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photoelectric laws and Einstein equation

Learning objectives

  • Outcome

    Write and apply the Einstein equation hν=Aout+Kmax⁡h\nu = A_{\text{out}} + K_{\max} to compute Kmax⁡K_{\max}, AoutA_{\text{out}}, or the frequency ν\nu.

  • Outcome

    Compute the stopping voltage UsU_{s} from eUs=Kmax⁡eU_{s}=K_{\max} and find the red threshold ν0=Aout/h\nu_0=A_{\text{out}}/h.

  • Outcome

    Explain the three laws of the photoelectric effect using the photon model: saturation current proportional to intensity, existence of a red threshold, and instantaneous emission.

  • Outcome

    Extract Planck's constant hh (from the slope h/eh/e) and the work function (from the axis intercept) from a graph of UsU_{s} against ν\nu.

Understand the idea

Laws of the photoelectric effect and Einstein equation

Text

Laws of the photoelectric effect (Stoletov): 1) at fixed frequency the saturation photocurrent is proportional to the light intensity; 2) every substance has a red threshold ν0\nu_0 — for ν<ν0\nu<\nu_0 there is no emission, however high the intensity; 3) emission begins almost instantaneously (t≈10−9t\approx10^{-9} s).

Wave theory cannot explain the second and third laws, whereas the photon model explains all three: light is a stream of photons of energy hνh\nu, and one photon interacts with one electron (photon energy and momentum: E=hνE=h\nu, p=h/λ=hν/cp=h/\lambda=h\nu/c). Energy conservation yields the Einstein equation

hν=Aout+Kmax⁡,h\nu = A_{\text{out}} + K_{\max},

where AoutA_{\text{out}} is the work function and Kmax⁡K_{\max} the maximum kinetic energy of an emitted electron. The stopping voltage UsU_{s} at which the current vanishes measures that energy: Kmax⁡=eUsK_{\max}=eU_{s}, hence

Us=heν−Aoute.U_{s} = \frac{h}{e}\nu - \frac{A_{\text{out}}}{e}.

The graph of UsU_{s} against ν\nu is a straight line of slope h/eh/e, meeting the frequency axis at ν0=Aout/h\nu_0=A_{\text{out}}/h.

Worked examples

Direct

Problem

A metal with work function Aout=2.2 eVA_{\text{out}}=2.2\ \text{eV} is illuminated by light of wavelength λ=400 nm\lambda=400\ \text{nm}. Find the maximum kinetic energy of the photoelectrons and the stopping voltage.

Solution

Use the convenient constant hc=1240 eV⋅nmhc=1240\ \text{eV}\cdot\text{nm}.

Photon energy:

E=hcλ=1240400=3.10 eV.E=\frac{hc}{\lambda}=\frac{1240}{400}=3.10\ \text{eV}.

Einstein equation:

Kmax⁡=E−Aout=3.10−2.2=0.90 eV=1.44×10−19 J.K_{\max}=E-A_{\text{out}}=3.10-2.2=0.90\ \text{eV}=1.44\times10^{-19}\ \text{J}.

Stopping voltage follows from Kmax⁡=eUsK_{\max}=eU_{s}:

Us=Kmax⁡e=0.90 eVe=0.90 V.U_{s}=\frac{K_{\max}}{e}=\frac{0.90\ \text{eV}}{e}=0.90\ \text{V}.

Answer: Kmax⁡=0.90 eVK_{\max}=0.90\ \text{eV}, Us=0.90 VU_{s}=0.90\ \text{V}.

Application

Problem

The red threshold of a metal is λ0=600 nm\lambda_0=600\ \text{nm}. The metal is illuminated with light of λ=400 nm\lambda=400\ \text{nm}. Find the work function, the stopping voltage, and the maximum speed of the photoelectrons (me=9.11×10−31 kgm_e=9.11\times10^{-31}\ \text{kg}).

Solution

Work function corresponds to the red threshold (Kmax⁡=0K_{\max}=0):

Aout=hcλ0=1240600=2.07 eV.A_{\text{out}}=\frac{hc}{\lambda_0}=\frac{1240}{600}=2.07\ \text{eV}.

Photon energy: E=1240/400=3.10 eVE=1240/400=3.10\ \text{eV}.

Einstein equation:

Kmax⁡=E−Aout=3.10−2.07=1.03 eV=1.65×10−19 J.K_{\max}=E-A_{\text{out}}=3.10-2.07=1.03\ \text{eV}=1.65\times10^{-19}\ \text{J}.

Stopping voltage: Us=Kmax⁡/e=1.03 VU_{s}=K_{\max}/e=1.03\ \text{V}.

Maximum speed:

vmax⁡=2Kmax⁡me=2⋅1.65×10−199.11×10−31≈6.0×105 m/s.v_{\max}=\sqrt{\frac{2K_{\max}}{m_e}}=\sqrt{\frac{2\cdot1.65\times10^{-19}}{9.11\times10^{-31}}}\approx6.0\times10^{5}\ \text{m/s}.

Answer: Aout=2.07 eVA_{\text{out}}=2.07\ \text{eV}, Us=1.03 VU_{s}=1.03\ \text{V}, vmax⁡≈6.0×105 m/sv_{\max}\approx6.0\times10^{5}\ \text{m/s}.

Transfer

Problem

A laser of power P=2.0 mWP=2.0\ \text{mW} sends light of λ=500 nm\lambda=500\ \text{nm} onto a cathode with work function Aout=1.5 eVA_{\text{out}}=1.5\ \text{eV}. (a) How many photons hit the cathode per second? (b) How do the saturation current and the stopping voltage change if the laser power is doubled at the same wavelength?

Solution

(a) Energy of one photon:

E=hcλ=1240500=2.48 eV=3.97×10−19 J.E=\frac{hc}{\lambda}=\frac{1240}{500}=2.48\ \text{eV}=3.97\times10^{-19}\ \text{J}.

Power is energy per second, so the number of photons per second is

N=PE=2.0×10−33.97×10−19≈5.0×1015 s−1.N=\frac{P}{E}=\frac{2.0\times10^{-3}}{3.97\times10^{-19}}\approx5.0\times10^{15}\ \text{s}^{-1}.

(b) Doubling the power doubles the photon flux and hence the number of ejected electrons: the saturation current doubles (first law of the photoelectric effect). The energy of each photon is unchanged, so

K_{\max}=E-A_{\text{out}}=2.48-1.5=0.98\ \text{eV},\qquad U_{s}=0.98\ \text{V}$$ — the stopping voltage stays the same. Note: for $\lambda>1240/1.5\approx827\ \text{nm}$ there is no current at all, however large the power.

Practice

Text

A simulation instead of a hazardous experiment. Do not use real ultraviolet lamps: work in the PhET "Photoelectric Effect" simulation (or an equivalent one).

  1. Choose a metal (for example, sodium) and record its work function.
  2. Set the wavelength λ=400 nm\lambda=400\ \text{nm} and a moderate intensity. Slowly increase the stopping voltage until the photocurrent becomes zero; record UsU_{s}.
  3. Repeat for 5–6 wavelengths (for example, 350, 400, 450, 500, 550, 600 nm).
  4. Plot UsU_{s} against ν=c/λ\nu=c/\lambda and draw a straight line. The slope gives h/eh/e — estimate hh; the intercept with the ν\nu axis gives the red threshold ν0\nu_0.
  5. Changing only the intensity, check that the saturation current grows in proportion to intensity while UsU_{s} stays the same.
  6. Lower the frequency below ν0\nu_0 and check that the current is zero at any intensity.

Visual reference

Purpose

Show that the stopping voltage depends linearly on frequency, and link the slope and the intercept of the line to Planck's constant and the work function.

Representation

Graph: frequency ν\nu on the horizontal axis, stopping voltage UsU_{s} on the vertical axis. The experimental points fall on a straight line Us=heν−Aoute.U_{s}=\frac{h}{e}\nu-\frac{A_{\text{out}}}{e}. The graph marks the slope h/eh/e, the intercept with the frequency axis ν0=Aout/h\nu_0=A_{\text{out}}/h (the red threshold), and the negative intercept on the UsU_{s} axis equal to −Aout/e-A_{\text{out}}/e. For different metals the lines are parallel and shifted vertically by the difference of their work functions divided by ee.

Real-world examples

Photogate on a running track

Scenario

At a school 100 m race, a blue light beam with wavelength λ=450 nm\lambda = 450\ \text{nm} falls on a cesium photocathode with work function W=2.14 eVW = 2.14\ \text{eV}. The light flux produces a photocurrent; when a runner blocks the beam, the current drops and the timer records the time. The maximum kinetic energy of emitted electrons is Ekmax⁡=hν−W=hcλ−W≈2.76−2.14=0.62 eVE_{k\max}=h\nu - W=\frac{hc}{\lambda}-W \approx 2.76-2.14=0.62\ \text{eV}, and the stopping voltage is Us=Ekmax⁡/e≈0.62 VU_s=E_{k\max}/e \approx 0.62\ \text{V}.

Connection

The scenario exercises the first photoelectric law: the photocurrent is proportional to the number of photons per second, that is, to light intensity. Einstein's equation hν=W+Ekmax⁡h\nu = W + E_{k\max} shows that the maximum kinetic energy and stopping voltage are set by light frequency and work function, not by beam brightness.

Ambient light sensor in a smartphone

Scenario

A smartphone screen automatically changes brightness from the signal of a silicon photodiode. Green light from a window has λ=550 nm\lambda = 550\ \text{nm}, so the photon energy is E=1240550≈2.25 eVE=\frac{1240}{550}\approx 2.25\ \text{eV}. For silicon the threshold energy is about W=1.12 eVW=1.12\ \text{eV}, so the maximum photoelectron energy is Ekmax⁡≈1.13 eVE_{k\max}\approx 1.13\ \text{eV}, and the red threshold is λmax⁡=hcW≈1107 nm\lambda_{\max}=\frac{hc}{W}\approx 1107\ \text{nm}. If the window brightness doubles, the photocurrent doubles, but Ekmax⁡E_{k\max} does not change.

Connection

The scenario tests the photoelectric red threshold and the independence of Ekmax⁡E_{k\max} from intensity. If the wavelength exceeds λmax⁡\lambda_{\max}, a single photon cannot eject an electron, so the sensor does not respond. Einstein's equation gives Ekmax⁡=hν−WE_{k\max}=h\nu-W for each absorbed photon.

Automatic kitchen faucet

Scenario

A kitchen faucet turns on when a hand reflects an infrared beam with λ=940 nm\lambda=940\ \text{nm} back to a photodetector. The photon energy is E=1240940≈1.32 eVE=\frac{1240}{940}\approx 1.32\ \text{eV}. For a silicon detector with W=1.12 eVW=1.12\ \text{eV}, the maximum kinetic energy is Ekmax⁡=1.32−1.12=0.20 eVE_{k\max}=1.32-1.12=0.20\ \text{eV}, and the stopping voltage is Us=0.20 VU_s=0.20\ \text{V}. Brighter infrared light only increases the number of electrons, not their maximum energy.

Connection

The scenario shows the instantaneous nature of the photoelectric effect: current appears immediately upon illumination, and its magnitude is proportional to intensity. The threshold frequency νmin⁡=W/h\nu_{\min}=W/h explains why the detector is chosen for a particular wavelength, while Einstein's equation links photon energy to work function and electron kinetic energy.