers this topic with weekly problem sets and Paper 4 practical drills.
Comprehensive revision pack
9478 Section VI, Topic 19 Syllabus outcomes
Candidates should be able to:
(a) show an understanding that the existence of a threshold frequency in the photoelectric effect provides evidence that supports the particulate nature of electromagnetic radiation while phenomena such as interference and diffraction provide evidence that supports its wave nature.
(b) state that a photon is a quantum of electromagnetic radiation, and recall and use the equation E=hf for the energy of a photon to solve problems, where h is the Planck constant.
(c) show an understanding that while a photon is massless, it has a momentum given by p=cE and p=λh, where c is the speed of light in free space.
(d) show an understanding that electron diffraction and double-slit interference of single particles provide evidence that supports the wave nature of particles.
(e) recall and use the equation λ=ph for the de Broglie wavelength to solve problems.
(f) show an understanding that the state of a particle can be represented as a wavefunction ψ, e.g. for an electron cloud in an atom, and that the square of the wavefunction amplitude ∣ψ∣2 is the probability density function (including calculation of normalisation factors for square and sinusoidal wavefunctions).
(g) show an understanding that the principle of superposition applies to the wavefunctions describing a particle's position, leading to standing wave solutions for a particle in a box and phenomena such as single-particle interference in double-slit experiments.
(h) show an understanding that the Heisenberg position-momentum uncertainty principle ΔxΔp≳h relates to the necessity of a spread of momenta for localised particles, and apply this to solve problems.
(i) show an understanding of standing wave solutions ψn for the wavefunction of a particle in a one-dimensional infinite square well potential.
(j) solve problems using En=8mL2h2n2
(k) show an understanding of the existence of discrete electronic energy levels for the electron's wavefunction in isolated atoms (e.g. atomic hydrogen) and deduce how this leads to the observation of spectral lines.
(l) distinguish between emission and absorption line spectra.
(m) solve problems involving photon absorption or emission during atomic energy level transitions.
Concept map (in words)
Photons deliver energy E=hf to liberate electrons above threshold frequency. Matter exhibits wave behaviour with λ=ph.
Wavefunctions ψ give probability distributions when ∣ψ∣2 is normalised.
Confining particles quantises energy via En=8mL2n2h2.
Spectral lines correspond to transitions obeying ΔE=hf=λhc.
Key relations
Concept
Expression / reminder
Photon energy
E=hf=λhc
Photoelectric equation
hf=ϕ+21mvmax2 (work function ϕ)
Stopping potential
eVs=21mvmax2
de Broglie wavelength
λ=ph=mvh
Uncertainty principle
ΔxΔp≥4πh (use ≳h for quick estimates)
Particle-in-box energies
En=8mL2n2h2
Transition energy
ΔE=hf=λhc
Derivations & reasoning to master
Photoelectric graph: derive the linear relation between stopping potential and frequency; the slope gives eh.
de Broglie: show consistency with diffraction experiments (Davisson-Germer) using λ=ph.
Particle-in-box normalisation: integrate ψ2 to unity to obtain amplitude A=L2
Spectral identification: use the Rydberg formula to map photon energies to transitions.
Worked example 1 - stopping potential
Ultraviolet light of frequency 8.0×1014Hz shines on a metal with work function 2.6eV. Determine maximum kinetic energy and stopping potential for emitted electrons.
Solution: Kmax=hf−ϕ. Convert to joules with 1eV=1.60×10−19J, then compute Vs=eKmax.
hf=(6.63×10−34)(8.0×1014)=5.30×10−19J.
ϕ=2.6eV=2.6(1.60×10−19)=4.16×10−19J.
Kmax=hf−ϕ=1.14×10−19J⇒Vs=eKmax≈0.71V.
Worked example 2 - particle in a box transition
An electron confined to a one-dimensional box of length 0.35nm makes a transition from n=3 to n=2. Calculate the photon wavelength emitted.
Method: Use En=8mL2n2h2, compute ΔE, convert to wavelength via λ=ΔEhc, and compare to the visible spectrum.
ΔE=(32−22)8mL2h2=58mL2h2.
With L=0.35nm=3.5×10−10m, h=6.63×10−34J⋅s, me=9.11×10−31kg:
ΔE≈2.46×10−18J,λ=ΔEhc≈8.1⋅10−8m≈81nm.
So the photon is in the ultraviolet (visible light is roughly 400 to 700 nm).
Practical & data tasks
Analyse photoelectric experiment data (Vs vs f) to extract Planck's constant.
Simulate particle-in-box wavefunctions with Desmos/Python; verify nodal structure for each n.
Examine hydrogen spectra using a school spectroscope; identify Balmer lines.
Common misconceptions & exam traps
Believing intensity affects photoelectron kinetic energy (it affects number only).
Forgetting to convert eV to J or vice versa.
Mixing de Broglie wavelength with photon wavelength when comparing massive vs massless particles.
Ignoring normalisation when interpreting probability densities.
Quick self-check quiz
What happens to photoelectron emission if light frequency drops below threshold? - No electrons emitted regardless of intensity.
State de Broglie's relation. - λ=ph.
Why can't an electron in a box have zero energy? - Boundary conditions enforce non-zero momentum, so E1>0.
How does confinement length affect energy spacing? - Shorter L increases spacing (proportional to L21).
What information does a line spectrum provide? - Discrete energy level differences of the atom or molecule via ΔE=hf.
Revision workflow
Re-derive the photoelectric equation and practise slope/intercept interpretation weekly.
Solve mixed problems on de Broglie wavelengths for electrons, neutrons, and atoms.
Build flashcards linking spectral series (Lyman, Balmer, Paschen) with wavelength ranges.
Attempt uncertainty principle estimation questions to build physical intuition.
