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EINSTEIN MODEL
&
HEAT CONDUCTION BY
PHONONS
QP & QC
NANOTECHNOLOGY
ωε 





+=
2
1
nn n = 0,1,2,3,..
ω
ω
ω
ω
E
Quantum Mechanical Simple Harmonic Oscillator
• Quantum mechanical results for a simple harmonic oscillator
with classical frequency ω: The energy is quantized
En
• Energy levels are
equally spaced!
Often, we consider En as being constructed by adding n excitation
quanta of energy to the ground state.ω
ωε 
2
1
0 =
If the system makes a transition from a lower energy level to a higher
energy level, it is always true that the change in energy is an integer
multiple of
Phonon absorption or
emission
E0 Ground state energy of the
oscillator.
ω
ΔE = (n – n΄) ω
n & n ΄ = integers
In complicated processes, such as phonons interacting with
electrons or photons, it is known that phonons are not conserved.
That is, they can be created and destroyed during such
interactions.
Thermal Energy & Lattice Vibrations
As we’ve been discussing in detail, the atoms in a crystal vibrate
about their equilibrium positions.
This motion produces vibrational waves.
The amplitude of this vibrational motion increases
as the temperature increases.
In a solid, the energy associated with these vibrations is called
Thermal
Energy
• A knowledge of the thermal energy is fundamental to obtaining an
understanding many of the basic properties of solids. A relevant
question is how do we calculate this thermal energy?
• Also, we would like to know how much thermal energy is available to
scatter a conduction electron in a metal or semiconductor. This is
important; this scattering contributes to electrical resistance in the material.
• Most important, though, this thermal energy plays a fundamental
role in determining the
Thermal Properties of a Solid
• A knowledge of how the thermal energy changes with temperature gives
an understanding of the heat energy which is necessary to raise the
temperature of the material.
• An important, measureable property of a solid is it’s
Specific Heat or Heat Capacity
The thermal energy is the dominant contribution to the heat
capacity in most solids. In non-magnetic insulators, it is the only
contribution. Some other contributions:
Conduction Electrons in metals & semiconductors.
The magnetic ordering in magnetic materials.
Calculation of the vibrational contribution to the thermal energy & heat
capacity of a solid has 2 parts:
1. Evaluation of the contribution of a single vibrational mode.
2. Summation over the frequency distribution of the modes.
Lattice Vibrational Contribution to the Heat Capacity
Vibrational Specific Heat of Solids
cp Data at T = 298 K
n
n
nP εε ∑=
_
Average energy of a harmonic
oscillator and hence of a lattice
mode of angular frequency at
temperature T
Average energy of a harmonic
oscillator and hence of a lattice
mode of angular frequency at
temperature T
Energy of oscillatorEnergy of oscillator
1
2
n nε ω
 
= + ÷
 
h
The probability of the oscillator being in
this level as given by the Boltzman factor
The probability of the oscillator being in
this level as given by the Boltzman factor
exp( / )n Bk Tε−
Thermal Energy & Heat Capacity
Einstein Model
0
/2 3 /2 5 /2
/2 / 2 /
/2 / 1
1
exp[ ( ) ]
2
.....
(1 .....
(1 )
B B B
B B B
B B
n B
k T k T k T
k T k T k T
k T k T
z n
k T
z e e e
z e e e
z e e
ω ω ω
ω ω ω
ω ω
ω∞
=
− − −
− − −
− − −
= − +
= + + +
= + + +
= −
∑
h h h
h h h
h h
h
_
0
0
1 1
exp /
2 2
1
exp /
2
B
n
B
n
n n k T
n k T
ω ω
ε
ω
∞
=
∞
=
    
+ − + ÷  ÷ 
    =
  
− + ÷ 
  
∑
∑
h h
h
(*)
According to the Binomial expansion for x«1 where
/ Bx k Tω= −h
n
n
nP εε ∑=
_
Eqn (*) can be written
_
/
1
2 1Bk T
e ω
ω
ε ω= +
−h
h
h
'
(ln )
x
x
x x
∂
=
∂
( )
( )
( )
_
2 2
/ 2_
2
/
_
/2 /2
_
/2
/
2 2_
2
2 2 /
1
(ln )
ln
1
ln ln 1
ln 1
2
2
4 1
B
B
B B
B
B
B
B B
k T
B k T
k T k T
B
k T
B
B
k TB
B B
B k T
B
z
k T k T z
z T T
e
k T
T e
k T e e
T
k T e
T k T T
k
e
k k T
k T
k T e
ω
ω
ω ω
ω
ω
ω
ε
ε
ε
ω
ε
ω
ω
ε
−
−
− −
−
−
−
∂ ∂
= =
∂ ∂
 ∂
=  ÷
∂ − 
∂  = − − ∂
  ∂ ∂
= − − −  ÷
∂ ∂  
 

= +
−
 
h
h
h h
h
h
h
h
h
h
( )
/
/
1
2 1
B
B
k T
k T
e
e
ω
ω
ω
ω
−
−

 = +
−

h
h
h
h
Finally, the
result is
_
/
1
2 1Bk T
e ω
ω
ε ω= +
−h
h
h
This is the Mean Phonon Energy. The first term in the above
equation is the zero-point energy. As mentioned before even at 0ºK
atoms vibrate in the crystal and have zero-point energy. This is the
minimum energy of the system.
The average number of phonons is given by the Bose-Einstein
distribution as
1
1
)(
−
=
TBk
e
n ωω h
The second term in the mean energy is the phonon contribution to the
thermal energy.
(number of phonons) x (energy of phonon) = (second term in )
_
ε
ε Mean energy of a
harmonic oscillator
as a function of T
Low Temperature Limit
T
ωh
2
1
TkB
TkBhω
12
1_
−
+=
TBk
e
ω
ω
ωε h
h
h
ωε h
2
1_
= Zero Point Energy
Since exponential term
gets bigger
is independent of frequency of oscillation.
This is the classical limit because the energy
steps are now small compared with the energy
of the harmonic oscillator.
So that is the thermal energy of the
classical 1D harmonic oscillator.
ε
..........
!2
1
2
+++=
x
xex
Tk
e
B
TBk
ωω
hh
+=1
112
1_
−+
+=
TkB
ω
ω
ωε
h
h
h
_
1
2
Bk Tε ω= +h
_
Bk Tε ≈
ε
High Temperature Limit
T
ωh
2
1
TkB Mean energy of a
harmonic oscillator
as a function of T
Bk Tωh =<<
ε
Heat Capacity C
• Heat capacity C can be found by differentiating the
average phonon energy
12
1_
−
+=
TBk
e
ω
ω
ωε h
h
h
( )
( )
2
2
1
k TB
k TB
B
B
v
k
e
k Td
C
dT
e
ω
ω
ω
ω
ε
−
−
= =
−
h
h
h
h
( )
( )
( )
2
2 2
1
k TB
k TB
v B
B
e
C k
k T e
ω
ω
ω
=
−
h
h
h
k
ω
θ =
h
( )
2
2
1
T
T
v B
e
C k
T
e
θ
θ
θ 
=  ÷
  −
Let
( )
2
2
1
T
T
v B
e
C k
T
e
θ
θ
θ 
=  ÷
  −
Area =
2
ωh
T
Bk
Bk
ωh
Specific heat in this approximation
vanishes exponentially at low T and
tends to classical value at high
temperatures.
These features are common to all
quantum systems; the energy tends to
the zero-point-energy at low T and to
the classical value of Boltzmann
constant at high T.
vC
k
ω
θ =
h
where
,T K
3R
This range usually includes RT.
From the figure it is seen that Cv is
equal to 3R at high temperatures
regardless of the substance. This fact is
known as Dulong-Petit law. This law
states that specific heat of a given
number of atoms of any solid is
independent of temperature and is the
same for all materials!
vC
Specific heat at constant volume depends on temperature as shown in
figure below. At high temperatures the value of Cv is close to 3R,
where R is the universal gas constant. Since R is approximately 2
cal/K-mole, at high temperatures Cv is app. 6 cal/K-mole.
Cv vs T for Diamond
Points:
Experiment
Curve:
Einstein Model
Prediction
Classical Theory of Heat Capacity of Solids
The solid is one in which each atom is bound to its side
by a harmonic force. When the solid is heated, the atoms
vibrate around their sites like a set of harmonic oscillators.
The average energy for a 1D oscillator is kT. Therefore, the
averaga energy per atom, regarded as a 3D oscillator, is 3kT,
and consequently the energy per mole is
=
where N is Avagadro’s number, kB is Boltzmann constant and R is the gas
constant. The differentiation wrt temperature gives;
3 3BNk T RT=
23 23
3 3 6.02 10 ( / ) 1.38 10 ( / )vC R atoms mole J K−
= = × × × ×
24.9 ;1 0.2388 6
( ) ( )
J Cal
Cv J Cal Cv
K mole K mole
= = ⇒
− −
;
v
d
C
dT
ε
=
ε
Einstein heat capacity of solids
• The theory explained by Einstein is the first quantum theory of solids.
He made the simplifying assumption that all 3N vibrational modes of a
3D solid of N atoms had the same frequency, so that the whole solid had
a heat capacity 3N times
• In this model, the atoms are treated as independent oscillators, but the energy
of the oscillators are taken quantum mechanically as
This refers to an isolated oscillator, but the atomic oscillators in a solid are not
isolated.They are continually exchanging their energy with their surrounding
atoms.
• Even this crude model gave the correct limit at high temperatures, a heat
capacity of the Dulong-Petit law where R is universal gas constant.
( )
2
2
1
T
T
v B
e
C k
T e
θ
θ
θ 
=  ÷
  −
3 3BNk R=
ωh
• At high temperatures, all crystalline solids have a specific heat of
6 cal/K per mole; they require 6 calories per mole to raise their
temperature 1 K.
•This arrangement between observation and classical theory break
down if the temperature is not high.
•Observations show that at room temperatures and below the
specific heat of crystalline solids is not a universal constant.
6
cal
Kmol
Bk
ωh
vC
T
3vC R=
In each of these materials (Pb,Al,
Si,and Diamond) specific heat
approaches constant value
asymptotically at high T. But at
low T’s, the specific heat
decreases towards zero which is
in a complete contradiction with
the above classical result.
• Einstein model also gave correctly a specific heat
tending to zero at absolute zero, but the
temperature dependence near T= 0 did not agree
with experiment.
• Taking into account the actual distribution of
vibration frequencies in a solid this discrepancy
can be accounted using one dimensional model of
monoatomic lattice
Density of States
According to Quantum Mechanics if a particle is constrained;
• the energy of particle can only have special discrete energy
values.
• it cannot increase infinitely from one value to another.
• it has to go up in steps.
Thermal Energy & Heat Capacity
Debye Model
• These steps can be so small depending on the system
that the energy can be considered as continuous.
• This is the case of classical mechanics.
• But on atomic scale the energy can only jump by a
discrete amount from one value to another.
Definite energy levels Steps get small Energy is continuous
• In some cases, each particular energy level can be
associated with more than one different state (or
wavefunction )
• This energy level is said to be degenerate.
• The density of states is the number of discrete
states per unit energy interval, and so that the number
of states between and will be .
( )ρ ε
( )dρ ε εdε ε+ε
Effect of phonons in nanostructures
 The broadening and shift of the Si and Ge Raman lines to
lower frequencies as the particle size decreases has been
attributed to phonon confinement effects in the nanocrystals.
 Acoustic phonons of nanoparticles exhibit Brillouin scattering
that depends on particle size.
 Acoustic modes shift to higher frequencies with reduced
particle size and optical modes shift to lower frequencies as
the particle size is reduced.

Contd…
 The temperature variation of the electrical mobility and
electrical conductivity for semiconductor nanostructures:
 Scattering by impurity atoms is important at low temperatures
but decreases with increasing temperature.
 In contrast, scattering by phonons increases with temperature,
reflecting the increasing amplitude of the lattice vibrations.
 The combined effect of these two processes is to give a mobility
which, at low temperatures, increases with increasing
temperature, followed by a decrease at high temperatures.
 In certain semiconductor nanostructures it is possible to turn
off the scattering by impurity atoms, resulting in very high
carrier nobilities at low temperatures.
THAN Q !THAN Q !

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Einestein model density of states

  • 1. EINSTEIN MODEL & HEAT CONDUCTION BY PHONONS QP & QC NANOTECHNOLOGY
  • 2. ωε       += 2 1 nn n = 0,1,2,3,.. ω ω ω ω E Quantum Mechanical Simple Harmonic Oscillator • Quantum mechanical results for a simple harmonic oscillator with classical frequency ω: The energy is quantized En • Energy levels are equally spaced!
  • 3. Often, we consider En as being constructed by adding n excitation quanta of energy to the ground state.ω ωε  2 1 0 = If the system makes a transition from a lower energy level to a higher energy level, it is always true that the change in energy is an integer multiple of Phonon absorption or emission E0 Ground state energy of the oscillator. ω ΔE = (n – n΄) ω n & n ΄ = integers In complicated processes, such as phonons interacting with electrons or photons, it is known that phonons are not conserved. That is, they can be created and destroyed during such interactions.
  • 4. Thermal Energy & Lattice Vibrations As we’ve been discussing in detail, the atoms in a crystal vibrate about their equilibrium positions. This motion produces vibrational waves. The amplitude of this vibrational motion increases as the temperature increases. In a solid, the energy associated with these vibrations is called Thermal Energy
  • 5. • A knowledge of the thermal energy is fundamental to obtaining an understanding many of the basic properties of solids. A relevant question is how do we calculate this thermal energy? • Also, we would like to know how much thermal energy is available to scatter a conduction electron in a metal or semiconductor. This is important; this scattering contributes to electrical resistance in the material. • Most important, though, this thermal energy plays a fundamental role in determining the Thermal Properties of a Solid • A knowledge of how the thermal energy changes with temperature gives an understanding of the heat energy which is necessary to raise the temperature of the material. • An important, measureable property of a solid is it’s Specific Heat or Heat Capacity
  • 6. The thermal energy is the dominant contribution to the heat capacity in most solids. In non-magnetic insulators, it is the only contribution. Some other contributions: Conduction Electrons in metals & semiconductors. The magnetic ordering in magnetic materials. Calculation of the vibrational contribution to the thermal energy & heat capacity of a solid has 2 parts: 1. Evaluation of the contribution of a single vibrational mode. 2. Summation over the frequency distribution of the modes. Lattice Vibrational Contribution to the Heat Capacity
  • 7. Vibrational Specific Heat of Solids cp Data at T = 298 K
  • 8. n n nP εε ∑= _ Average energy of a harmonic oscillator and hence of a lattice mode of angular frequency at temperature T Average energy of a harmonic oscillator and hence of a lattice mode of angular frequency at temperature T Energy of oscillatorEnergy of oscillator 1 2 n nε ω   = + ÷   h The probability of the oscillator being in this level as given by the Boltzman factor The probability of the oscillator being in this level as given by the Boltzman factor exp( / )n Bk Tε− Thermal Energy & Heat Capacity Einstein Model
  • 9. 0 /2 3 /2 5 /2 /2 / 2 / /2 / 1 1 exp[ ( ) ] 2 ..... (1 ..... (1 ) B B B B B B B B n B k T k T k T k T k T k T k T k T z n k T z e e e z e e e z e e ω ω ω ω ω ω ω ω ω∞ = − − − − − − − − − = − + = + + + = + + + = − ∑ h h h h h h h h h _ 0 0 1 1 exp / 2 2 1 exp / 2 B n B n n n k T n k T ω ω ε ω ∞ = ∞ =      + − + ÷  ÷      =    − + ÷     ∑ ∑ h h h (*) According to the Binomial expansion for x«1 where / Bx k Tω= −h n n nP εε ∑= _
  • 10. Eqn (*) can be written _ / 1 2 1Bk T e ω ω ε ω= + −h h h ' (ln ) x x x x ∂ = ∂ ( ) ( ) ( ) _ 2 2 / 2_ 2 / _ /2 /2 _ /2 / 2 2_ 2 2 2 / 1 (ln ) ln 1 ln ln 1 ln 1 2 2 4 1 B B B B B B B B B k T B k T k T k T B k T B B k TB B B B k T B z k T k T z z T T e k T T e k T e e T k T e T k T T k e k k T k T k T e ω ω ω ω ω ω ω ε ε ε ω ε ω ω ε − − − − − − − ∂ ∂ = = ∂ ∂  ∂ =  ÷ ∂ −  ∂  = − − ∂   ∂ ∂ = − − −  ÷ ∂ ∂      = + −   h h h h h h h h h h ( ) / / 1 2 1 B B k T k T e e ω ω ω ω − −   = + −  h h h h Finally, the result is
  • 11. _ / 1 2 1Bk T e ω ω ε ω= + −h h h This is the Mean Phonon Energy. The first term in the above equation is the zero-point energy. As mentioned before even at 0ºK atoms vibrate in the crystal and have zero-point energy. This is the minimum energy of the system. The average number of phonons is given by the Bose-Einstein distribution as 1 1 )( − = TBk e n ωω h The second term in the mean energy is the phonon contribution to the thermal energy. (number of phonons) x (energy of phonon) = (second term in ) _ ε
  • 12. ε Mean energy of a harmonic oscillator as a function of T Low Temperature Limit T ωh 2 1 TkB TkBhω 12 1_ − += TBk e ω ω ωε h h h ωε h 2 1_ = Zero Point Energy Since exponential term gets bigger
  • 13. is independent of frequency of oscillation. This is the classical limit because the energy steps are now small compared with the energy of the harmonic oscillator. So that is the thermal energy of the classical 1D harmonic oscillator. ε .......... !2 1 2 +++= x xex Tk e B TBk ωω hh +=1 112 1_ −+ += TkB ω ω ωε h h h _ 1 2 Bk Tε ω= +h _ Bk Tε ≈ ε High Temperature Limit T ωh 2 1 TkB Mean energy of a harmonic oscillator as a function of T Bk Tωh =<< ε
  • 14. Heat Capacity C • Heat capacity C can be found by differentiating the average phonon energy 12 1_ − += TBk e ω ω ωε h h h ( ) ( ) 2 2 1 k TB k TB B B v k e k Td C dT e ω ω ω ω ε − − = = − h h h h ( ) ( ) ( ) 2 2 2 1 k TB k TB v B B e C k k T e ω ω ω = − h h h k ω θ = h ( ) 2 2 1 T T v B e C k T e θ θ θ  =  ÷   − Let
  • 15. ( ) 2 2 1 T T v B e C k T e θ θ θ  =  ÷   − Area = 2 ωh T Bk Bk ωh Specific heat in this approximation vanishes exponentially at low T and tends to classical value at high temperatures. These features are common to all quantum systems; the energy tends to the zero-point-energy at low T and to the classical value of Boltzmann constant at high T. vC k ω θ = h where
  • 16. ,T K 3R This range usually includes RT. From the figure it is seen that Cv is equal to 3R at high temperatures regardless of the substance. This fact is known as Dulong-Petit law. This law states that specific heat of a given number of atoms of any solid is independent of temperature and is the same for all materials! vC Specific heat at constant volume depends on temperature as shown in figure below. At high temperatures the value of Cv is close to 3R, where R is the universal gas constant. Since R is approximately 2 cal/K-mole, at high temperatures Cv is app. 6 cal/K-mole.
  • 17. Cv vs T for Diamond Points: Experiment Curve: Einstein Model Prediction
  • 18. Classical Theory of Heat Capacity of Solids The solid is one in which each atom is bound to its side by a harmonic force. When the solid is heated, the atoms vibrate around their sites like a set of harmonic oscillators. The average energy for a 1D oscillator is kT. Therefore, the averaga energy per atom, regarded as a 3D oscillator, is 3kT, and consequently the energy per mole is = where N is Avagadro’s number, kB is Boltzmann constant and R is the gas constant. The differentiation wrt temperature gives; 3 3BNk T RT= 23 23 3 3 6.02 10 ( / ) 1.38 10 ( / )vC R atoms mole J K− = = × × × × 24.9 ;1 0.2388 6 ( ) ( ) J Cal Cv J Cal Cv K mole K mole = = ⇒ − − ; v d C dT ε = ε
  • 19. Einstein heat capacity of solids • The theory explained by Einstein is the first quantum theory of solids. He made the simplifying assumption that all 3N vibrational modes of a 3D solid of N atoms had the same frequency, so that the whole solid had a heat capacity 3N times • In this model, the atoms are treated as independent oscillators, but the energy of the oscillators are taken quantum mechanically as This refers to an isolated oscillator, but the atomic oscillators in a solid are not isolated.They are continually exchanging their energy with their surrounding atoms. • Even this crude model gave the correct limit at high temperatures, a heat capacity of the Dulong-Petit law where R is universal gas constant. ( ) 2 2 1 T T v B e C k T e θ θ θ  =  ÷   − 3 3BNk R= ωh
  • 20. • At high temperatures, all crystalline solids have a specific heat of 6 cal/K per mole; they require 6 calories per mole to raise their temperature 1 K. •This arrangement between observation and classical theory break down if the temperature is not high. •Observations show that at room temperatures and below the specific heat of crystalline solids is not a universal constant. 6 cal Kmol Bk ωh vC T 3vC R= In each of these materials (Pb,Al, Si,and Diamond) specific heat approaches constant value asymptotically at high T. But at low T’s, the specific heat decreases towards zero which is in a complete contradiction with the above classical result.
  • 21. • Einstein model also gave correctly a specific heat tending to zero at absolute zero, but the temperature dependence near T= 0 did not agree with experiment. • Taking into account the actual distribution of vibration frequencies in a solid this discrepancy can be accounted using one dimensional model of monoatomic lattice
  • 22. Density of States According to Quantum Mechanics if a particle is constrained; • the energy of particle can only have special discrete energy values. • it cannot increase infinitely from one value to another. • it has to go up in steps. Thermal Energy & Heat Capacity Debye Model
  • 23. • These steps can be so small depending on the system that the energy can be considered as continuous. • This is the case of classical mechanics. • But on atomic scale the energy can only jump by a discrete amount from one value to another. Definite energy levels Steps get small Energy is continuous
  • 24. • In some cases, each particular energy level can be associated with more than one different state (or wavefunction ) • This energy level is said to be degenerate. • The density of states is the number of discrete states per unit energy interval, and so that the number of states between and will be . ( )ρ ε ( )dρ ε εdε ε+ε
  • 25. Effect of phonons in nanostructures  The broadening and shift of the Si and Ge Raman lines to lower frequencies as the particle size decreases has been attributed to phonon confinement effects in the nanocrystals.  Acoustic phonons of nanoparticles exhibit Brillouin scattering that depends on particle size.  Acoustic modes shift to higher frequencies with reduced particle size and optical modes shift to lower frequencies as the particle size is reduced. 
  • 26. Contd…  The temperature variation of the electrical mobility and electrical conductivity for semiconductor nanostructures:  Scattering by impurity atoms is important at low temperatures but decreases with increasing temperature.  In contrast, scattering by phonons increases with temperature, reflecting the increasing amplitude of the lattice vibrations.  The combined effect of these two processes is to give a mobility which, at low temperatures, increases with increasing temperature, followed by a decrease at high temperatures.  In certain semiconductor nanostructures it is possible to turn off the scattering by impurity atoms, resulting in very high carrier nobilities at low temperatures.