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A Presentation on
Fermi -Dirac distribution function
By
Ms.Chetana Magadum
Smt. Kasturbai Walchand College,Sangli
 Some basic concepts:-
 Fermi level :- This is the term used to describe the
top of the collection of electron energy levels at
absolute zero temperature.
 Fermi energy:-This is the maximum energy that an
electron can have in a conductor at 0K. It is given
by
𝐸 𝐹 =
1
2
𝑚𝑣 𝐹
2
where 𝑣 𝐹 is the velocity of electron at Fermi level.
 Fermi -Dirac distribution function :- This describes the
occupancy of energy levels by electrons in a solid. The
probability that the energy level E is filled by an electron is
given by
𝑓 𝐸 =
1
1 + 𝑒(𝐸−𝐸 𝐹)/𝑘𝑇
where 𝐸 𝐹 is the Fermi level energy.
 Note:-
1.The Fermi velocity of these conduction electrons can be
calculated from the Fermi energy.
𝑣 𝐹 =
2𝐸 𝐹
𝑚
1
2
2. The Fermi function 𝑓 𝐸 gives the probability that a given
available electron energy state will be occupied at a given
temperature. The Fermi function comes from Fermi-Dirac
statistics
3. The basic nature of this function dictates that at ordinary
temperatures, most of the levels up to the Fermi level EF
are filled, and relatively few electrons have energies above
the Fermi level.
4. The Fermi level is on the order of electron volts (e.g., 7
eV for copper), whereas the thermal energy kT is only
about 0.026 eV at 300K.
5. The band theory of solids gives the picture that there is
a sizable gap between the Fermi level and the conduction
band of the semiconductor. At higher temperatures, a
larger fraction of the electrons can bridge this gap and
participate in electrical conduction.
 Derivation of the Fermi-Dirac distribution function
We start from a series of possible energies, labeled Ei. At each
energy we can have gi possible states and the number of states
that are occupied equals gifi, where fi is the probability of
occupying a state at energy Ei.
The number of possible ways - called configurations - to fit gi fi
electrons in gi states, given the restriction that only one electron
can occupy each state, equals:
This equation is obtained by numbering the individual states and
exchanging the states rather than the electrons. This yields a
total number of gi! possible configurations. However since the
empty states are all identical, we need to divide by the number
of permutations between the empty states, as all permutations
can not be distinguished and can therefore only be counted
once. In addition, all the filled states are indistinguishable from
each other, so we need to divide also by all permutations
between the filled states, namely gifi!.
The number of possible ways to fit the electrons in the
number of available states is called the multiplicity function.
The multiplicity function for the whole system is the product
of the multiplicity functions for each energy Ei
Using Stirling’s approximation, one can eliminate the
factorial signs, yielding:
The total number of electrons in the system equals N and
the total energy of those N electrons equals E. These
system parameters are related to the number of states at
each energy, gi, and the probability of occupancy of each
state, fi, by: and
According to the basic assumption of statistical
thermodynamics, all possible configurations are equally
probable. The multiplicity function provides the number of
configurations for a specific set of occupancy probabilities,
fi. The multiplicity function sharply peaks at the thermal
equilibrium distribution. The occupancy probability in
thermal equilibrium is therefore obtained by finding the
maximum of the multiplicity function, W, while keeping the
total energy and the number of electrons constant.
For convenience, we maximize the logarithm of the
multiplicity function instead of the multiplicity function itself.
According to the Lagrange method of undetermined
multipliers, we must maximize the following function:
where a and b need to be determined. The maximum
multiplicity function is obtained from:
or
which can be written in the following form
with 𝛽= 1/b and EF = -a/b. The symbol EF was chosen since
this constant has units of energy and will be the constant
associated with this probability distribution.
Taking the derivative of the total energy, one obtains:
Using the Lagrange equation, this can be rewritten as:
Any variation of the energies, Ei, can only be caused by a
change in volume, so that the middle term can be linked to
a volume variation dV.
Comparing this to the thermodynamic identity:
one finds that b = kT and S = k lnW . The energy, EF,
equals the energy associated with the particles, m.
The comparison also identifies the entropy, S, as
being the logarithm of the multiplicity function, W,
multiplied with Boltzmann’s constant.
The Fermi-Dirac distribution function then becomes:
Thank you.

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Presentation on the Fermi-Dirac Distribution Function

  • 1. A Presentation on Fermi -Dirac distribution function By Ms.Chetana Magadum Smt. Kasturbai Walchand College,Sangli
  • 2.  Some basic concepts:-  Fermi level :- This is the term used to describe the top of the collection of electron energy levels at absolute zero temperature.  Fermi energy:-This is the maximum energy that an electron can have in a conductor at 0K. It is given by 𝐸 𝐹 = 1 2 𝑚𝑣 𝐹 2 where 𝑣 𝐹 is the velocity of electron at Fermi level.
  • 3.  Fermi -Dirac distribution function :- This describes the occupancy of energy levels by electrons in a solid. The probability that the energy level E is filled by an electron is given by 𝑓 𝐸 = 1 1 + 𝑒(𝐸−𝐸 𝐹)/𝑘𝑇 where 𝐸 𝐹 is the Fermi level energy.  Note:- 1.The Fermi velocity of these conduction electrons can be calculated from the Fermi energy. 𝑣 𝐹 = 2𝐸 𝐹 𝑚 1 2 2. The Fermi function 𝑓 𝐸 gives the probability that a given available electron energy state will be occupied at a given temperature. The Fermi function comes from Fermi-Dirac statistics
  • 4. 3. The basic nature of this function dictates that at ordinary temperatures, most of the levels up to the Fermi level EF are filled, and relatively few electrons have energies above the Fermi level. 4. The Fermi level is on the order of electron volts (e.g., 7 eV for copper), whereas the thermal energy kT is only about 0.026 eV at 300K. 5. The band theory of solids gives the picture that there is a sizable gap between the Fermi level and the conduction band of the semiconductor. At higher temperatures, a larger fraction of the electrons can bridge this gap and participate in electrical conduction.
  • 5.  Derivation of the Fermi-Dirac distribution function We start from a series of possible energies, labeled Ei. At each energy we can have gi possible states and the number of states that are occupied equals gifi, where fi is the probability of occupying a state at energy Ei. The number of possible ways - called configurations - to fit gi fi electrons in gi states, given the restriction that only one electron can occupy each state, equals: This equation is obtained by numbering the individual states and exchanging the states rather than the electrons. This yields a total number of gi! possible configurations. However since the empty states are all identical, we need to divide by the number of permutations between the empty states, as all permutations can not be distinguished and can therefore only be counted once. In addition, all the filled states are indistinguishable from each other, so we need to divide also by all permutations between the filled states, namely gifi!.
  • 6. The number of possible ways to fit the electrons in the number of available states is called the multiplicity function. The multiplicity function for the whole system is the product of the multiplicity functions for each energy Ei Using Stirling’s approximation, one can eliminate the factorial signs, yielding: The total number of electrons in the system equals N and the total energy of those N electrons equals E. These system parameters are related to the number of states at each energy, gi, and the probability of occupancy of each state, fi, by: and
  • 7. According to the basic assumption of statistical thermodynamics, all possible configurations are equally probable. The multiplicity function provides the number of configurations for a specific set of occupancy probabilities, fi. The multiplicity function sharply peaks at the thermal equilibrium distribution. The occupancy probability in thermal equilibrium is therefore obtained by finding the maximum of the multiplicity function, W, while keeping the total energy and the number of electrons constant. For convenience, we maximize the logarithm of the multiplicity function instead of the multiplicity function itself. According to the Lagrange method of undetermined multipliers, we must maximize the following function:
  • 8. where a and b need to be determined. The maximum multiplicity function is obtained from: or which can be written in the following form with 𝛽= 1/b and EF = -a/b. The symbol EF was chosen since this constant has units of energy and will be the constant associated with this probability distribution. Taking the derivative of the total energy, one obtains:
  • 9. Using the Lagrange equation, this can be rewritten as: Any variation of the energies, Ei, can only be caused by a change in volume, so that the middle term can be linked to a volume variation dV. Comparing this to the thermodynamic identity: one finds that b = kT and S = k lnW . The energy, EF, equals the energy associated with the particles, m.
  • 10. The comparison also identifies the entropy, S, as being the logarithm of the multiplicity function, W, multiplied with Boltzmann’s constant. The Fermi-Dirac distribution function then becomes: