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Spec mapping: OCR H556 Module 4.5 — Quantum physics (the particulate nature of electromagnetic radiation; the photon as a quantum of energy with E=hf=hc/λ; Planck's constant). Refer to the official OCR H556 specification document for exact wording.
For most of the nineteenth century, physicists were convinced that light was a wave. Young's double-slit experiment (1801) showed that light interferes. Fresnel, Fraunhofer and Kirchhoff built elegant mathematical theories of diffraction. Maxwell (1865) showed that light is an oscillation of the electromagnetic field travelling at the speed c=1/μ0ε0. By 1900, the wave theory seemed complete. Optics was a solved problem.
Then, within a few short years at the beginning of the twentieth century, experiments began to show that this neat picture was incomplete. Blackbody radiation, the photoelectric effect, atomic line spectra — none of them could be explained by a pure wave theory of light, no matter how sophisticated. In 1900 Max Planck proposed, reluctantly, that electromagnetic energy is emitted and absorbed in discrete packets. In 1905 Albert Einstein went further: he proposed that light itself consists of discrete, localised packets of energy — photons — which travel through space and interact with matter one at a time.
This lesson opens the OCR H556 quantum-physics module. It introduces the photon model: what a photon is, how much energy it carries, the universal constants involved, and the units (joule and electronvolt) used throughout the rest of the topic. It is the conceptual foundation for the photoelectric effect (lessons 3–5), wave–particle duality (lessons 6–8), and atomic spectra (lessons 9–10).
The word quantum (Latin quantus, "how much") refers to the smallest discrete amount of something that can exist or be exchanged. A quantum of charge is the magnitude of the electronic charge, e=1.60×10−19 C; you cannot have a charge of 0.3e. A quantum of electromagnetic energy at frequency f is a photon, with energy E=hf; you cannot have half a photon.
The essential claim of quantum physics is this: some quantities that look continuous in classical physics are, at a deep level, discrete — they come in integer multiples of a fundamental unit, the quantum. The continuity we see in everyday phenomena (a bright bulb appears to emit a smooth stream of light) is an illusion of large numbers; at the level of single atoms and single photons, discreteness reveals itself.
The transition from classical to quantum physics is not a matter of small refinements but of conceptual revolution. The discrete photon model resolves three nineteenth-century puzzles in one stroke — blackbody radiation (Planck), the photoelectric effect (Einstein) and atomic spectra (Bohr) — none of which a pure wave theory could touch.
A photon is a quantum of electromagnetic energy — a discrete, indivisible packet of light. It has the following properties:
The photon is not a tiny classical particle like a billiard ball. While propagating it can pass through both slits of a double-slit apparatus and interfere with itself; while being detected (by a photocell, a photographic emulsion, a retinal rod) it deposits its energy at a single point in a single event. This wave-in-flight, particle-on-arrival behaviour is the first manifestation of wave–particle duality, which we develop properly in lessons 6–8.
A useful image: a photon is the smallest unit of a "click" of the electromagnetic field. Bright light is many clicks per second; dim light is few clicks. Every click delivers exactly hf joules.
The central equation of the photon model is the Planck–Einstein relation:
E=hf
where:
The OCR data sheet value is
h=6.63×10−34 J s
Note the units carefully: joule seconds. Energy multiplied by time. This combination — called action in analytical mechanics — is the natural currency of quantum physics. Wherever quantum effects appear, h appears.
Because every electromagnetic wave in vacuum satisfies c=fλ, we can substitute f=c/λ to obtain the equivalent wavelength form:
E=hf=λhc
This is often more convenient for laboratory work, because optical instruments measure wavelength directly (with a diffraction grating, for example).
Exam Tip: Know both forms — E=hf and E=hc/λ — and recognise from the wording of a question which one is most direct. If wavelength is given, use hc/λ; if frequency is given, use hf. Converting between f and λ via c=fλ is a sign you are taking the long way round.
The product hc comes up so often in calculations that it is worth memorising:
hc=(6.63×10−34)×(3.00×108)=1.99×10−25 J m
Equivalently, in eV nm (after dividing through by e=1.60×10−19 and converting metres to nanometres):
hc≈1240 eV nm
This second form means that, for any wavelength quoted in nanometres, the photon energy in electronvolts is simply 1240/λ(nm) — a powerful shortcut for fast mental estimates.
Planck's constant h=6.63×10−34 J s is extraordinarily small on human scales, which is why quantum effects are not obvious in everyday life. A single photon of visible green light (λ=550 nm) has energy
E=λhc=550×10−91.99×10−25≈3.6×10−19 J≈2.3 eV
A 100 W bulb therefore emits of order 100/(3.6×10−19)≈3×1020 photons every second. The arrival of so many discrete quanta blends into the smooth sensation of "light"; the human eye cannot, in normal conditions, resolve individual photons (though dark-adapted retinal rods can actually respond to single quanta).
Quantum effects become visible only when we zoom in to where small numbers of photons matter — single-photon avalanche diodes, photomultiplier tubes, single-molecule fluorescence, the rod cells of a dark-adapted eye. In these regimes the discreteness of light is unmistakable.
Working with joules at the atomic scale is cumbersome because atomic energies are typically of order 10−18 to 10−19 J. For this reason physicists use a more practical unit: the electronvolt (eV).
Definition. One electronvolt is the kinetic energy gained by an electron (of charge e=1.60×10−19 C) when accelerated from rest through a potential difference of one volt:
W=eV=(1.60×10−19 C)(1 V)=1.60×10−19 J
So the conversion factor is
1 eV=1.60×10−19 J
and equivalently 1 J≈6.24×1018 eV. The electronvolt is not an SI unit but is universally used in atomic, molecular and particle physics because the relevant energies come out as manageable numbers:
| Physical quantity | Typical energy |
|---|---|
| Visible photon | 1.6 – 3.3 eV |
| Work function of caesium | 2.1 eV |
| Ionisation energy of hydrogen | 13.6 eV |
| X-ray photon | 102 eV – 105 eV |
| Nuclear binding energy per nucleon | ∼8 MeV |
| LHC collision energy | up to 13 TeV |
(SI prefixes: keV =103 eV, MeV =106 eV, GeV =109 eV, TeV =1012 eV.)
Exam Tip: When OCR asks for an answer in eV, divide the joule answer by 1.60×10−19. When OCR asks for joules, multiply by 1.60×10−19. A reliable sanity check: an atomic-scale photon energy should be a few eV, not 10−38 eV; a chemical bond energy should be a few eV per molecule, not 1018 eV.
A photon of red light has wavelength λ=650 nm. Calculate its energy in (a) joules and (b) electronvolts.
Solution.
(a) Using E=hc/λ with hc=1.99×10−25 J m and λ=650×10−9 m:
E=650×10−91.99×10−25=3.06×10−19 J
(b) Converting to electronvolts:
E=1.60×10−193.06×10−19=1.91 eV
Equivalently, using the shortcut E(eV)=1240/λ(nm)=1240/650≈1.91 eV — same answer in one step.
A red photon therefore carries about 1.9 eV — close to the band gap of silicon and to several common metal work functions.
A photon has energy 2.50 eV. What is its frequency?
Solution. First convert to joules:
E=(2.50)(1.60×10−19)=4.00×10−19 J
Then use f=E/h:
f=6.63×10−344.00×10−19=6.03×1014 Hz
This lies in the visible range (the corresponding wavelength is λ=c/f≈497 nm — blue-green).
A green laser pointer (λ=532 nm) has rated power 1.0 mW. How many photons does it emit per second?
Solution. Photon energy:
Ephoton=λhc=532×10−91.99×10−25=3.74×10−19 J
Photon flux:
tN=EphotonP=3.74×10−191.0×10−3≈2.7×1015 s−1
Almost three quadrillion photons per second — which is why the beam appears continuous to the eye. Quantum discreteness is hidden by sheer numerical overwhelm.
Because photon energy scales linearly with frequency (and inversely with wavelength), each region of the electromagnetic spectrum corresponds to a characteristic photon energy range:
flowchart LR
Radio["Radio<br/>~10⁻⁹ eV<br/>λ ~ m – km"]
Micro["Microwave<br/>~10⁻⁵ eV<br/>λ ~ mm – cm"]
IR["Infrared<br/>~10⁻² eV<br/>λ ~ μm"]
Vis["Visible<br/>~2 eV<br/>λ ~ 400 – 700 nm"]
UV["Ultraviolet<br/>~10 eV<br/>λ ~ 10 – 400 nm"]
Xray["X-ray<br/>~10³ – 10⁵ eV<br/>λ ~ 0.01 – 10 nm"]
Gamma["Gamma<br/>>10⁵ eV<br/>λ < 0.01 nm"]
Radio --> Micro --> IR --> Vis --> UV --> Xray --> Gamma
A radio photon (∼10−9 eV) is so feeble that no detector responds to individual quanta; radio receivers sum the action of vast numbers of coherent photons, behaving classically. A gamma photon (>105 eV) is energetic enough to ionise atoms one at a time, and its interaction is always discrete. Twelve orders of magnitude separate the two ends of the spectrum — and this same factor of 1012 explains why radio waves are harmless to biological tissue while gamma rays damage DNA.
The following flowchart summarises when an electromagnetic exchange behaves classically (wave-like) and when the photon picture is essential:
flowchart TD
A[Electromagnetic energy exchange] --> B{Photon energy hf<br/>vs atomic-scale energies}
B -- "hf << atomic scale<br/>(radio, microwave)" --> C[Wave picture adequate<br/>continuous classical limit]
B -- "hf comparable to<br/>atomic energies<br/>(visible, UV, X-ray)" --> D[Photon picture essential<br/>discrete absorption/emission]
D --> E[Photoelectric effect,<br/>atomic spectra, ionisation]
C --> F[Antennas, waveguides,<br/>Maxwell theory]
The diagram below sketches the photon picture of light: a source emits photons of energy E=hf; the photons travel at c until they encounter a detector, where each photon is absorbed in a single discrete event.
Einstein's 1905 argument from the photoelectric effect (lessons 3 and 4) is the most spectacular justification of the photon model, but it was not the first. The earlier motivation came from blackbody radiation — the spectrum of electromagnetic energy emitted by a hot opaque body.
A blackbody at absolute temperature T emits a characteristic continuous spectrum that peaks at a wavelength inversely proportional to T (Wien's law: λpeakT≈2.9×10−3 m K) and integrates to a total power proportional to T4 (Stefan's law). Classical statistical mechanics, applied to the modes of the electromagnetic field inside a cavity, predicted that the spectrum should diverge at short wavelengths — the so-called "ultraviolet catastrophe" — with an infinite total radiated power. This was nonsense; experiment showed a finite peak.
Max Planck solved the puzzle in 1900 by postulating that each oscillator mode of frequency f can only exchange energy with the field in integer multiples of hf. The high-frequency modes are then statistically suppressed (because a single quantum hf exceeds the available thermal energy kBT), and the catastrophe is averted. Planck himself viewed this as a calculational trick, not a physical claim. It was Einstein in 1905 who took the bolder step of arguing that the quantisation is a property of the radiation field itself, not merely of the matter that exchanges energy with it.
Blackbody radiation is not directly on the OCR H556 specification, but it is worth knowing as the historical seed of the photon concept — and the same Planck constant h that appears in the blackbody formula reappears in the photoelectric effect, atomic spectra and de Broglie's hypothesis. The unity of Nature is enforced through a single number.
Question (8 marks): A research laboratory uses two monochromatic light sources. Source X emits red light of wavelength λX=700 nm at a power of 5.0 mW. Source Y emits ultraviolet light of wavelength λY=280 nm at a power of 2.0 mW.
(a) Calculate the energy of a single photon from each source, expressing each answer in both joules and electronvolts. [3]
(b) Determine the number of photons emitted per second by each source. [2]
(c) A student claims that "Source X is the more dangerous because it has the higher power and so delivers more energy per second." Discuss the validity of this claim, using ideas from the photon model. [3]
| Mark | AO | Awarded for |
|---|---|---|
| 1 | AO2 | EX=hc/λX=2.84×10−19 J |
| 2 | AO2 | EY=hc/λY=7.11×10−19 J |
| 3 | AO2 | Conversion to eV (1.78 eV and 4.44 eV respectively) |
| 4 | AO2 | NX/t=PX/EX=1.76×1016 s−1 |
| 5 | AO2 | NY/t=PY/EY=2.81×1015 s−1 |
| 6 | AO3 | Recognises that "danger" depends on photon energy, not total power |
| 7 | AO3 | UV photons (4.44 eV) can ionise / break chemical bonds; red photons (1.78 eV) cannot |
| 8 | AO3 | Conclusion: Source Y is the more biologically dangerous despite lower total power |
AO split: AO1 = 0, AO2 = 5, AO3 = 3.
Mid-band response (4/8):
(a) EX=hc/λ=(6.63×10−34)(3×108)/(700×10−9)=2.84×10−19 J =1.78 eV. For Y: EY=hc/λ=7.11×10−19 J = 4.44 eV.
(b) Number per second = power / energy per photon. For X: 1.76×1016. For Y: 2.81×1015.
(c) The student is right because X has more power. More power means more energy.
Examiner commentary: The next-band move is to engage with the biological effect of a single photon, not just the total power. Marks 1–5 awarded for the numerical calculations. Mark 6 not awarded — the candidate accepts the student's claim uncritically rather than questioning it. Marks 7 and 8 lost because the answer never identifies that UV photon energy can ionise molecules while red photon energy cannot, regardless of how many red photons there are. This is the central conceptual point of the photon model and is missed entirely.
Stronger response (6/8):
(a) Photon energies:
EX=λXhc=700×10−91.99×10−25=2.84×10−19 J=1.78 eV
EY=λYhc=280×10−91.99×10−25=7.11×10−19 J=4.44 eV
(b) Photon flux:
tNX=EXPX=2.84×10−195.0×10−3=1.76×1016 s−1
tNY=EYPY=7.11×10−192.0×10−3=2.81×1015 s−1
(c) The student is wrong. The biological effect of light depends on the energy per photon, not the total power. The UV photons from Y have higher energy (4.44 eV vs 1.78 eV) and so can damage DNA by ionising it, while red photons from X cannot regardless of intensity. Source Y is more dangerous despite delivering less total power.
Examiner commentary: To lift this to top-band the candidate would need to be explicit about the threshold-energy concept — that ionisation or bond-breaking requires a photon energy exceeding a specific binding energy of the target molecule, so individual photons must be above threshold; pouring more low-energy photons at a target does not help. Marks 1–7 awarded; Mark 8 partial — the conclusion is stated but not framed in terms of the threshold-energy principle that connects this answer to the photoelectric work function studied later in the topic.
Top-band response (8/8):
(a) Using E=hc/λ with hc=1.99×10−25 J m:
EX=700×10−91.99×10−25=2.84×10−19 J=1.60×10−192.84×10−19=1.78 eV
EY=280×10−91.99×10−25=7.11×10−19 J=4.44 eV
(b) Photon flux N/t=P/Ephoton:
tNX=2.84×10−195.0×10−3≈1.76×1016 s−1
tNY=7.11×10−192.0×10−3≈2.81×1015 s−1
Source X emits roughly six times as many photons per second as Y, despite having only 2.5 times the power, because each X photon carries 2.5 times less energy.
(c) The student's claim conflates intensity (joules per second per unit area) with photon energy (joules per quantum). Biological damage from electromagnetic radiation depends on whether single photons individually exceed a threshold energy — typically the ionisation energy of biomolecules (∼3−10 eV) or the bond-dissociation energy of DNA strands (∼3−5 eV). UV photons from Y at 4.44 eV exceed this threshold and can therefore initiate single-quantum ionisation or bond rupture; red photons from X at 1.78 eV cannot, regardless of how many arrive. Pouring a billion red photons onto a DNA molecule simply heats it; one UV photon can break a bond. This is exactly the threshold-energy concept formalised in Einstein's photoelectric equation hf=ϕ+KEmax (later in this module): a single photon either does or does not have enough energy to liberate an electron, and total intensity is irrelevant to that question. Conclusion: Source Y is the more biologically dangerous despite emitting less total power.
Examiner commentary: Full marks. The discriminator moves: (i) explicit recognition that single-photon energy, not total power, controls the photochemistry; (ii) explicit naming of a threshold concept that prefigures the photoelectric work function; (iii) the "billion red photons just heat it" illustration which makes the abstract concept concrete; (iv) connection to the upcoming Einstein equation. Top-band answers don't just compute — they reason about which physical quantity does the work and why intensity is the wrong frame.
Pedagogical observations from teaching the photon model, with no fabricated examiner-report percentages.
The photon concept is the conceptual seam between classical electromagnetism (Maxwell) and modern quantum electrodynamics (QED). Three substantial follow-on topics show how the simple E=hf formula opens onto far deeper physics.
Compton scattering (1923). When a high-energy X-ray photon scatters off a free electron, the wavelength of the scattered photon is longer than the incident wavelength — and the wavelength shift depends only on the scattering angle, not on the incident wavelength:
Δλ=λ′−λ=mech(1−cosθ)
The combination h/(mec)≈2.43×10−12 m is the Compton wavelength of the electron. Compton's experiment was, alongside the photoelectric effect, the second decisive demonstration that photons carry momentum p=h/λ and behave as particles in collisions. He won the 1927 Nobel Prize.
Blackbody radiation and Planck's law. The full Planck spectrum is
B(λ,T)=λ52hc2exp(hc/(λkBT))−11
— the exponential factor in the denominator suppresses high-frequency modes and resolves the ultraviolet catastrophe. The h that first appears here is the same h that governs the photoelectric effect, atomic spectra and de Broglie waves: a single universal constant.
Second quantisation. In the deepest treatment (quantum electrodynamics), the electromagnetic field itself is a quantum field: every mode of the field is a harmonic oscillator whose excitations are photons. "Creating a photon" means raising one mode by one quantum of energy. This formalism, developed by Dirac, Feynman, Schwinger and Tomonaga, is the most accurately tested theory in physics — it agrees with experiment to better than one part in 1012 in the measurement of the electron's anomalous magnetic moment.
Oxbridge interview prompts that probe the photon model:
Recommended reading: QED: The Strange Theory of Light and Matter by Richard Feynman (the most accessible treatment of the photon as a quantum-field excitation); The Theoretical Minimum: Quantum Mechanics by Leonard Susskind; Quantum Theory by Bohm (the classical conceptual treatise).
Reference: OCR A-Level Physics A (H556) specification 4.5 — Quantum physics (refer to the official OCR H556 specification document for exact wording).