The Free Electron Theory of Metals - PowerPoint PPT Presentation

1 / 23
About This Presentation
Title:

The Free Electron Theory of Metals

Description:

Density of States. How many states between energy levels E and E dE? ... Z(E): density of states. Only positive values for nX, nY, and nZ , so it needs to ... – PowerPoint PPT presentation

Number of Views:2064
Avg rating:3.0/5.0
Slides: 24
Provided by: Meng6
Category:

less

Transcript and Presenter's Notes

Title: The Free Electron Theory of Metals


1
The Free Electron Theory of Metals
  • Chapter 6 of Solymar

2
Free Electrons
  • The valence electrons in the metal are free to
    move around, but they cant escape the metal
  • They are in a potential well
  • In 1-dimensional case
  • If a cube of side L

3
Quantized Energy Levels?
  • The allowed energy is an integral multiple of
    h2/8mL2
  • If L 1 cm
  • Yes! The energy is quatized!
  • The difference between adjacent energy levels
    increases at higher energy
  • If the maximum energy E 3 eV
  • If
  • Then nX 1.64?107
  • Then energy level just below the maximum energy
    is nX 1, nY, nZ

4
Density of States
  • How many states between energy levels E and E
    dE?
  • Consider a 3-dimensional space formed by nX, nY,
    and nZ
  • Each point with integer coordinates represents a
    state, i.e. a unit cube contains exactly one
    state
  • The number of states in a sphere of radius n is
    equal to the numerical value of the volume
  • The number of states having energy less than E

5
Density of States (Cont.)
  • Number of states with energy less than E dE
  • Number of states with energy between E and E dE
  • Z(E) density of states
  • Only positive values for nX, nY, and nZ , so it
    needs to multiply 1/8
  • Each state allows two values for spin, so it
    needs to multiply 2

6
Fermi-Dirac Distribution
  • What is the probability of occupancy for a state?
  • Based on Paulis exclusion principle
  • EF Fermi level
  • At T 0 (Fig. 6.1)
  • F(E) 1 when E lt EF Electrons fill up states to
    EF
  • F(E) 0 when E gt EF All states above EF are
    empty

7
Fermi Level
  • Therefore
  • N number of electrons/volume
  • Table 1 calculated EF

8
Fermi-Dirac Distribution (Cont.)
  • When E EF gtgt kT (low temperature or high
    energy)
  • This is Maxwell-Boltzmann distribution
  • When EF E gtgt kT (low energy)
  • The probability of non-occupancy is 1 F(E), so
    the probability of non-occupancy varies
    exponentially
  • In the range E EF, F(E) changes sharply
  • If we define the transition region as between
    F(E) 0.9 and F(E) 0.1, the width of the
    region is 4.4kT

9
Specific Heat
  • The specific heat per electron
  • ltEgt is the average energy of electrons
  • In classical physics
  • In quantum mechanics, ltEgt is finite when
    temperature goes to zero
  • So
  • Electrons way below EF have nowhere to go when
    they receive a small amount of energy, so they
    dont contribute to specific heat

10
Work Function
  • It takes energy to remove electrons from a metal
  • Heat, light, etc.
  • There is a certain threshold energy the electrons
    must possess in order to escape a given metal
  • This threshold energy is called work function f
  • At T 0, f is the energy barrier for electrons
    to escape (Fig. 6.2)

11
Thermionic Emission
  • Emission of electrons from a metal at high
    temperatures is called thermionic emission
  • They must have energy more than EF f
  • For free electrons
  • If x is normal to the surface of the metal,
    electrons must travel in the x-direction to
    escape
  • If the reflection coefficient is g(px), the
    probability of escape is 1 - g(px)

12
Thermionic Emission (Cont.)
  • The number of electrons arriving at the surface
    per second per unit area
  • N(px) number of electrons having momentum
    between px and px dpx
  • Number of electrons with a chance to escape
  • The emission current density

13
How to Find N(px)
  • First find density of states Z(px)
  • For a cube of metal of side 1
  • The number of states in a volume dnxdnydnz is
    dnxdnydnz or
  • Divide it by 8 and multiply by 2

14
Mathematics
  • The number of electrons in the momentum range px,
    px dpx, py, py dpy, pz, pz dpz
  • Integrate

15
Thermionic Current
  • Assume g(px) g is independent of px
  • Where
  • J varies exponentially, which agrees with
    experiments
  • Work functions of several metals (Table 6.2)
  • Measurement setup (Fig. 6.3)
  • Current cant sustain due to charge build-up
  • (a) thermionic electrons scattered by air
    molecules
  • (b) thermionic electrons accumulates in the
    vicinity of the metal
  • (c) a dc voltage sweeps electrons to anode

16
Image Force
  • Thermionic emission with image force and electric
    field
  • Image Force (Fig. 6.4)
  • An electron in front of an infinitely conducting
    sheet experiences a force which is equivalent to
    replacing the sheet by the mirror charge
  • The potential energy
  • The reference point is at x ?
  • Previously the reference point was the bottom of
    the potential well, i.e. a valence electron at
    rest

17
Electric Field
  • Fig. 6.5
  • (a) Metal-vacuum interface without image force or
    electric field
  • (b) Effect of image force
  • (c) Effect of a constant electric field
  • (d) Combined effect of image force and electric
    field
  • The maximum of the potential energy
  • The energy required to escape is reduced by -Vmax

18
The Schottky Effect
  • Due to image force and electric field, the
    effective work function is
  • The thermionic current
  • This is known as the Schottky effect or barrier
    lowering effect
  • Fig. 6.6 Log(J) vs. 1/T or Log(J/T2) vs. 1/T
    gives a straight line

19
Field Emission
  • The presence of an electric field increases the
    emission current due to barrier lowering
  • Further increase in electric field (109 V/m)
    leads to electrons tunneling through the
    potential barrier
  • Fig. 6.7 The barrier becomes thin under the
    electric field and the electrons can tunnel
    through field emission
  • Higher energy electrons have thinner barrier to
    tunnel through, but they are few of them
  • The main contribution to the tunneling current
    comes from electrons around the Fermi level
  • The width of the barrier
  • The height of the barrier is feff

20
Field Emission Current
  • Equivalent barrier (Fig. 6.8)
  • Tunneling current can be derived
  • J is an exponential function of xF
  • This current is temperature independent
  • Tunneling current is temperature independent, but
    thermionic current is temperature dependent

21
Photoelectric Effect
  • Photons can excite electrons in a metal to escape
    (Fig. 6.11)
  • Experimental set-up
  • When an electromagnetic wave is incident, there
    is no current unless the frequency of the wave is
    high enough
  • Then an electric current flows between the
    electrodes. The magnitude of the current is
    proportional to incident power
  • Photons are the particle equivalents of
    electromagnetic waves
  • Each photon has energy
  • If incident power is P and frequency is w, the
    number of photons incident is

22
Metallic Junction
  • When two metals of different work functions are
    in contact
  • Fig. 6.12 Electrons flow from left to right
    particle equivalents of electromagnetic waves
  • An excess of positive charge on left and negative
    charge on right
  • An electric field is built in the metallic
    junction
  • The electric field drives electrons from right to
    left
  • At equilibrium, equal numbers of electrons move
    left to right and right to left
  • Fig. 6.13
  • At equilibrium, the Fermi level is leveled
  • The potential difference between two metals, the
    contact potential, is equal to the work function
    difference
  • If we put an electron in the contact region, it
    will be pulled to left

23
HW Assignment
  • 6.3, 6.5, 6.7, 6.8
Write a Comment
User Comments (0)
About PowerShow.com