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Chapter 11: Dual Nature of Radiation and Matter

The early 20th century revealed that light, long thought of as a wave (Maxwell, Young), behaves as a stream of particles (photons) in the photoelectric effect. Conversely, electrons, supposedly classical particles, were found to diffract like waves (Davisson-Germer). This wave-particle duality is the hallmark of quantum mechanics.

Concept Map

  • Electron emission →\rightarrow thermionic / photoelectric / field / secondary.
  • Photoelectric effect →\rightarrow classical failures →\rightarrow Einstein's photon hypothesis →\rightarrow KEmax⁡=hν−ϕKE_{\max} = h\nu - \phi.
  • Photons →\rightarrow E=hνE = h\nu, p=h/λp = h/\lambda, rest mass zero.
  • Matter waves →\rightarrow de Broglie λ=h/p\lambda = h/p →\rightarrow electron through VV: λ=12.27/V\lambda = 12.27/\sqrt V Å.
  • Davisson-Germer →\rightarrow electron diffraction confirms duality.
  • Uncertainty principle →\rightarrow ΔxΔp≥ℏ/2\Delta x \Delta p \geq \hbar/2.

11.1 Electron Emission and Work Function

Definition

Electrons in a metal are held by the binding energy of the lattice. The work function ϕ\phi is the minimum energy required to free an electron from the surface. Typical values: Cs ∼2.14 eV\sim 2.14\,\text{eV}, Na ∼2.75\sim 2.75, Cu ∼4.65\sim 4.65, Pt ∼5.65\sim 5.65.

Four mechanisms supply this energy:

TypeSource of energyExample
ThermionicHeatFilament in a vacuum tube
PhotoelectricEM radiationPhotocell
Field (cold) emissionStrong external EE field (∼108\sim 10^8 V/m)Field-emission electron gun
SecondaryBombardment by fast electrons/ionsPhotomultiplier tube

Pitfalls

  • ϕ\phi is a property of the surface, not the bulk; oxide layers can change it.
  • "Work function in eV" is convenient; converting to joules requires the factor 1 eV=1.6×10−19 J1\,\text{eV} = 1.6 \times 10^{-19}\,\text{J}.

11.2 Photoelectric Effect — Observations

Discovery

Hertz (1887) noticed that UV light shining on a spark-gap electrode made discharges easier. Lenard (1900) showed that the ejected particles were negatively charged with the same e/me/m as cathode rays — they were electrons.

Setup

An evacuated tube contains a photosensitive cathode CC and a collector anode AA. Light of frequency ν\nu illuminates CC; emitted photoelectrons reach AA, giving a photocurrent II measured by a galvanometer. A variable voltage VV (with reversible polarity) accelerates or retards the electrons.

Pitfalls

  • Photocurrent is observed only above a threshold frequency — even very intense low-frequency light cannot eject any electron.
  • The effect is essentially instantaneous (<10−9 s< 10^{-9}\,\text{s}), contradicting wave-theory predictions of long lag times.

11.3 Effect of Intensity, Potential, Frequency

Photocurrent vs Anode Potential (fixed ν\nu, varying intensity)

Plot photocurrent II vs anode potential VV:

  • For positive VV, the photocurrent rises and saturates at a value IsatI_{\text{sat}} that depends on intensity.
  • Saturation Isat∝I_{\text{sat}} \propto intensity: more photons →\to more photoelectrons per second.
  • For negative VV (retarding), photocurrent falls. The minimum negative VV at which the photocurrent becomes zero is the stopping potential V0V_0 — and it is independent of intensity.

Stopping potential vs Frequency

For a given metal, varying ν\nu (at fixed intensity):

  • Below threshold ν0\nu_0: no current at any intensity.
  • Above ν0\nu_0: V0V_0 increases linearly with ν\nu. Slope =h/e= h/e (universal, independent of metal); intercept on the ν\nu-axis =ν0= \nu_0 (metal-dependent).

Graph summary

PlotResult
Photocurrent II vs VV at different intensities (fixed ν\nu)Same V0V_0; saturation ∝\propto intensity
Photocurrent II vs VV at different ν\nu (fixed intensity)Different V0V_0; same saturation
V0V_0 vs ν\nuStraight line, slope h/eh/e, intercept ν0\nu_0
IsatI_{\text{sat}} vs intensityStraight line through origin
KEmax⁡KE_{\max} vs ν\nuStraight line, slope hh, intercept −ϕ-\phi

Pitfalls

  • Stopping potential is independent of intensity but depends on frequency and metal.
  • Saturation current depends on intensity but not on VV once VV is large enough.

11.4 Threshold Frequency and Classical Wave-Theory Failures

Classical predictions (Maxwell)

  1. Higher intensity →\to larger EE field →\to more KE per electron.
  2. No threshold frequency: even low-ν\nu light should eventually eject electrons given enough time.
  3. Time lag: for weak intensity, light's energy must accumulate at an atom — measurable lag time of ∼\sim minutes/hours predicted.

Experimental facts

  1. KE of photoelectrons is independent of intensity. Higher intensity only increases the number of photoelectrons.
  2. Below threshold ν0\nu_0, no current is observed at any intensity.
  3. The effect is virtually instantaneous (<10−9 s< 10^{-9}\,\text{s}), even at very low intensity.

These three observations falsify the wave picture for the energy-transfer step.

Pitfalls

  • The wave model is fine for diffraction and interference; it fails specifically for single-photon-absorption energetics.

11.5 Einstein's Photoelectric Equation

Einstein's hypothesis (1905)

Light of frequency ν\nu is delivered in discrete packets — photons — each carrying energy

E=hν.E = h\nu.

When a photon is absorbed by an electron in the metal, the electron uses up to ϕ\phi of that energy to escape and keeps the rest as kinetic energy. Hence

  KEmax⁡=hν−ϕ  .\boxed{\;KE_{\max} = h\nu - \phi\;}.

If ν<ν0≡ϕ/h\nu < \nu_0 \equiv \phi/h, no electron has enough energy to escape — explains threshold.

Stopping potential

The most energetic electrons are stopped when eV0=KEmax⁡eV_0 = KE_{\max}:

eV0=hν−ϕ⇒V0=heν−ϕe.eV_0 = h\nu - \phi \quad\Rightarrow\quad V_0 = \frac{h}{e}\nu - \frac{\phi}{e}.

So V0V_0 vs ν\nu is linear with slope h/eh/e and xx-intercept ν0\nu_0.

Explanation of all observations

  • Intensity ∝\propto number of photons / sec ∝\propto number of ejected electrons / sec ∝Isat\propto I_{\text{sat}}. KE per electron unchanged.
  • Threshold ν0=ϕ/h\nu_0 = \phi/h arises naturally.
  • One photon ejects one electron in a single quantum event — explains instantaneous response.

Worked Example

Light of λ=400 nm\lambda = 400\,\text{nm} falls on Cs (ϕ=2.14 eV\phi = 2.14\,\text{eV}). Find V0V_0.

hν=hc/λ=(1240 eV nm)/400=3.1 eVh\nu = hc/\lambda = (1240\,\text{eV nm})/400 = 3.1\,\text{eV}. KEmax⁡=3.1−2.14=0.96 eVKE_{\max} = 3.1 - 2.14 = 0.96\,\text{eV}. V0=0.96 VV_0 = 0.96\,\text{V}.

Pitfalls

  • ϕ\phi is in joules or eV — match units with hνh\nu.
  • The "max⁡\max" in KEmax⁡KE_{\max} matters: most electrons emerge with less because they lose energy reaching the surface; only the surface-layer ones have KEmax⁡KE_{\max}.
  • eV0=KEmax⁡eV_0 = KE_{\max} is the only condition tested — applies to maximum KE, not average.

11.6 Photon — Properties

A photon, the quantum of the EM field, has

  • Energy E=hν=hc/λE = h\nu = hc/\lambda.
  • Momentum p=E/c=h/λp = E/c = h/\lambda.
  • Rest mass zero (always travels at cc).
  • Spin 11 (boson).
  • Particle-like in interactions (photoelectric effect, Compton scattering); wave-like in propagation (interference, diffraction).

Number of photons per second

A source of power PP at frequency ν\nu emits

N=Phνphotons / s.N = \frac{P}{h\nu}\quad\text{photons / s}.

Radiation pressure

A photon absorbed by a surface delivers momentum p=h/λp = h/\lambda. For light of intensity II on a perfectly absorbing surface:

Prad=Ic.P_{\text{rad}} = \frac{I}{c}.

For a perfectly reflecting surface: Prad=2I/cP_{\text{rad}} = 2I/c.

Worked Example

λ=500 nm\lambda = 500\,\text{nm}. Find EE and pp of a photon.

E=hc/λ=(6.63×10−34)(3×108)/(5×10−7)=3.98×10−19 J=2.48 eVE = hc/\lambda = (6.63\times 10^{-34})(3\times 10^8)/(5\times 10^{-7}) = 3.98\times 10^{-19}\,\text{J} = 2.48\,\text{eV}. p=h/λ=(6.63×10−34)/(5×10−7)=1.33×10−27 kg m/sp = h/\lambda = (6.63\times 10^{-34})/(5\times 10^{-7}) = 1.33\times 10^{-27}\,\text{kg m/s}.

Pitfalls

  • Photon mass m=0m = 0, but momentum p=h/λp = h/\lambda is nonzero — relativistically, E=pcE = pc requires m0=0m_0 = 0.
  • A photon's frequency is the same in any inertial frame's measurement of the same event count, but Doppler effect changes ν\nu between source and observer frames.

11.7 de Broglie Hypothesis

Hypothesis (1924)

If radiation has dual nature, so does matter. A particle of momentum pp is associated with a wave of wavelength

  λ=hp=hmv  .\boxed{\;\lambda = \frac{h}{p} = \frac{h}{mv}\;}.

For non-relativistic particles, p=mvp = mv; for relativistic, p=γmvp = \gamma m v.

For a particle of kinetic energy KK (non-relativistic): p=2mKp = \sqrt{2mK}, so

λ=h2mK.\lambda = \frac{h}{\sqrt{2mK}}.

Worked Example

A bullet of mass 10 g10\,\text{g} moves at 1000 m/s1000\,\text{m/s}. Find λ\lambda.

λ=(6.63×10−34)/(0.01⋅1000)=6.63×10−35 m\lambda = (6.63\times 10^{-34})/(0.01\cdot 1000) = 6.63\times 10^{-35}\,\text{m}. Far below any atomic scale, hence not observable as wave.

For an electron of K=1 eVK = 1\,\text{eV}: λ=h/2mK≈1.23 nm\lambda = h/\sqrt{2mK} \approx 1.23\,\text{nm}. Observable by diffraction in a crystal lattice.

Pitfalls

  • de Broglie's λ\lambda is meaningful only when λ\lambda is comparable to the system's relevant size (slit width, lattice spacing, atom size).
  • For macroscopic objects, λ\lambda is absurdly small — quantum effects negligible.

11.8 de Broglie Wavelength of an Electron in Potential VV

Derivation: λ=12.27/V\lambda = 12.27/\sqrt V Å

An electron accelerated through potential VV gains kinetic energy K=eVK = eV. Then

p=2meeV,λ=h2meeV.p = \sqrt{2 m_e e V}, \quad \lambda = \frac{h}{\sqrt{2 m_e e V}}.

Plug numbers: h=6.626×10−34h = 6.626\times 10^{-34} J s, me=9.11×10−31m_e = 9.11\times 10^{-31} kg, e=1.6×10−19e = 1.6\times 10^{-19} C:

λ=6.626×10−342⋅9.11×10−31⋅1.6×10−19⋅V.\lambda = \frac{6.626\times 10^{-34}}{\sqrt{2\cdot 9.11\times 10^{-31}\cdot 1.6\times 10^{-19}\cdot V}}.

The denominator =5.40×10−25V= 5.40\times 10^{-25}\sqrt V (SI), so λ=(1.227×10−9/V) m=(12.27/V)\lambda = (1.227\times 10^{-9}/\sqrt V)\,\text{m} = (12.27/\sqrt V) Å.

  λe=12.27V  A˚,V in volts  .\boxed{\;\lambda_e = \frac{12.27}{\sqrt V}\;\text{Å},\quad V\text{ in volts}\;}.

Worked Example

Electron accelerated through V=100 VV = 100\,\text{V}.

λ=12.27/10=1.227 A˚\lambda = 12.27/10 = 1.227\,\text{Å}. Comparable to atomic spacing; perfect for diffraction off a crystal.

Pitfalls

  • Use VV in volts, get λ\lambda in Å. For VV in kV, you must scale: λ=12.27/V(V)\lambda = 12.27/\sqrt{V(\text{V})} Å =0.388/V(kV)= 0.388/\sqrt{V(\text{kV})} Å.
  • For electron V≳100 kVV \gtrsim 100\,\text{kV}, relativistic correction is needed.

11.9 Davisson-Germer Experiment

Setup

A heated tungsten filament emits electrons, which are accelerated by a variable potential VV and directed normally onto a polished single crystal of nickel. A movable Faraday-cup detector measures the intensity of scattered electrons as a function of scattering angle ϕ\phi at fixed VV.

Observation

For V=54 VV = 54\,\text{V}, a sharp maximum in scattered intensity is found at ϕ=50∘\phi = 50^\circ — a "diffraction peak" from the nickel lattice.

Analysis

Treating the Ni atomic rows as a diffraction grating with spacing d=0.91 A˚d = 0.91\,\text{Å} (for Ni (111)(111) plane), Bragg-like condition gives wavelength of the scattering wave: λ=dsin⁡ϕ=0.91sin⁡50∘≈0.165 nm=1.65 A˚\lambda = d\sin\phi = 0.91\sin 50^\circ \approx 0.165\,\text{nm} = 1.65\,\text{Å} (using the appropriate plane and incidence). Cross-checking with de Broglie: λ=12.27/54=1.67 A˚\lambda = 12.27/\sqrt{54} = 1.67\,\text{Å}.

Conclusion

The measured wavelength matches the de Broglie wavelength of the electrons. Electrons therefore behave as waves; matter waves are real.

Pitfalls

  • The "peak angle" depends on VV; varying VV shifts the peak in agreement with λ∝1/V\lambda \propto 1/\sqrt V.
  • This was an accidental discovery — Davisson and Germer were originally studying electron scattering from oxidised Ni; an accident annealed the Ni into a single crystal.

11.10 Heisenberg Uncertainty Principle (Qualitative)

Statement

For any quantum particle, one cannot simultaneously know position xx and momentum pxp_x with arbitrary precision:

Δx Δpx≥ℏ2,ℏ=h2π.\Delta x\,\Delta p_x \geq \frac{\hbar}{2}, \quad \hbar = \frac{h}{2\pi}.

Analogous: ΔE Δt≥ℏ/2\Delta E\,\Delta t \geq \hbar/2.

Intuition from de Broglie

If a particle is localised in space within Δx\Delta x, it must be built from a wave packet — a superposition of many de Broglie waves with momentum spread Δp∼h/Δx\Delta p \sim h/\Delta x.

Implications

  • The classical orbit of an electron in an atom has no well-defined trajectory.
  • Zero-point energy: a confined particle (in a box of size LL) has minimum KE ∼ℏ2/(2mL2)\sim \hbar^2/(2mL^2).
  • Cannot "see" an electron with light shorter than its size without imparting huge momentum to it.

Worked Example

An electron is confined to an atom of size Δx=1 A˚\Delta x = 1\,\text{Å}. Estimate Δp\Delta p and corresponding KE.

Δp≥ℏ/(2Δx)=(1.05×10−34)/(2⋅10−10)=5.3×10−25 kg m/s\Delta p \geq \hbar/(2\Delta x) = (1.05\times 10^{-34})/(2\cdot 10^{-10}) = 5.3\times 10^{-25}\,\text{kg m/s}.

KE∼(Δp)2/(2me)=(5.3×10−25)2/(2⋅9.11×10−31)≈1.5×10−19 J≈1 eVKE \sim (\Delta p)^2/(2m_e) = (5.3\times 10^{-25})^2/(2\cdot 9.11\times 10^{-31}) \approx 1.5\times 10^{-19}\,\text{J} \approx 1\,\text{eV} — sensible atomic scale.

Pitfalls

  • Δx\Delta x and Δp\Delta p are standard deviations, not measurement errors.
  • The uncertainty principle is not about disturbing the system in measurement; it is an intrinsic feature of the quantum state.

Solved Problems

1. Light of λ=200 nm\lambda = 200\,\text{nm} hits a metal of ϕ=4.0 eV\phi = 4.0\,\text{eV}. Find V0V_0.

hν=1240/200=6.2 eVh\nu = 1240/200 = 6.2\,\text{eV}. V0=(6.2−4.0)=2.2 VV_0 = (6.2 - 4.0) = 2.2\,\text{V}.

2. A metal has threshold λ0=600 nm\lambda_0 = 600\,\text{nm}. Find ϕ\phi.

ϕ=hc/λ0=1240/600=2.07 eV\phi = hc/\lambda_0 = 1240/600 = 2.07\,\text{eV}.

3. Slope of V0V_0 vs ν\nu is found to be 4.12×10−15 V s4.12\times 10^{-15}\,\text{V s}. Find hh.

h=e⋅slope=(1.6×10−19)(4.12×10−15)=6.59×10−34 J sh = e\cdot\text{slope} = (1.6\times 10^{-19})(4.12\times 10^{-15}) = 6.59\times 10^{-34}\,\text{J s}. (Standard h=6.626×10−34 J sh = 6.626\times 10^{-34}\,\text{J s}.)

4. Power 5 mW5\,\text{mW} laser at λ=633 nm\lambda = 633\,\text{nm}. Photon rate?

Ephoton=1240/633=1.96 eV=3.14×10−19 JE_{\text{photon}} = 1240/633 = 1.96\,\text{eV} = 3.14\times 10^{-19}\,\text{J}. N=P/E=5×10−3/3.14×10−19≈1.6×1016N = P/E = 5\times 10^{-3}/3.14\times 10^{-19} \approx 1.6\times 10^{16} photons/s.

5. A 1 eV1\,\text{eV} electron's de Broglie wavelength?

λ=12.27/1=12.27 A˚\lambda = 12.27/\sqrt 1 = 12.27\,\text{Å}.

6. Find the ratio λe/λp\lambda_{\text{e}}/\lambda_{\text{p}} for an electron and a proton of equal KE.

λ∝1/m\lambda \propto 1/\sqrt m at equal KK, so λe/λp=mp/me=1836≈42.85\lambda_e/\lambda_p = \sqrt{m_p/m_e} = \sqrt{1836} \approx 42.85.

7. A particle of Δx=10−10 m\Delta x = 10^{-10}\,\text{m}. Minimum Δv\Delta v of an electron in it?

Δv=ℏ/(2meΔx)=(1.05×10−34)/(2⋅9.11×10−31⋅10−10)≈5.8×105 m/s\Delta v = \hbar/(2 m_e \Delta x) = (1.05\times 10^{-34})/(2\cdot 9.11\times 10^{-31}\cdot 10^{-10}) \approx 5.8\times 10^5\,\text{m/s}.

JEE/NEET Edge Cases

  • A common trap: "doubling intensity doubles V0V_0" — false. V0V_0 depends only on ν\nu and ϕ\phi.
  • Threshold wavelength λ0\lambda_0 and frequency ν0\nu_0: λ0ν0=c\lambda_0\nu_0 = c; ϕ=hν0=hc/λ0\phi = h\nu_0 = hc/\lambda_0.
  • For a photon, p=h/λ=E/cp = h/\lambda = E/c; for matter, p=h/λp = h/\lambda but E≠pcE \neq pc (because matter has rest mass).
  • For equal momenta λe=λp\lambda_e = \lambda_p; for equal KE λ∝1/m\lambda \propto 1/\sqrt m; for equal velocity λ∝1/m\lambda \propto 1/m.
  • de Broglie wavelength of a neutron in a thermal reactor (K≈0.025 eVK \approx 0.025\,\text{eV}): λ≈1.8 A˚\lambda \approx 1.8\,\text{Å} — perfect for crystallography.
  • The V0V_0-vs-ν\nu line is the same slope for all metals (it's h/eh/e, universal); only the threshold ν0\nu_0 depends on the metal.
  • Saturating current ∝\propto intensity for fixed ν\nu. Reducing intensity to almost zero still gives instantaneous photoelectrons above threshold — one photon, one electron.
  • Davisson-Germer specifically supports the wave nature of electrons; G P Thomson's transmission diffraction through gold foil is its other classic confirmation.

Quick Recap

  • Work function ϕ\phi: minimum energy to free an electron. ν0=ϕ/h\nu_0 = \phi/h.
  • Einstein: KEmax⁡=hν−ϕKE_{\max} = h\nu - \phi; eV0=hν−ϕeV_0 = h\nu - \phi.
  • V0V_0 vs ν\nu linear, slope h/eh/e.
  • Photon: E=hνE = h\nu, p=h/λp = h/\lambda, m0=0m_0 = 0.
  • de Broglie: λ=h/p=h/2mK\lambda = h/p = h/\sqrt{2mK}. Electron: λ=12.27/V\lambda = 12.27/\sqrt V Å.
  • Davisson-Germer: 54 V54\,\text{V} electron diffracts off Ni at 50∘50^\circ, λ≈1.65 A˚\lambda \approx 1.65\,\text{Å}.
  • Heisenberg: ΔxΔp≥ℏ/2\Delta x \Delta p \geq \hbar/2.

Formula Sheet

QuantityFormula
Photon energyE=hν=hc/λE = h\nu = hc/\lambda
Photon momentump=h/λ=E/cp = h/\lambda = E/c
Threshold frequencyν0=ϕ/h\nu_0 = \phi/h
Threshold wavelengthλ0=hc/ϕ\lambda_0 = hc/\phi
Einstein equationKEmax⁡=hν−ϕKE_{\max} = h\nu - \phi
Stopping potentialeV0=hν−ϕeV_0 = h\nu - \phi
Slope of V0V_0 vs ν\nuh/e≈4.14×10−15 V sh/e \approx 4.14\times 10^{-15}\,\text{V s}
Photon rate from power PPN=P/hνN = P/h\nu
Radiation pressure (absorb)I/cI/c
Radiation pressure (reflect)2I/c2I/c
de Broglie wavelengthλ=h/p\lambda = h/p
de Broglie from KEλ=h/2mK\lambda = h/\sqrt{2mK}
Electron through VVλ=12.27/V\lambda = 12.27/\sqrt V Å
Davisson-Germerλ=dsin⁡ϕ\lambda = d\sin\phi (Bragg-like)
Uncertainty (position-momentum)ΔxΔp≥ℏ/2\Delta x \Delta p \geq \hbar/2
Uncertainty (energy-time)ΔEΔt≥ℏ/2\Delta E \Delta t \geq \hbar/2
Useful constantshc≈1240 eV nmhc \approx 1240\,\text{eV nm}, ℏ=1.055×10−34 J s\hbar = 1.055\times 10^{-34}\,\text{J s}

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