3- Energy Band Theory

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    ENERGY BAND THEORY

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    Introduction

    To develop the current-voltage characteristics of semiconductordevices, we need to determine the electrical properties ofsemiconductor materials.

    To accomplish this, we have to:

    determine the properties of electrons in a crystal lattice, determine the statistical characteristics of the very large number of

    electrons in a crystal.

    We know that electron in a single crystal take discrete values ofenergy.

    We expand this concept to a band of allowed energies in a crystal.

    This energy band theory is a basic principle of semiconductormaterial physics.

    It can also be used to explain differences in electrical

    characteristics between metals, insulators, and semiconductors. We will introduce electron effective mass which relates quantum

    mechanics to classical Newtonian mechanics.

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    Introduction

    we will define a new particle in a semiconductor called a hole.

    We will develop the statistical behavior of electrons in a crystal

    To determine the statistical law of electrons, we note that Pauli

    exclusion principle is an important factor. The resulting probability function will determine the distribution of

    electrons among the available energy states.

    The energy band theory and the probability function will be usedlater to develop the theory of the semiconductor in equilibrium.

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    Probability Density Functions forOne and Two Hydrogen Atoms

    Probability density function for the

    lowest electron energy state of thesingle, noninteracting hydrogen atom

    Overlapping probability densityfunction of two adjacent hydrogenatomsThe wave functions of the twoatom electrons overlap, which

    means that the two electrons willinteract.

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    Energy Level Splitting By InteractionBetween Two Atoms

    This interaction or perturbation results in thediscrete quantized energy level splitting intotwo discrete energy levels.The splitting is consistent with Pauli

    exclusion principle.When we push several atoms together tomake close to each other, the initial quantizedenergy level will split into a band of discreteenergy levels.

    Within the allowed band, the energies are atdiscrete levels.

    According to Pauli exclusion principle, totalnumber of quantum states does not change.However, since no two electrons can have

    the same quantum number, the discreteenergy must split into a band of energies inorder that each electron can occupy a distinct

    quantum state.When a large number of atoms get close to

    make a crystal, difference between energystates are very small.

    equilibrium interatomic distance

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    Allowed And Forbidden Energy Bands

    Two atoms with n=3 energy levelWhen these two atoms are

    brought close together, first theoutermost level (n=3) is split and

    then the second level and finally thefirst level (n=1).

    This energy-bandsplitting and theformation of allowed

    and forbidden bands

    is the energy-bandtheory of single-crystal materials

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    Energy Band Formation

    As the interatomic distance decreases,

    the 3s and 3p states interact and overlap.At the equilibrium interatomic distance,

    the bands have again split.But now four quantum states per atomare in the lower band and four quantum

    states per atom are in the upper band.

    At absolute zero degrees, electrons are in

    the lowest energy state,So that all states in the lower band (thevalence band) will be full and all states in

    the upper band (the conduction band) willbe empty.

    The bandgap energy Eg between the top of the valence band and the bottom ofthe conduction hand is the width of the forbidden energy band.

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    Potential Function for SingleIsolated Atom

    Consider an one-dimensional array of atoms in a crystalline lattice:

    a= lattice constant

    The attractive force between an atomic core located at x=0 and electronsituated at an arbitrary point x is:

    Allowed energy levels for the electron

    2

    0

    1( )

    4

    qV x

    r r=

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    Potential Functions ofAdjacent Atoms

    If we add the attractive force by theatomic core located at x=a:

    rV(r)

    And for the one-dimensional crystalline

    lattice: V(r)

    r

    The potential functions of adjacentatoms overlap:

    We need this potential function touse in Schrodinger's wave equation to

    model a one-dimensional single-crystalmaterial.

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    Kronig-Penney Model ofPotential Functions

    a: potential well width;b: potential barrier width

    This model is used to represent a one-

    dimensional single-crystal lattice for

    considering electron behavior in crystallinelattice.

    The Kronig-Penney model isan idealized periodic potential

    representing a one-dimensionalsingle crystal.

    Schrodinger's wave equation ineach region must be solved.

    To obtain the solution to Schrodinger's wave equation, we make use Blochtheorem.

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    Bloch TheoremThe theorem states that:

    If V(x+a)=V(x)

    Then (x+a)=ejka (x)

    Or, equivalently

    (x)=ejkx u(x) u(x) is unit cell wavefunction andu(x+a)= u(x)

    The parameter k is called a constant of motion

    ( / )( , ) ( ) ( ) ( ) .jkx j E tx t x t u x e e = = We have

    ( )( )/( , ) ( )

    j kx E t x t u x e

    =

    This traveling-wave solution represents the motion of an electron in a single-crystal material.

    The amplitude of the traveling wave is a periodic function.

    k=wave number.

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    The k-Space Diagram

    For free electron

    and

    and

    For electron in a infinite potential well2 2 2

    2

    2

    n

    nE

    m a

    =

    n

    np

    a

    =

    Discrete points lie along the E-p curve

    of a free electron.

    Since the momentum and wave number

    are linearly related, these figures are alsothe E versus k curve.

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    Relation between k and ETime-independent Schrdingers Equation:

    Assume E < VoIn region I, 0

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    For region I:

    ( ) ( )

    1( )j k x j k x

    u x Ae Be +

    = +For region II

    ( ) ( )

    2

    ( )j k x j k x

    u x Ce De += +

    Since the potential function V(x) is everywhere finite, both the wave

    function (x) and its first derivative (x)/x must be continuous.So, at x=0: u1(0)=u2(0) A+B C-D=0

    On other hand using 1 20 0| |x xdu du

    dx dx= ==

    We obtain

    Also u1(a)=u2(b) and by applying it:

    ( ) ( ) ( ) ( )

    0j k a i k a j k b j k b

    Ae Be Ce De + +

    + = =

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    Finally, the boundary condition

    gives

    By using the resulted equations, we obtain constants and the solution.The result is:

    This equation relates the parameter k to the total energy E (through theparameter a) and the potential function Vo (through the parameter ).

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    We have

    If E < V0, then is imaginary quantity.Then the equation

    can be written as

    The solution of this equation results in a band of allowed energies.

    To obtain a graphical solution for this equation, let the potential

    barrier width b 0 and the barrier height Vo 0, such that the productbVo remains finite.We may approximate sinhb b and coshb 1

    The equation can be written as:

    2 2

    (sin )(sinh ) (cos )(cosh ) cos ( )2

    a b a b k a b + = +

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    ' 0

    2

    m V b a

    P =

    If we define

    ' s in

    c o s c o s ( )

    a

    P a k aa

    + =

    If the left side of this equation is plotted as a function ofa, we have:

    Since |cos ka| 1, the

    right side falls between 1,

    -1.

    Therefore, only the

    shaded regions are allowed

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    The k-Space Diagram

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    Consider the equation' s in c o s c o s ( )

    aP a k a

    a

    + =

    For cosine we have

    where n is a positive integer

    We may consider

    various segments of the curve can be

    displaced by the 2 factor. E versus k diagram in thereduced-zone representation.

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    Forbidden Gap

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    The E versus k diagram of the

    conduction and valence bands of asemiconductor at T > 0 K.

    The E versus k diagram of the

    conduction and valence bandsof a semiconductor at T = 0 K

    The energy states in the valence band

    are completely full and the states in the

    conduction band are empty.

    At T>0oK, some electrons have

    gained enough energy to jump to the

    conduction band and have left

    empty states in the valence hand.

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    Electron Effective Mass

    The movement of an electron in a lattice will, in general, be different from that

    of an electron in free space.

    In addition to an externally applied force, there are internal forces in the

    crystal due to

    positively charged ions or protons and

    negatively charged electrons, which will influence the motion of electrons

    in the lattice.

    We have

    F ma=To take into account internal forces, we can write: *F m a=

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    Electron Effective Mass

    Newtons second Law of motion,

    Electrons wave-particle duality,

    The first

    derivative of E

    with respect to k

    is related to thevelocity of the

    particle.

    The second derivative of E with respect to k is inversely proportional to themass of the particle.

    2 2

    2 *d Ed k m

    =

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    Example

    Consider energy band segment

    First derivative

    Second derivative

    One concludes that m*>0 near the band-energy

    minimum and m*

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    Concept of HoleA positively charged "empty state" is created when a valence electron is elevated

    into the conduction band.

    if a valence electron gains a small amount of thermal energy, it may move into the

    empty state.

    Hole has a positive chargeHole has a positive effective mass.

    Hole moves in the same direction as an

    applied electric field.

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    Conduction Band and Valence Band

    For valence band

    holes

    For conduction

    band electrons

    Bandgap

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    Band Structure of Insulators

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    Band Structure of Semiconductors

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    Band Structure of Metals

    It is easy for the electrons to jump into the empty levels, so metals

    have high conductivity.

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    E-k Diagram in 3Dwe will extend the allowed and forbidden energy band and effective mass

    concepts to three dimensions and to real crystals.

    One problem encountered in extending the potential function to a three-

    dimensional crystal is that the distance between atoms varies as the direction

    through the crystal changes.

    So, Electrons traveling in

    different directions

    encounter different potential

    patterns and

    therefore different k-space

    boundaries.

    The E versus k diagrams

    are in general a function of

    the k-space direction in acrystal.

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    The k-Space Diagrams of Si and GaAs

    direct bandgap semiconductor indirect bandgap semiconductor

    Germanium is also an indirect bandgap material, whose valence band

    maximum occurs at k=0 and whose conduction band minimum occurs along

    the [111] direction.

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    Carriers for Conductance

    The number of carriers that can contribute to current flow is a function of thenumber of available energy states or quantum states.

    we indicated that the band of allowed energies was actually made up of discrete

    energy levels.

    We must determine the density of these allowed energy states as a function of

    energy in order to calculate the electron and hole concentrations.

    Probability ofoccupation of

    statesX

    Number of

    available

    states

    Actual

    Population ofConductance

    Band

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    Density of States

    For the 3D infinite potential well

    For the conductance band

    nk

    a

    =and

    For the valence band

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    Plot of Density of States

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    The Distribution Function

    Distribution function: the probability that a quantum state at the energy E will beoccupied by an electron.

    ( )

    ( ) ( )

    N E

    f E g E=

    N (E): the number density, i.e., the number of particles per unit energy

    per unit volumeg (E): the density of states, i.e., the number of quantum states per unit energy per

    unit volume

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    The Fermi-Distribution Function

    At equilibrium, the electrons behavior follows the Fermi (or Fermi-Diract)distribution function

    ( )

    ( )

    N E

    g E=

    EF: the Fermi level or

    Fermi energy

    energy of the highestquantum state of

    electrons at 0 K

    At 0 K,EEF, f(E)=0

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    The Fermi-Distribution Function

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    The Fermi-Distribution Function

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    Maxwell-Boltzmann approximation

    when E - EF >> kT

    This equation is called Maxwell-Boltzmann approximation or Boltzmann

    approximation to Fermi-Dirac function