22. Quantum physics A2

Syllabus
9702–2028–2029
Section
22
Level
A2

22.1 Energy and momentum of a photon

Syllabus
9702–2028–2029
Topic
22.1
Level
A2

Electromagnetic radiation behaves as both a wave and a stream of particles

Electromagnetic radiation shows wave behaviour such as interference and diffraction and particle behaviour such as quantised photon interactions.

Use the model that explains the observation; neither classical wave nor classical particle language alone covers every experiment.

A diffraction pattern supports wave behaviour, while the photoelectric effect requires discrete energy transfers.

Wave–particle duality is not a claim that light alternates between two physical substances during travel.

A photon is a quantum packet of electromagnetic energy

A photon is a discrete packet of electromagnetic energy with energy proportional to frequency and zero rest mass.

Photons travel at c in vacuum and are absorbed or emitted as whole quanta in interactions.

A higher-frequency ultraviolet photon carries more energy than a visible red photon.

A photon is not a tiny classical wave crest, and increasing intensity increases photon number at fixed frequency rather than each photon’s energy.

Calculate photon energy, wavelength and photon rate with E=hf

one−photonenergyE=hf=hc/λ,withh=6.63×10−34Jsandc=3.00×108ms−1one-photon energy E=hf=hc/λ, with h=6.63×10⁻³⁴ J s and c=3.00×10⁸ m s⁻¹

For λ=630 nm, E=hc/λ=(6.63×10⁻³⁴)(3.00×10⁸)/(630×10⁻⁹)=3.16×10⁻¹⁹ J=1.97 eV.

For photon energy 74 keV, first convert E=74×10³×1.60×10⁻¹⁹ J, then λ=hc/E=1.68×10⁻¹¹ m.

beampowerP=(numberofphotonspersecond)×Ephotonphotonrate=P/Ephotonbeam power P=(number of photons per second)×E_photon photon rate=P/E_photon

A 1.0×10⁻² W beam of 1.97 eV photons emits (1.0×10⁻²)/(1.97×1.60×10⁻¹⁹)=3.2×10¹⁶ photons s⁻¹.

E=hf is energy per photon. Higher f means larger E; larger λ means smaller E. Convert nm to m and eV to J before using SI constants.

An electronvolt is the energy gained by one elementary charge through one volt

One electronvolt is 1 eV=1.60×10⁻¹⁹ J, the energy transfer when a charge of magnitude e moves through 1 V.

Use eV for particle-scale energies and convert to joules when applying SI equations or comparing macroscopic work.

A 5.0 eV electron has energy about 8.0×10⁻¹⁹ J.

An electronvolt is an energy unit, not a voltage or an electron’s mass.

Photon momentum p=E/c transfers force when light is absorbed or reflected

photonmomentummagnitudep=E/c=hf/c=h/λphoton momentum magnitude p=E/c=hf/c=h/λ

A photon has zero rest mass but non-zero momentum directed along its propagation. Shorter wavelength or higher energy means greater momentum.

For E=3.11×10⁻¹⁹ J, p=E/c=(3.11×10⁻¹⁹)/(3.00×10⁸)=1.04×10⁻²⁷ kg m s⁻¹ (or N s).

Normal interaction at a stationary surface Photon momentum change magnitude Momentum delivered to surface
photon absorbed p p
photon reflected straight back 2p 2p

averageforce=momentumtransferredperunittimeForcompleteabsorptionofbeampowerP:F=P/c;forperfectreflection:F=2P/c.average force = momentum transferred per unit time For complete absorption of beam power P: F=P/c; for perfect reflection: F=2P/c.

Do not use p=mv for a photon. Reflection transfers twice the normal momentum of absorption because the photon momentum reverses, rather than merely falling to zero.

22.2 Photoelectric effect

Syllabus
9702–2028–2029
Topic
22.2
Level
A2

Photoelectrons can be emitted when light of sufficient frequency illuminates a metal

The photoelectric effect is emission of electrons from a metal when incident photons have enough energy to overcome the surface work function.

Increasing intensity above threshold increases the number of emitted electrons, while frequency controls each photon’s energy and maximum electron speed.

Dim ultraviolet light can eject electrons while bright red light may not if red photon energy is below threshold.

Photoemission is not caused by accumulating energy over time from sub-threshold photons in the simple model.

Threshold frequency is the minimum frequency for photoemission, with an equivalent threshold wavelength

Threshold frequency f₀ is the minimum photon frequency that ejects electrons; threshold wavelength λ₀ is the maximum wavelength, related by c=f₀λ₀.

Below f₀ or above λ₀ no electrons are emitted regardless of intensity in the ideal model.

A metal with threshold frequency 6.0×10¹⁴ Hz has threshold wavelength about 500 nm.

Threshold frequency is not the frequency of emitted electrons, and higher intensity cannot compensate for lower photon frequency.

Photoelectric emission compares photon energy with the metal work function

A photon ejects an electron if hf≥Φ, where Φ is the work function; any excess becomes the electron’s kinetic energy.

Use Φ as the minimum energy needed to escape the surface and connect it to threshold frequency via Φ=hf₀.

Increasing frequency above threshold increases maximum photoelectron kinetic energy by the excess photon energy.

Work function is not the same as binding energy of every electron in the bulk and does not depend on beam intensity in this model.

Use hf=Φ+Kmax for speed, stopping potential and graphs

hf=Φ+Kmax=Φ+½mevmax2=Φ+eVshf=Φ+K_max=Φ+½m_ev_max²=Φ+eV_s

One photon supplies hf. The maximum-energy electrons spend Φ escaping and keep the remainder Kmax; a stopping potential Vs removes that maximum kinetic energy because Kmax=eVs.

For f=1.10×10¹⁵ Hz and Φ=5.80×10⁻¹⁹ J: Kmax=hf−Φ=1.49×10⁻¹⁹ J, so vmax=√(2Kmax/me)=5.72×10⁵ m s⁻¹ and Vs=Kmax/e=0.933 V.

Kmax=hf−ΦKmaxagainstf:gradienth;f−axisinterceptf0=Φ/h;extrapolatedK−axisintercept−ΦK_max=hf−Φ K_max against f: gradient h; f-axis intercept f₀=Φ/h; extrapolated K-axis intercept −Φ

Different metals give parallel Kmax–f lines because h is universal. A larger work function shifts the threshold to a larger frequency and the extrapolated intercept to a more negative value.

Use maximum—not average—kinetic energy. If Φ is in eV, either keep the whole energy calculation in eV or convert consistently; do not write Kmax=Vs without the charge factor when using joules.

Maximum photoelectron kinetic energy depends on frequency, not light intensity

For photoelectrons, the maximum kinetic energy is set by the energy of one incident photon: K_max=hf−Φ.

At a fixed frequency above threshold, raising intensity sends more photons per second, so the photocurrent can rise, but each photon still supplies the same energy and K_max is unchanged.

Doubling the intensity of ultraviolet light doubles the possible emission rate in an ideal experiment, not the stopping potential.

Intensity is not a substitute for frequency: sub-threshold photons do not eject electrons simply because the beam is brighter.

22.3 Wave–particle duality

Syllabus
9702–2028–2029
Topic
22.3
Level
A2

Wave-particle duality: choose the light model that explains the observation

Wave-particle duality means electromagnetic radiation shows wave-like behavior in some observations and particle-like behavior in others; neither classical picture alone explains all evidence.

Photoelectric effect → particulate evidence: energy arrives in photons E=hf. A threshold frequency, immediate emission and Kmax depending on frequency rather than intensity follow from one-electron/one-photon transfer.

Interference and diffraction → wave evidence: overlapping alternatives produce stable maxima and minima through constructive and destructive superposition.

Dim radiation above threshold can eject electrons immediately, while bright sub-threshold radiation cannot; yet the same electromagnetic radiation can form interference fringes or diffract through an aperture.

Duality is not light physically switching between two substances. It is an evidence-based rule about which model predicts the measured outcome.

Electron diffraction gives evidence for electron wave behaviour

When electrons pass through a thin crystal or narrow spacing, they can form diffraction patterns rather than only particle-like spots.

The pattern is explained by a wavelength associated with the moving electrons; changing electron momentum changes the spacing of maxima and minima.

A ring pattern from a polycrystalline film is evidence of constructive interference from many crystal orientations.

Diffraction does not say an electron is a classical water wave; it reveals wave-like interference in the probability description.

The de Broglie wavelength is the wavelength associated with a moving particle

A particle with momentum p has de Broglie wavelength λ=h/p, so greater momentum means a shorter wavelength.

For a non-relativistic electron p=mv; use the momentum actually delivered by the apparatus, not simply the particle’s rest mass.

Accelerating an electron through a larger potential difference increases its speed and reduces λ, changing the diffraction scale.

The wavelength is not a path the particle visibly traces; it predicts the scale of interference and diffraction effects.

The de Broglie relation can be used quantitatively as λ=h/p

Use λ=h/p with h=6.63×10⁻³⁴ J s and momentum p in kg m s⁻¹.

If speed is known and v is far below c, calculate p=mv first; keep units consistent before comparing λ with a slit or lattice spacing.

For a 9.11×10⁻³¹ kg electron moving at 2.0×10⁶ m s⁻¹, λ is about 0.36 nm, comparable with atomic spacings.

Do not substitute kinetic energy directly for p unless you first use the appropriate relation; rounding p too early can distort λ.

22.4 Energy levels in atoms and line spectra

Syllabus
9702–2028–2029
Topic
22.4
Level
A2

Electrons in isolated atoms occupy discrete energy levels

An isolated atom allows electrons only in particular energy states, not every energy between them.

An electron changes level by absorbing or emitting a photon whose energy equals the gap: ΔE=hf. Larger gaps correspond to higher-frequency, shorter-wavelength lines.

A hydrogen emission spectrum contains separate lines because only certain transitions are allowed between its levels.

The electron does not radiate continuously while remaining in a stationary level; emission occurs during a transition between allowed states.

Emission gives bright lines; absorption removes matching wavelengths

Emission spectrum: excited atoms in a hot, low-pressure gas make downward electron transitions and emit photons. Against a dark background, only the allowed photon wavelengths appear as separate bright lines.

Absorption spectrum: continuous light passes through a cooler, low-pressure gas. Electrons absorb only photons whose energies match upward level gaps, so those wavelengths appear as dark lines in the transmitted continuous spectrum.

Excited electrons later fall and re-emit photons, but in random directions. Along the original viewing direction, fewer photons remain at the absorbed wavelengths, so the dark lines persist.

For the same element, absorption and emission lines occur at the same characteristic wavelengths because both use the same energy-level gaps.

Each line has one frequency f and photon energy hf. Discrete line frequencies therefore imply discrete photon energies, discrete energy gaps and hence discrete atomic electron levels.

A line spectrum is not a continuous rainbow with uneven brightness: only specific transitions are possible, and absorption does not permanently destroy the photon energy.

A spectral photon carries the positive energy gap between two levels

Ephoton=hf=hc/λ=∣Eupper−Elower∣E_photon=hf=hc/λ=|E_upper−E_lower|

Downward transition: one photon is emitted. Upward transition: one matching photon is absorbed. In both cases photon energy is the positive magnitude of the level difference.

For hydrogen E3=−1.51 eV and E2=−3.40 eV, the n=3→2 gap is (−1.51)−(−3.40)=1.89 eV=3.02×10⁻¹⁹ J.

Then f=ΔE/h=(3.02×10⁻¹⁹)/(6.63×10⁻³⁴)=4.56×10¹⁴ Hz and λ=c/f=6.58×10⁻⁷ m=658 nm.

To find an unknown upper level from an emitted photon, use Eupper=Elower+hf. Keep signed level energies until after the subtraction.

Do not use the energy of either level alone as the photon energy. Convert 1 eV=1.60×10⁻¹⁹ J before using h in J s, and choose the transition direction from the wording or arrow.