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Conductivité Optique Conductivité Optique Ricardo Lobo École Supérieure de Physique et Chimie Industrielles de la Ville de Paris [email protected] [email protected]

2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

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Page 1: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Conductivité OptiqueConductivité Optique

Ricardo Lobocar LÉcole Supérieure de Physique et Chimie Industrielles

de la Ville de Paris

[email protected]@espci.fr

Page 2: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Nichols, Phys. Rev. 1, 1 (1893)., y , ( )

Page 3: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

A few optical excitations in solidsA few optical excitations in solids

~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40 000 cm-11 eV~ 0.25 meV 2 eV 3 eV 4 eV 5 eV

~ 5 mm 1 m 500 nm 250 nm333 nmSuperconducting gap

Plasmon SemiconductorsPhonons

Molecular Vibrations (biology and chemistry)Molecular Vibrations (biology and chemistry)

Density-wave gapPolarons

Gap Semiconductors

Density-wave gap

Plasmon oxidesGap Semiconductors

Oxides Charge TransferPlasmon metals

Page 4: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

OutlineOutline

The basics of optical conductivityThe optical conductivity of metalsp y fThe f-sum rule and gapsFermi liquid signaturesFermi liquid signaturesKinetic energyPh s d h s t siti sPhonons and phase transitionsDisordered Materials

Page 5: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Preview: YBCO from an insulator to a conductorPreview: YBCO from an insulator to a conductor

1.0O7 - conducteur

0.8vi

tyO7 con uct ur

0 4

0.6

flec

tiv

0.2

0.4

Re

O6 - isolant

100 1000 100000.0

0.2

100 1000 10000

Frequency (cm-1)

Page 6: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Optical C d i i

Optical C d i iConductivity

B ildi BlConductivity

B ildi BlBuilding Blocs Building Blocs

Page 7: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Light scatteringLight scatteringSource

Black Box

Detector

Optical conductivityPhoton in Photon out

Detector

Optical conductivityHence the misnomer "center of zone" technique

B tt " t d" t h iBetter name: "momentum averaged" technique

Elastic light scattering

The interaction with the electric field dominates

Broadband (whitelight) spectroscopy

Page 8: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Maxwell Equations – The Message in the "Photon Out"

Maxwell Equations – The Message in the "Photon Out"

I Maxwell Equations in matter In vacuum

Wave with speed "c"

In matter

Ohm's law

In matter

Wave with renormalized speedPlane wave

Wave with renormalized speed

Page 9: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

The common optical functionsThe common optical functions

Refraction index: light propagation and tt tiattenuation

Dielectric function: microscopic polarizability

Optical conductivity: high-frequency electrical transport

Page 10: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Inside the Black Box – Fourier Transform Spectroscopy

Inside the Black Box – Fourier Transform Spectroscopy

Fixed mirror

Moving mirrorFellgett advantageMultiplex

Jacquinot advantageSlitless spectrometer

Nyquist theoremDiscrete FT is fine

Page 11: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

A Strange Choice for UnitsA Strange Choice for Units

W b 1/ 2 / 1Wavenumber = 1/ = 2c/ cm-1

Energy E = h = hcgy1 eV ~ 8000 cm-1

Wavelength = 1/Wavelength = 1/1 µm = 10000 cm-1

Temperature T = hc/kB10000 K ~ 7000 cm-1

Page 12: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

What else is in the black box?What else is in the black box?

I()

TR

R(ω) and T(ω) ~ |E|2

are real functions.R

Reflected Power (Real)

Kramers-Kronig, simulation; fit; R & T inversion... Other techniques using the same process:

Complex Optical Function

the same process:EllipsometryMach-ZehnderCoherent THzCoherent THz

Page 13: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Kramers-Kronig relations & the ReflectivityKramers-Kronig relations & the Reflectivity

Cauchy theorem0

Hilbert transform

Kramers-KronigCausality:Causality:

Reflectivity:

But we need R() at all energies

Page 14: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

The optical The optical conductivity in conductivity in

metals metals

Page 15: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Drude ModelDrude Model

Free electron gas

No electron-electron interactionsNo electron electron nteract ons

No electron-phonon interactions

Scattering through elastic collisions

Drude, Ann. Physik 306, 566 (1900)

Drude Modelg g

Page 16: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Drude in lightly doped SiDrude in lightly doped Si

R Re 1 Hole dopedn ~ 10-15 cm-3

Electron doped

Im 1

n ~ 4 x 10-14 cm-3

Im 1

Dressel and Scheffler, Ann. Phys. 15, 535 (2006)

Page 17: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Transparent conducting oxidesTransparent conducting oxides

0.8

1.0CdO

mis

sion

0 4

0.6

& Tr

ansm

0.2

0.4

efle

ctiv

ity &

0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.50.0R

e

Energy (eV)

Keep n small (tweak materials) Increase (improve materials) Increase (improve materials) Play with m* (create materials)

Metz et al., JACS 126, 8477 (2004), , ( )

Page 18: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Drude in metals (Silver)Drude in metals (Silver)

1.0

0.8

30000

35000

40000

0.6

efle

ctiv

ity

20000

25000

30000

-1 c

m-1]

0.4Re

0 2 5000

10000

15000

1 [

S. Biermann

0 0

0.2

0 2000 4000 6000 80000

5000

Frequency [cm-1]0

0.010000 20000 30000

Frequency [cm-1]

Frequency [cm ]

Page 19: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

But Drude fails in correlated matter…But Drude fails in correlated matter…

8000

60001/DC

4000cm-1)

2000 1 (

-1

YBCO – 100 K

0

Drude

0 500 1000 1500 2000 2500 30000

Fréquence (cm-1)

Page 20: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Ignoring the elephantIgnoring the elephant

3500.0 0.1 0.2 0.3

500

Energy [eV]

200

250

300

300

400

2000

3000m

-1]

Bi2Sr2CaCu2O8

T = 100 K

m-1]

cm-1]

50

100

150

100

200

1000

1 [-1 c

m

[

-1 c

m

1/

[c

0 50 100 150 200 250 3000

50

00 1000 2000 3000

0

Frequency [cm-1] Temperature [K]

Coherent peak described by Drude

Mid IR response

The Drude temperature dependent scattering rate

Quijada et al PRB 60 14917 (1999)

Mid-IR response simulated as Lorentz oscillators

follows the resistivity

Quijada et al., PRB 60, 14917 (1999)

Page 21: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

The optical conductivity and multiband pnictidesThe optical conductivity and multiband pnictides

0 00 0 25 0 50 0 75 1 00

Energy [eV]

60000.00 0.25 0.50 0.75 1.00

Ag (divided by 100)Bi2212 (Quijada et al)

4000Bi2212 (Quijada et. al) Ba(Fe,Co)2As2

cm-1]

2000

1 [

-10 2000 4000 6000 8000

0

Frequency [cm-1]

Singh, PRB (2008).

Frequency [cm ]

Page 22: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Multiband – pnictides DresselMultiband – pnictides Dressel

Using two Drude terms [two bands (??)] solves the problems

Wu et al., PRB 81, 100512 (2010)

Page 23: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Can we take a look at the elephant?Can we take a look at the elephant?

8000

60001/DC

4000cm-1)

2000 1 (

-1

YBCO – 100 K

0

Drude

0 500 1000 1500 2000 2500 30000

Fréquence (cm-1)

Page 24: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Patching the Drude ModelPatching the Drude ModelDrude, Ann. Physik 306, 566 (1900)

Allen, PRB 3, 305 (1971)

Drude Model Extended Drude Model

S tt i t MassScattering rate Massenhancement

"Optical self-energy"Optical self energy

Page 25: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Is this extended Drude mambo-jambo of any use?Is this extended Drude mambo-jambo of any use?

0 00 0 25 0 50 0 75 1 000 00 0 05 0 10 0 15 0 20

Energy [eV]Energy [eV]

30.00 0.25 0.50 0.75 1.000.00 0.05 0.10 0.15 0.20

1000

Bi2212 - 300 Knon Fermi liquid (ω)

Correlations

1

2

500m-1]

Bi2212 300 K

= 1

+ YBCO 100 K

0

1500

1/

[cm

Cr - 320 K

m /

m* =

Fermi liquid (ω2)

Free electron

0 2000 4000 6000 8000-1

0 500 1000 1500 20000

Fermi liquid (ω )Interband

Frequency [cm-1] Frequency [cm-1]

Basov et al., PRB 65, 054516 (2002) Puchkov et al., JPCM 8, 10049 (1996)Basov et al., PRB 65, 054516 (2002) Puchkov et al., JPCM 8, 10049 (1996)

Page 26: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

One of the multiple versions of the cuprates phase diagram

One of the multiple versions of the cuprates phase diagram

TW i d t lW i d m t l

TW i d t lW i d m t l

PsPs

Weird metalWeird metal

PsPs

Weird metalWeird metal

“F i h”t

ins.

tt in

s.

Pseudoga

Pseudoga “F i h”t

ins.

tt in

s.

Pseudoga

Pseudoga “Fermish”liquid

“Fermish”liquidM

otM

ot

gapgap “Fermish”

liquid“Fermish”

liquidMot

Mot

gapgap

SCSCAFAF SCSCSCSCSCSCAFAF

Hole concentrationHole concentration

Page 27: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

From a Nodal Metal to a Bad Metal to a Fermi Liquid

From a Nodal Metal to a Bad Metal to a Fermi Liquid

1/: Fermi liquidness increases with doping

T

ins.

ins.

Pseudo

Pseudo

Weird metalWeird metalT

ins.

ins.

Pseudo

Pseudo

Weird metalWeird metal

Hwang, Nature 427, 714 (2004)

m*: Correlations decrease with increasing dopingSCSC

“Fermish”liquid

“Fermish”liquid

AFAF

Mot

t M

ott

dogapdogap

SCSCSCSCSCSC

“Fermish”liquid

“Fermish”liquid

AFAF

Mot

t M

ott

dogapdogap

Ma, PRB 73, 144503 (2006). Hole concentrationHole concentration

Page 28: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Heavy Fermions and LF DrudeHeavy Fermions and LF Drude

300 neV 3 µeV 30 µeV

UPd2Al3

Awasthiet al. PRB 48, 10692 (1993).

Mass enhancement leads to scattering rate decrease

Dressel and Scheffler, Ann. Phys. 15, 535 (2006), ( )

Page 29: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Gaps andGaps andGaps and the sum rule

Gaps and the sum rulethe sum rule the sum rule

Page 30: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

The Optical Conductivity Sum RuleThe Optical Conductivity Sum Rule

Sum rule

1() 1()

nedT2

)(

Sum rule

mdT

0 1 2),(

Fréquence (cm-1) 0 Fréquence (cm-1) 0 q ( )q ( )

Page 31: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

The charge transfer gap of (La,Sr)2CuO4The charge transfer gap of (La,Sr)2CuO4

Uchida et al. PRB 43, 7942 (1991).

Page 32: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Density-wave like gapDensity-wave like gap

P4W14O50

CDW transition at T~140 K

CDW 1400 1 CDW gap at 1400 cm-1

Spectral weight transfer from low to high frequencies from low to h gh frequenc es

Zh l PRB 65 214519 (2002)Zhu et al., PRB 65, 214519 (2002)

Page 33: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Hidden order in URu2Si2Hidden order in URu2Si2

Phase transition at 17K to an Phase transition at 17K to an unknown order parameter

Possible renormalization of th b d t tthe band structure

Order closely related to magnetismg

Gap opening at the Fermi surface

Bonn, PRL 61, 1305 (1988)E h d k h h Even when we do not know what the crap is the gap, it still creates a spectral weight transfer

Page 34: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

And let's go superconductingAnd let's go superconducting

0 5 10 15 20

Energy [meV]

15NbN18 K

103

-1 c

m-1]

5

1 [x10

9 K

0 50 100 1500

Frequency [cm-1]

Is the sum rule violated???

Page 35: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Superconducting gap – Back to DrudeSuperconducting gap – Back to Drude

Area transfered toth ( ) functi n

1.0

b.)

the () function = 0 not accessible

to optics

The "Lost area" 0.6

0.8

vity

(arb

The Lost area gives superfluid density

0 2

0.4

Con

duct

iv

1/

0 5 10 150.0

0.2C

Energy / 2 Energy /

Page 36: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Manifestation of the superconducting gap in the infrared

Manifestation of the superconducting gap in the infrared

s-wave (Pr,Ce)2CuO4 - Tc = 21 KZimmers et al., PRB 70, 132502 (2004)

d-wave

NbN – Tc = 16.5 KSomal et al., PRL 76, 1525 (1996)

Mazin, Nature 464, 183 (2010).s-multiband

Pnictides:s ? d? Multiband?

MgB2 – Tc = 39 KPerucchi et al., PRL 89, 097001 (2002).

s±? d? Multiband?Extended s?

Page 37: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

The gap in the cupratesThe gap in the cuprates

Tc changes by a factor 3 and the thing that looks like the gap stays put ?!?!?!?!

Page 38: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Clean and DirtyClean and Dirty

Clean superconductor

0 75

1.00N

0.50

0.75

dc NS

In a clean superconductor you do

0.25

1 /

SN

In a clean superconductor you do not see the gap because there is no optical conductivity left at that frequency

0 2 4 60.00

SS

Nq y

The important feature in the optical conductivity is the determination of the superfluid

Energy / determination of the superfluid density.

The gap is a bonus!!!

Page 39: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

The gap in the cupratesThe gap in the cuprates

Tc changes by a factor 3 and the thing that looks like the gap stays put ?!?!?!?!Yep! Cause it ain't the gap, stupid!!

Page 40: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Pnictides Gap ReviewPnictides Gap Review

Claim: 2 gap BCS H t l Xi 0912 0636 1van Heuman et al., arXiv:0912.0636v1

Claim: Good agreement with s-wave BCSGorshunov et al., PRB 81, 060509 (2010)

Claim: 3 gap BCSKim et al., arXiv:0912.0140

Page 41: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

s ± gap: Interband scattering is pair breakings± gap: Interband scattering is pair breaking

Interband scattering annihilates Cooper pairsp p

Residual Drude peak in the superconducting state

Lobo et al (2010)Lobo et al. (2010)

Page 42: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

The infamous The infamous cuprate

dcuprate

dpseudogap pseudogap

Page 43: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

The pseudogapThe pseudogapT

. PsPs

Weird metalWeird metalT

. PsPs

Weird metalWeird metal

“Fermish”liquid

“Fermish”liquidM

ott

ins.

Mot

t in

s .

Pseudogap

Pseudogap “Fermish”liquid

“Fermish”liquidM

ott

ins.

Mot

t in

s .

Pseudogap

Pseudogap

SCSC

Hole concentration

liquidliquidAFAF SCSCSCSCSCSC

Hole concentration

liquidliquidAFAF

Nd2-xCexCuO4Bi-2212

95 K

Alloul, PRL 63, 1700 (1989)Hole concentrationHole concentration

120 K

95 K

Armitage et al PRL 81 257001 (2002) Norman et al. Nature 392, 157 (1998).

180 K

Armitage et al. PRL 81, 257001 (2002). , ( )

Page 44: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

Restricted Spectral Weight or Partial Sum RuleRestricted Spectral Weight or Partial Sum Rule

nedT2

0 1 2),(

Sum rule

m0 2

1() 1()

Restricted spectral i ht

W (T)

[0, 2.5/2 cm-1]W (300K)

weight

1.3

1 15

[ , 2 ]

dTW c

c )(),,0(0 1

1.15

1

0 50 100 150 200 250 300

TempératureFréquence (cm-1) 0 Fréquence (cm-1) 0

c

Page 45: 2010 06 10 Aussois Optics Lobo.ppt [Mode de …gdr-mico.cnrs.fr/UserFiles/file/Ecole/lobo_mico.pdfA few optical excitations in solids ~ 2 cm-1 10 000 cm-1 20 000 cm-1 30 000 cm-1 40

The Sum Rule when a Gap OpensThe Sum Rule when a Gap Opens

Ec0 8

1.0

Wei

ght

0.6

0.8

uctiv

ity

Spec

tral

W

0.4Con

du

S

0.0

0.2

Temperature0.0 0.2 0.4 0.6 0.8 1.0

Energy

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(Pr,Ce)2CuO4 - A well behaved normal state (pseudo) gap

(Pr,Ce)2CuO4 - A well behaved normal state (pseudo) gap

Energy [eV]

0.00 0.25 0.50 0.75

3 Pr2-xCexCuO4

Energy [eV]

Partial Sum Rule

2 25 K 300 K

1 ]

1.8

H,3

00K) 0-500 cm-1

0.17

0

1

x 10

3 -1cm

-1

1.4

1.6

/ RSW

(L,

(a)0.15

0

1[x

1.2

W (

L,H,T

) /

0.13

0

0 2000 4000 60000

(b) 0 100 200 300

1.0

RSW

Temperature (K)

Zimmers et al EPL 70 225 (2005)

Wavenumber [cm-1]

Zimmers et al., EPL 70, 225 (2005).

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Bi-2212 – Where is the pseudogap?Bi-2212 – Where is the pseudogap?

6 80 K

Optical conductivity Partial sum rule

T 70 K 7 7

4

6 80 K 150 K 250 K

Tc = 70 K

Bi2Sr2CaCu2O8+δ7.6

7.7

cm

)

Over Tc = 63K Under Tc = 70KOver T = 67K

0

2

3 -1

cm

-1]

2 2 2 8+δ

7.5

ht (

106

.c Over Tc 67K

Under Tc = 66K

1 [103

491 K 143 K 300 K

Tc = 86 K

7.3

7.4

Santander-Syro et al PRL '02ectra

l wei

gh0 500 1000 1500

0

2

50 100 150 200 250 3007.2

Santander Syro et al., PRL 02 Molegraaf et al., Science '02Sp

eT (K)0 500 1000 1500

Frequency (cm-1)

Santander Syro et al PRL 88 097005(2002)

Temperature (K)

Santander-Syro et al., PRL 88, 097005(2002).

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Why the difference?Why the difference?

The ab-plane optical probes mostly the nodal ( ) directions() directions

Bi-221295 K

120 K

95 K

(La,Sr)2CuO4

Armitage et al PRL 81 257001 (2002)

Nd2-xCexCuO4

Norman et al. Nature 392, 157 (1998).

180 K

Armitage et al. PRL 81, 257001 (2002). , ( )

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The pseudogap in the scattering rateThe pseudogap in the scattering rate

2500.0 0.1 0.2 0.3

3

Energy [eV]

200

(b)

K]

Bi2223

1

2

3

300 K(a)

200 K

100

150

pera

ture

[K

Bi22120

0

1

x103 c

m-1]

1

150 K

73 K

50

100

Tem

p

Bi2201

1 /

[x

0

1

20 K

0

1

73 K

0.1 0.2 0.30

Bi2212 - UD - Tc = 67 K

0 1000 2000 30000

1

0

Doping

Lobo et al. (2009)

Frequency [cm-1]

Hwang et al., Nature 427, 714 (2004)

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The pseudogap along the c-axis of YBCO (Tc = 63 K)

The pseudogap along the c-axis of YBCO (Tc = 63 K)

Spectral weight decrease

Knight shift

Homes et al., PRL 71, 1645 (1993).Homes et al., RL 7 , 6 5 ( 993).

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AND NOW FOR SOMETHING AND NOW FOR SOMETHING AND NOW FOR SOMETHING COMPLETELY DIFFERENT

AND NOW FOR SOMETHING COMPLETELY DIFFERENT

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Light and Matter interaction in an Insulator

Light and Matter interaction in an Insulatorin an Insulatorin an Insulator

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Phonons and the Harmonic ApproximationPhonons and the Harmonic Approximation

And for many phonons

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Phonons & the f-sum rulePhonons & the f-sum rule

The f-sum rule (particle conservation):

The f-sum rule for phonons:

The f-sum rule for decoupled phonons:

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Soft Mode & Phase TransitionsSoft Mode & Phase TransitionsQ is a dynamic variable of the system

Order parameter = < Q > = 0, T > Tc 0 T T

Order parameter Q ≠ 0, T < Tc

<Q>Energie libre QgT > Tc

TTc

T ~ Tc

T < Tc

= < Q0 > (paramètre d’ordre)

c

TT

Q (variable dynamique)

TTc

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SrTiO3 – A wannabe ferroelectricSrTiO3 – A wannabe ferroelectric

1001.0

60

80

m-1)

0.6

0.8

vity

20

40

WTO

(1) (

c

0.4

0.6

Ref

lect

i

20 K 180 K 250 K 300 K

0 50 100 150 200 250 3000

20W

Temperature0 200 400 600 800

0.0

0.2

F ( -1) TemperatureFrequency (cm )

Incipient soft mode driven f l ferroelectric transition

TC ~ -15 K

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Soft mode and FerroelectricsSoft mode and Ferroelectrics

BaTiO3100

Vogt et al, PRB 1982.

m-1)

50

(c

m

Merz, PR 91, 513 (1953)0300 500 700300 500 700

T(K)

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The Multiferroic Materials TotemThe Multiferroic Materials Totem

Coexistence of at least two ferroic orders [ferromagnetic,

P

ferroelectric, ferroelastic, ferrotoroidal (??)] *

P

F l t iMagnetoelectricsPiezoelectrics

Schmid, Ferroelectrics 162, 317 (1994).

Ferroelectric

FerromagneticFerroelastic

Magnetostriction

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Magneto-electric MultiferroicsMagneto-electric MultiferroicsEerenstein et al., Nature 442, 759 (2006).

Multiferroics

FM FEMagnetoelectricsMagnetoelectric

Magnetict i l

Electricl

Multiferroics(Control of either

polarization materials materials

pby either field)

*antiferromagnets also accepted.

Small coupling – 4 state memory Large coupling – “E” write / “M” read

also accepted.

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Ying & YangYing & YangFerroelectricity & Magnetism coexist

Magnetism causes Ferroelectricity

BiFeO3Large moments High temperature transitions

TbMnO3Small momentsLow temperaturesHigh temperature transitions

Weak couplingmp

Strong coupling

Lebeugle et al. APL 2007 Kimura, Nature 2003

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Yang (TbMnO3) is more fun!Yang (TbMnO3) is more fun!

Kimura Nature 2003Kimura, Nature 2003.

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TbMnO3 Phonon Spectra (T = 5 K)TbMnO3 Phonon Spectra (T = 5 K)

0.8

1.0

115

116

117

E // a

0.4

0.6

112

113

114

204

cm-1)

0.0

0.2

vity

E // a

0.4201

202

203

est T

O m

ode

(c

E // b

Ref

lect

iv

0 0

0.2

E // b199

200

201

eque

ncy

of lo

we

168

0.0

0.2

0.4

E // c

Fre

165

166

167

168

0 200 400 600 800 10000.0

Frequency (cm-1)

E // c

0 50 100 150 200 250 300

164

165

Temperature (K)

E // c

q y ( )

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So, where is the action?So, where is the action?

Pimenov et al., Nat. Phys, 2006.

M ti it ti

Senff et al. PRL 2007

Magnetic excitation

Activated by electric field of light only

Suppressed by an external magnetic field Suppressed by an external magnetic field

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Magnons and PhononsMagnons and Phonons

Stronger electromagnon at 60 cm-1 coupled to phonon at 110 cm-1

Takahashi et al PRL 101 187201 (2008)

Stronger electromagnon at 60 cm coupled to phonon at 110 cm

Takahashi et al. PRL 101, 187201 (2008)

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Phonon and magnon optical responsePhonon and magnon optical response

1 0 0 6

0.8

1.0

TbMnO3 E // a

0 4

0.5

0.6

n

50K 25K5K

0.4

0.6

flect

ivity

0.3

0.4

smis

sion 5K

simulation 5K

0.2

Ref

6.5 K 60 K 0.1

0.2

Tran

s

0 50 100 150 200 2500.0

Wavenumber (cm-1)

0 50 100 150 2000.0

Wavenumber (cm-1)( )

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Phonon spectral weigthsPhonon spectral weigths

2 )

100 1 2 3

1 0

K) (

1 cm2

-100

0

0.8

1.0

E // aT = 5K

100

200

T)-W

(60K

4 7 5 86 9

0 4

0.6

efle

ctiv

ity

T 5K

0

100

(T) =

W(T 6 9

0.2

0.4Re

-200

-100

W (

0 200 400 600 800 10000.0

Frequency (cm-1)

0 20 40 60Temperature (K)

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The electromagnon is built from two phononsThe electromagnon is built from two phonons

200

0

100

-1cm

-2)

All phonons MagnonPhonons 1 & 3

200

-100

T)-W

(50K

) ( Phonons 1 & 3

-300

-200

W (T

) = W

(T TNTC

0 10 20 30 40 50 60-500

-400W

0 10 20 30 40 50 60Temperature (K)

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DiSordEredDiSordEredDiSordEred MEdiA

DiSordEred MEdiAMEdiAMEdiA

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Disorder in (Y,Pr)Ba2Cu3O7Disorder in (Y,Pr)Ba2Cu3O7

8000

(P Y )B C O

4000

6000 (PrxY1-x)Ba2Cu3O7

100 K

)

2000

4000

x = 0 0-1cm

-1

Pr is an underdoping agent

Empties CuO2 planes

0

40 K x = 0 4

x = 0.0

1 ( p p

Localizes charges along chains

0

040 K

50 K

x 0.4

x = 0.50 500 1000 1500

0

Frequency (cm-1)Lobo et al. PRB 65, 104509 (2002).

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Effective Medium TheoriesEffective Medium Theories

Gold evaporated onto hot (600K)

hi b t tsapphire substrates

Cranberry glass (Ruby gold glass)Cranberry glass (Ruby gold glass)

Maxwell-Garnett Theory

insul.

metal

J. C. Maxwell Garnett, Colours in Metal Glasses and in Metallic Films Philos Trans R Soc 203 385 (1904) Metallic Films, Philos. Trans. R. Soc. 203, 385 (1904).

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Superconducting MoGe: Field Dependent Transmission

Superconducting MoGe: Field Dependent TransmissionTransmissionTransmission

2.0

K)

Far IR

1.5

K,H

)/T(8

B

1.0atio

T(3

K

0 5ssio

n R

a

0 T 6 T 1 T 7 T 2 T 8 T3 T 9 T0.5

Tran

smi 3 T 9 T

4 T 10 T 5 T

10 20 30 400.0

T

Frequency [cm-1]Frequency [cm ]

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S d t2.5

Br ggeman

Effective Medium Models for a Superconductor with Vortices

Effective Medium Models for a Superconductor with Vortices

1.5

2.0

Superconductor& Normal metalin parallel

o T S(

f)/T N

1 5

2.0

BruggemanEffective MediumApproximation

T S(f)/T

N

0.5

1.0

Tran

smis

sion

Rat

io

= f +(1 f ) 1.0

1.5

smis

sion

Rat

io

10 20 300.0

0.5T

Frequency [cm-1]

= f N+(1-f ) S

0 10 20 300.0

0.5

Tran

s

super

normal

Frequency [cm-1]

2.0

2.5Garnett TheoryNormal withSuperconductinginclusions

f)/T N

1.0

1.5

mis

sion

Rat

io T

S(f

0 10 20 300.0

0.5Tran

sm super

normal

Frequency [cm-1]

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Effective Medium Models for a Superconductor with Vortices

Effective Medium Models for a Superconductor with Vortices

2.5

Garnett TheorySuperconductor

/ N l i l i2.0 w/ Normal inclusionsT S(

f)/T N

1.5

on R

atio

T

1.0

ansm

issi

o

super0.5Tr

a super

normal

10 20 300.0

Frequency [cm-1]Frequency [cm ]

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SummarySummary1 01 0

0.6

0.8

1.0

ctiv

ity

O7 - conducteur

0.6

0.8

1.0

ctiv

ity

O7 - conducteur Optics is mostly an electrical measurement

Momentum averaged technique 0.2

0.4

Refl

ec

O6 - isolant0.2

0.4

Refl

ec

O6 - isolant

measurement

100 1000 100000.0

Frequency (cm-1)

100 1000 100000.0

Frequency (cm-1)

The optical conductivity specgtral weight is always conservedalways conserved

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RappelsRappels

Technique moyennée en impulsionq y pMesure de la conductivité électrique aux hautes

fréquencesf q Pic à fréquence nulle = charge mobile Pic à fréquence finie charge localisée Pic à fréquence finie = charge localiséeAccès aux états électroniques et à leur distribution

é ien énergieRègle de somme de la conductivité