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The Photoelectric Equation (HL) (HL IB Physics)

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The Photoelectric Equation

  • The energy possessed by a photon is equal to

E space equals space h f

  • The fraction of the energy transferred to the electron to release it from the metal is equal to the work function capital phi
  • The remaining amount is given as kinetic energy to the emitted photoelectron

E subscript K space m a x end subscript space equals 1 half m subscript e v subscript m a x end subscript squared

  • Since energy is always conserved, the energy of a photon incident on the surface of a metal is equal to:

The work function + the maximum kinetic energy of the photoelectron

  • This equation is known as the photoelectric equation:

E space equals space h f space equals space capital phi space plus space 1 half m subscript e v subscript m a x end subscript squared

  • Where:
    • h = Planck's constant (J s)
    • f = frequency of the incident radiation (Hz)
    • capital phi = work function of the metal (J) 
    • E subscript K space m a x end subscript = maximum kinetic energy of a photoelectron (J)
    • m subscript e = mass of an electron (kg)
    • v subscript m a x end subscript = maximum velocity of a photoelectron (m s−1)
  • This equation demonstrates:
    • If the incident photons do not have a high enough frequency and energy to overcome the work function (Φ), then no electrons will be emitted
    • When E space equals space h f subscript 0 space equals space capital phi, where f subscript 0 = threshold frequency, photoelectric emission only just occurs
    • The maximum kinetic energy E subscript K space m a x end subscript depends only on the frequency of the incident photon, and not the intensity of the radiation
    • The majority of photoelectrons will have kinetic energies less than E subscript K space m a x end subscript

Graphical Representation of Work Function

  • The photoelectric equation can be rearranged into the straight-line equation:

y space equals space m x space plus space c

  • Comparing this to the photoelectric equation:

E subscript K space m a x end subscript space equals space h f space minus space capital phi

  •  A graph of maximum kinetic energy E subscript K space m a x end subscript against frequency f can be obtained

  • The key elements of the graph are:
    • The work function Φ is the y-intercept
    • The threshold frequency f0 is the x-intercept
    • The gradient is equal to Planck's constant h
    • There are no electrons emitted below the threshold frequency f0

Kinetic Energy & Intensity

  • The kinetic energy of the photoelectrons is independent of the intensity of the incident radiation
    • This is because each electron can only absorb one photon
    • Kinetic energy is only dependent on the frequency of the incident radiation
  • Intensity is a measure of the number of photons incident on the surface of the metal
    • So, increasing the number of electrons striking the metal will not increase the kinetic energy of the electrons, it will increase the number of photoelectrons emitted

Why Kinetic Energy is a Maximum

  • Each electron in the metal acquires the same amount of energy from the photons in the incident monochromatic radiation.
  • However, the energy required to remove an electron from the metal varies because some electrons are on the surface whilst others are deeper in the metal
    • The photoelectrons with the maximum kinetic energy will be those on the surface of the metal since they do not require much energy to leave the metal
    • The photoelectrons with lower kinetic energy are those deeper within the metal since some of the energy absorbed from the photon is used to approach the metal surface (and overcome the work function)
    • There is less kinetic energy available for these photoelectrons once they have left the metal

Photoelectric Current

  • The photoelectric current is the number of photoelectrons emitted per second
  • Photoelectric current is proportional to the intensity of the radiation incident on the surface of the metal
  • This is because the intensity is proportional to the number of photons striking the metal per second
  • Since each photoelectron absorbs a single photon, the photoelectric current must be proportional to the intensity of the incident radiation

KE & Photocurrent Graphs, downloadable AS & A Level Physics revision notes

Graphs showing the variation of electron KE and photocurrent with the frequency of the incident light

Stopping Voltage

  • Stopping voltage V subscript S is defined as:

The voltage required to stop photoelectron emission from occurring

  • The photons arriving at the metal plate cause photoelectrons to be emitted
    • This is called the emitter plate
  • The electrons that cross the gap are collected at the other metal plate
    • This is called the collector plate

Stopping Potential, downloadable AS & A Level Physics revision notes

This setup can be used to determine the maximum kinetic energy of the emitted photoelectrons

  • The flow of electrons across the gap sets up an e.m.f. between the plates that allows a current to flow around the rest of the circuit
    • Effectively, it becomes a photoelectric cell which produces a photoelectric current
  • If the e.m.f. of the variable power supply is initially zero, the circuit operates only on the photoelectric current
  • As the supply is turned up, the emitter plate becomes more positive
    • This is because it is connected to the positive terminal of the supply
  • As a result, electrons leaving the emitter plate are attracted back towards it
    • This is because the p.d. across the tube opposes the motion of the electrons between the plates
  • If any electrons escape with high enough kinetic energy, they can overcome this attraction and cross to the collector plate
    • And if they don't have enough energy, they can't cross the gap
  • By increasing the e.m.f. of the supply, eventually, a p.d. will be reached at which no electrons will be able to cross the gap
    • This value of e.m.f. is equal to the stopping voltage V subscript S
  • At this point, the energy needed to cross the gap is equal to the maximum kinetic energy E subscript K space m a x end subscript of the electrons

E subscript K space m a x end subscript space equals space e V subscript S

  • Where:
    • E subscript K space m a x end subscript = maximum kinetic energy of the electrons (J)
    • e = elementary charge (C)
    • V subscript S = stopping voltage (V)

Worked example

The graph below shows how the maximum kinetic energy Ek of electrons emitted from the surface of sodium metal varies with the frequency f of the incident radiation.

5-2-2-work-function-graph-worked-example
Calculate the work function of sodium in eV.

Answer:

Step 1: Write out the photoelectric equation and rearrange it to fit the equation of a straight line

h f space equals space capital phi space plus space E subscript K space m a x end subscript

E subscript K space m a x end subscript space equals space h f space minus space capital phi

y space equals space m x space plus space c

  • Therefore, when E subscript K space equals space 0h f space equals space capital phi and f space equals space f subscript 0

 Step 2: Identify the threshold frequency from the x-axis of the graph

  • From the graph:
    • When E subscript K space equals space 0, threshold frequency:  f space equals space f subscript 0 = 4 × 1014 Hz

Step 3: Calculate the work function

capital phi space equals space h f subscript 0 space equals space open parentheses 6.63 cross times 10 to the power of negative 34 end exponent close parentheses space cross times space open parentheses 4 cross times 10 to the power of 14 close parentheses

Work function:  capital phi = 2.652 × 10−19 J

Step 4: Convert the work function into eV

  • To convert from J to eV:  divide by 1.6 × 10−19 J

E space equals space fraction numerator 2.652 space cross times space 10 to the power of negative 19 end exponent over denominator 1.6 space cross times space 10 to the power of negative 19 end exponent end fraction = 1.66 eV

Worked example

Monochromatic light of wavelength lambda subscript 1 is incident on the surface of a metal. The stopping voltage for this light is V subscript 1.

When another monochromatic light of wavelength lambda subscript 2 is incident on the same surface, the stopping voltage is V subscript 2.

What is the quantity fraction numerator open parentheses V subscript 2 space minus space V subscript 1 close parentheses over denominator open parentheses fraction numerator 1 space over denominator lambda subscript 2 end fraction space minus space fraction numerator 1 space over denominator lambda subscript 1 end fraction close parentheses end fraction equal to?

A.    fraction numerator h over denominator 2 straight pi end fraction                 B.    h over c                 C.    fraction numerator h c over denominator e end fraction                 D.    h over e



Answer:  C

  • The photoelectric equation for light 1 is

h f subscript 1 space equals space capital phi space plus thin space E subscript K space m a x open parentheses 1 close parentheses end subscript

Where E subscript K space m a x open parentheses 1 close parentheses end subscript space equals space e V subscript 1  and  E subscript 1 space equals space h f subscript 1 space equals fraction numerator h c over denominator lambda subscript 1 end fraction

  • The photoelectric equation for light 2 is

h f subscript 2 space equals space capital phi space plus thin space E subscript K space m a x open parentheses 2 close parentheses end subscript

Where E subscript K space m a x open parentheses 2 close parentheses end subscript space equals space e V subscript 2  and  E subscript 2 space equals space h f subscript 2 space equals fraction numerator h c over denominator lambda subscript 2 end fraction

  • Since the metal is the same, the work function capital phi is the same for both, so:

capital phi space equals fraction numerator h c space over denominator lambda subscript 1 end fraction minus space e V subscript 1 space equals space fraction numerator h c space over denominator lambda subscript 2 end fraction minus space e V subscript 2

  • Collecting the terms together and simplifying gives

e V subscript 2 space minus space e V subscript 1 space equals space fraction numerator h c space over denominator lambda subscript 2 end fraction space minus space fraction numerator h c space over denominator lambda subscript 1 end fraction

e open parentheses V subscript 2 space minus space V subscript 1 close parentheses space equals space h c open parentheses fraction numerator 1 space over denominator lambda subscript 2 end fraction space minus space fraction numerator 1 space over denominator lambda subscript 1 end fraction close parentheses

fraction numerator open parentheses V subscript 2 space minus space V subscript 1 close parentheses over denominator open parentheses fraction numerator 1 space over denominator lambda subscript 2 end fraction space minus space fraction numerator 1 space over denominator lambda subscript 1 end fraction close parentheses end fraction space equals space fraction numerator h c over denominator e end fraction

Exam Tip

When using the photoelectric effect equation, hfΦ and Ek(max) must all have the same units; Joules.

All values given in eV need to be converted into Joules by multiplying by 1.6 × 10−19. Do this right away, in the same way as you would convert into SI units before calculating.

It is important to note that the stopping voltage actually holds a negative value, but since we use it to determine the maximum kinetic energy of the emitted electrons, its sign is not important in calculations, it's acceptable to just quote its magnitude.

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Katie M

Author: Katie M

Katie has always been passionate about the sciences, and completed a degree in Astrophysics at Sheffield University. She decided that she wanted to inspire other young people, so moved to Bristol to complete a PGCE in Secondary Science. She particularly loves creating fun and absorbing materials to help students achieve their exam potential.