classical theory expectations

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© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips Classical Theory Expectations Equipartition: 1/2k B T per degree of freedom In 3-D electron gas this means 3/2k B T per electron In 3-D atomic lattice this means 3k B T per atom (why?) So one would expect: C V = du/dT = 3/2n e k B + 3n a k B Dulong & Petit (1819!) had found the heat capacity per mole for most solids approaches 3N A k B at high T 1 Molar heat capacity @ high T 25 J/mol/K

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Classical Theory Expectations. Equipartition : 1/2k B T per degree of freedom In 3-D electron gas this means 3/2k B T per electron In 3-D atomic lattice this means 3k B T per atom (why?) So one would expect: C V = du/ dT = 3/2n e k B + 3n a k B - PowerPoint PPT Presentation

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Page 1: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 1

Classical Theory Expectations

• Equipartition: 1/2kBT per degree of freedom

• In 3-D electron gas this means 3/2kBT per electron

• In 3-D atomic lattice this means 3kBT per atom (why?)

• So one would expect: CV = du/dT = 3/2nekB + 3nakB

• Dulong & Petit (1819!) had found the heat capacity per mole for most solids approaches 3NAkB at high T

Molar heat capacity @ high T 25 J/mol/K

Page 2: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 2

Heat Capacity: Real Metals

• So far we’ve learned about heat capacity of electron gas• But evidence of linear ~T dependence only at very low T• Otherwise CV = constant (very high T), or ~T3 (intermediate)• Why?

Cv = bT

3VC bT aT

due toelectron gas

due toatomic lattice

Page 3: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 3

Heat Capacity: Dielectrics vs. Metals

• Very high T: CV = 3nkB (constant) both dielectrics & metals

• Intermediate T: CV ~ aT3 both dielectrics & metals

• Very low T: CV ~ bT metals only (electron contribution)

Cv = bT

Page 4: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 4

Phonons: Atomic Lattice Vibrations

• Phonons = quantized atomic lattice vibrations ~ elastic waves

• Transverse (u ^ k) vs. longitudinal modes (u || k), acoustic vs. optical

• “Hot phonons” = highly occupied modes above room temperature

CO2 moleculevibrations

)](exp[),( tiit rkAru

transversesmall k

transversemax k=2p/a

k

Graphene Phonons [100]

200 meV

160 meV

100 meV

26 meV =300 K

Freq

uenc

y ω

(cm

-1)

~63 meVSi opticalphonons

Page 5: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 5

A Few Lattice Types• Point lattice (Bravais)

– 1D

– 2D

– 3D

Page 6: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 6

Primitive Cell and Lattice Vectors

• Lattice = regular array of points Rl in space repeatable by translation through primitive lattice vectors

• The vectors ai are all primitive lattice vectors

• Primitive cell: Wigner-Seitz

Page 7: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 7

Silicon (Diamond) Lattice

• Tetrahedral bond arrangement• 2-atom basis• Each atom has 4 nearest neighbors and 12 next-nearest

neighbors• What about in (Fourier-transformed) k-space?

Page 8: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 8

Position Momentum (k-) Space

• The Fourier transform in k-space is also a lattice• This reciprocal lattice has a lattice constant 2π/a

k

Sa(k)

Page 9: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 9

Atomic Potentials and Vibrations

• Within small perturbations from their equilibrium positions, atomic potentials are nearly quadratic

• Can think of them (simplistically) as masses connected by springs!

Page 10: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 10

Vibrations in a Discrete 1D Lattice

• Can write down wave equation• Velocity of sound (vibration

propagation) is proportional to stiffness and inversely to mass (inertia)

Freq

uenc

y,

Wave vector, K0 p/a

2 2

2 2x x

Yu uEt x

2 2

2 2 2

1x x

s

u ux v t

Y

sEv

sv k See C. Kittel, Ch. 4or G. Chen Ch. 3

Page 11: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 11

Two Atoms per Unit Cell

Lattice Constant, a

xn ynyn-1 xn+1

2

1 12

2

2 12

2

2

nn n n

nn n n

d xm k y y xdtd ym k x x ydt

Fr

eque

ncy,

Wave vector, K0 p/a

LATA

LOTO

OpticalVibrational

Modes

Page 12: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 12

Energy Stored in These Vibrations

• Heat capacity of an atomic lattice• C = du/dT =

• Classically, recall C = 3Nk, but only at high temperature• At low temperature, experimentally C 0• Einstein model (1907)

– All oscillators at same, identical frequency (ω = ωE)

• Debye model (1912)– Oscillators have linear frequency distribution (ω = vsk)

Page 13: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 13

The Einstein Model

• All N oscillators same frequency• Density of states in ω

(energy/freq) is a delta function

• Einstein specific heat

Freq

uenc

y,

0 2p/a

E

Wave vector, k (3 )Eg N

( )E

du dfC g ddT dT

Page 14: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 14

Einstein Low-T and High-T Behavior

• High-T (correct, recover Dulong-Petit):

• Low-T (incorrect, drops too fast)

2

2

1( ) 3 3

1 1

E

E

E

TE B BT

T

C T Nk Nk

/2

2/

2 /

( ) 3

3

E BE

BE B

E E B

B

k T

E B k T k T

k TB k T

eC T Nke

Nk e

Einstein modelOK for optical phonon

heat capacity

Page 15: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 15

The Debye Model• Linear (no) dispersion

with frequency cutoff• Density of states in 3D:

(for one polarization, e.g. LA)(also assumed isotropic solid, same vs in 3D)

• N acoustic phonon modes up to ωD

• Or, in terms of Debye temperature

Freq

uenc

y,

0

sv k

Wave vector, k 2p/a

2

2 32 s

gv

p

kD roughly corresponds to max lattice wave vector (2π/a)

ωD roughly corresponds tomax acoustic phonon frequency

1/326sD

B

v Nk

p

Page 16: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 16

Annalen der Physik 39(4)p. 789 (1912)

Peter Debye (1884-1966)

Page 17: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 17

Website Reminder

Page 18: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 18

The Debye Integral• Total energy

• Multiply by 3 if assuming all polarizations identical (one LA, and 2 TA)

• Or treat each one separately with its own (vs,ωD) and add them all up

• C = du/dTFr

eque

ncy,

0 Wave vector, k 2p/a

sv k

0

( ) ( ) ( )D

u T f g d

3 / 4

20

( ) 9( 1)

D T x

D B xD

T x e dxC T Nke

people like to write:(note, includes 3x)

Page 19: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 19

Debye Model at Low- and High-T• At low-T (< θD/10):

• At high-T: (> 0.8 θD)

• “Universal” behavior for all solids

• In practice: θD ~ fitting parameter to heat capacity data

• θD is related to “stiffness” of solid as expected

3412( )5D B

D

TC T Nkp

( ) 3D BC T Nk

Page 20: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 20

Experimental Specific Heat

10 410 310 210 110 1

10 2

10 3

10 4

10 5

10 6

10 7

Temperature, T (K)

Spec

ific

Hea

t, C

(J/

m -

K)3

C T 3

C 3kB 4.7106 Jm3 K

D 1860 K

Diamond

ClassicalRegime

Each atom has a thermal energy of 3KBT

Spec

ific

Heat

(J/m

3 -K)

Temperature (K)

C T3

3NkBT

Diamond

In general, when T << θD 1,d d

L Lu T C T

Page 21: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 21

Phonon Dispersion in Graphene

Maultzsch et al., Phys. Rev. Lett. 92, 075501 (2004) Optical

Phonons

Yanagisawa et al.,Surf. Interf. Analysis37, 133 (2005)

Page 22: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 22

Heat Capacity and Phonon Dispersion• Debye model is just a simple, elastic, isotropic approximation; be

careful when you apply it

• To be “right” one has to integrate over phonon dispersion ω(k), along all crystal directions

• See, e.g. http://www.physics.cornell.edu/sss/debye/debye.html

Page 23: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 23

Thermal Conductivity of Solids

how do we explain the variation?thermal conductivity spans ~105x(electrical conductivity spans >1020x)

Page 24: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 24

Kinetic Theory of Energy Transport

z

z - z

z + z

u(z-z)

u(z+z) λqz zzzz zuzuvq

21'

Net Energy Flux / # of Molecules

2' cosz z zdu duq v vdz dz

through Taylor expansion of u

13z

du dT dTq v kdT dz dz

Integration over all the solid angles total energy flux

13

k CvThermal conductivity:

Page 25: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 25

Simple Kinetic Theory Assumptions

• Valid for particles (“beans” or “mosquitoes”)– Cannot handle wave effects (interference, diffraction, tunneling)

• Based on BTE and RTA• Assumes local thermodynamic equilibrium: u = u(T)• Breaks down when L ~ _______ and t ~ _________• Assumes single particle velocity and mean free path

– But we can write it a bit more carefully:

Page 26: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 26

l

Temperature, T/D

Boundary

PhononScattering

Defect

Decreasing Boundary Separation

IncreasingDefectConcentration

0.01 0.1 1.0

Phonon MFP and Scattering Time• Group velocity only depends on dispersion ω(k)• Phonon scattering mechanisms

– Boundary scattering– Defect and dislocation scattering– Phonon-phonon scattering

21 13 3

k Cv Cv

Temperature, T/D

0.01 0.1 1.00.01 0.1 1.0

kl

dl Tk

Boundary

PhononScatteringDefect

Increasing DefectConcentration

Page 27: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 27

Temperature Dependence of Phonon KTH

C λ

low T Td

nph 0, soλ , but then

λ D (size) Td

high T 3NkB 1/T 1/T

C /1 1kTph ph

ph

en

3

d

B

T low TNk high T

Thigh

kT

Tlow

Page 28: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 28

Ex: Silicon Film Thermal Conductivity

Bulk single-crystal silicon:Touloukian et al. (1970)d = 0.44 cm

singlecrystal

110 100Temperature (K)

10

100

1000

Ther

mal

Con

duct

ivity

(W m

-1K

-1)

104

bulk

1

21

31),(

i

GG nA

dACvndk

Doped polysilicon film:McConnell et al. (2001)d = 1 mmdg = 350 nmn = 1.6·1019 cm-3 boron

Undoped polysilicon film:Srinivasan et al. (2001)d = 1 mmdg = 200 nm

undoped poly-crystal

doped

films

undoped

doped

Undoped single-crystal film:Asheghi et al. (1998)d = 3 mm

Doped single-crystal film:Asheghi et al. (1999)d = 3 mmn = 1·1019 cm-3 boron

McConnell, Srinivasan, and Goodson, JMEMS 10, 360-369 (2001)

sizeeffect

Page 29: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 29

Ex: Silicon Nanowire Thermal Conductivity

• Recall, undoped bulk crystalline silicon k ~ 150 W/m/K (previous slide)

Li, Appl. Phys. Lett. 83, 2934 (2003)

Nanowire diameter

Page 30: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 30

Ex: Isotope Scattering

~T3

~1/T

isotope~impurity

Page 31: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 31

Why the Variation in Kth?• A: Phonon λ(ω) and dimensionality (D.O.S.)• Do C and v change in nanostructures? (1D or 2D)• Several mechanisms contribute to scattering

– Impurity mass-difference scattering

– Boundary & grain boundary scattering

– Phonon-phonon scattering

224

2

14

i

ph i s

nV Mv M

p

1 s

ph b

vD

1 expph ph B

A T Bk T

Page 32: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 32

Surface Roughness Scattering in NWsWhat if you have really rough nanowires?• Surface roughness Δ ~ several nm!• Thermal conductivity scales as ~ (D/Δ)2• Can be as low as that of a-SiO2 (!) for very rough

Si nanowires

smooth Δ=1-3 Å

rough Δ=3-3.25 nm

Page 33: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 33

Data and Model From…

Data…

Model…(Hot Chips

class project)

Page 34: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 34

What About Electron Thermal Conductivity?

• Recall electron heat capacity

• Electron thermal conductivity

0

edu dfC E g E dEdT dT

2

2B

e e BF

k TC n kE

p

at most Tin 3D

ek Mean scattering time: e = _______

e

Temperature, T

Defect Scattering

PhononScattering

IncreasingDefect Concentration

Bulk Solidse

Electron Scattering Mechanisms

Grain Grain Boundary

• Defect or impurity scattering• Phonon scattering• Boundary scattering (film

thickness, grain boundary)

Page 35: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 35

Ex: Thermal Conductivity of Cu and Al• Electrons dominate k in metals

10 310 210 110 010 0

10 1

10 2

10 3

Temperature, T [K

Ther

mal

Con

duct

ivity

, k [

W/c

m-K

]

Copper

Aluminum

Defect Scattering Phonon Scattering

11

Matthiessen Rule:1 1 1 1

1 1 1 1e defect boundary phonon

e defect boundary phonon

Page 36: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 36

Wiedemann-Franz Law

• Wiedemann & Franz (1853) empirically saw ke/σ = const(T)

• Lorenz (1872) noted ke/σ proportional to T

22 21

3 2e B FF

Tk n vE

p

FE where

2qq n nm m recall electrical

conductivity

taking the ratio ek

Page 37: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 37

Lorenz Number

This is remarkable!It is independent of n, m, and even !

2 2

23e BkLT q p

L = /T 10-8 WΩ/K2

Metal 0 ° C 100 °C

Cu 2.23 2.33

Ag 2.31 2.37

Au 2.35 2.40

Zn 2.31 2.33

Cd 2.42 2.43

Mo 2.61 2.79

Pb 2.47 2.56

8 22.45 10 WΩ/KL

Agreement with experiment is quite good, although L ~ 10x lower when T ~ 10 K… why?!

Experimentally

Page 38: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 38

Amorphous Material Thermal Conductivity

Amorphous (semi)metals: bothelectrons & phonons contribute Amorphous dielectrics:

K saturates at high T (why?)

a-Si

a-SiO2

GeTe

Page 39: Classical Theory Expectations

© 2010 Eric Pop, UIUC ECE 598EP: Hot Chips 39

Summary

• Phonons dominate heat conduction in dielectrics• Electrons dominate heat conduction in metals

(but not always! when not?!)

• Generally, C = Ce + Cp and k = ke + kp

• For C: remember T dependence in “d” dimensions• For k: remember system size, carrier λ’s (Matthiessen)

• In metals, use WFL as rule of thumb