Thermomagnetic properties of the strongly correlated semimetal - - PowerPoint PPT Presentation

thermomagnetic properties of the strongly correlated
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Thermomagnetic properties of the strongly correlated semimetal - - PowerPoint PPT Presentation

MAX-PLANCK-INSTITUT FR CHEMISCHE PHYSIK FESTER STOFFE Thermomagnetic properties of the strongly correlated semimetal CeNiSn Niels Oeschler Max Planck Institute for Chemical Physics of Solids, Dresden, Germany MAX-PLANCK-INSTITUT FR


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SLIDE 1

Thermomagnetic properties

  • f the strongly correlated semimetal

CeNiSn

Niels Oeschler

Max Planck Institute for Chemical Physics of Solids, Dresden, Germany

MAX-PLANCK-INSTITUT

FÜR CHEMISCHE PHYSIK FESTER STOFFE

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SLIDE 2

Acknowledgements:

Measurements:

  • U. Köhler, MPI CPfS, Dresden, Germany
  • P. Sun, MPI CPfS, Dresden, Germany
  • S. Paschen, Vienna University of Technology, Austria
  • F. Steglich, MPI CPfS, Dresden, Germany

Samples:

  • T. Takabatake, Hiroshima University, Japan

MAX-PLANCK-INSTITUT

FÜR CHEMISCHE PHYSIK FESTER STOFFE

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SLIDE 3

Outline

Introduction

  • Thermoel. and thermomagn. effects
  • Exp. setup

Correlated semimetal CeNiSn

Results

Resistivity and Hall effect Thermopower Nernst effect and Righi-Leduc effect

Discussion

Field-dependent thermopower Nernst effect

Summary

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SLIDE 4

Introduction

  • Thermoel. and thermomagn. Effects

Charge transport: J = σE - σSΔT Heat transport: JQ = σSTE - κΔT Thermal conductivity: κ = JQ/ΔTx Thermopower: S = -Ux/ΔTx

x y z JQ heater bath B

ΔTx Ux

slide-5
SLIDE 5

Introduction

  • Thermoel. and thermomagn. Effects

Charge transport: J = σE - σSΔT Heat transport: JQ = σSTE - κΔT Thermal conductivity: κ = JQ/ΔTx Thermopower: S = -Ux/ΔTx Nernst effect: ν = -Uy/ΔTxB Righi-Leduc effect: L = -κy/B ΔTy/ΔTx

x y z JQ heater bath B

Uy ΔTy

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SLIDE 6

Introduction

  • Thermomagn. Effects: Ettingshausen cooling

j B

source/hot sink/cold

ΔT

Lc Lh

j B infinite stage Ettingshausen device

α

⎟ ⎟ ⎠ ⎞ ⎜ ⎜ ⎝ ⎛ − = Δ

h c hot max

1 L L T T

2

2 cold mag max

T Z T = Δ κ υ σ T B T Z

2 mag

) ( =

  • Thermomagn. figure of merit ZmagT
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SLIDE 7

Kondo Insulator

2π/a E k N(E) EF EF

unperturbed conduction band unperturbed 4f band hybridized bands

2π/a E k

(a) (d) (c) (b)

N(E)

Heavy fermion metals

  • ρ ~ -lnT at T ≈ TK
  • enhanced DOS at EF below ~TK

metal-like behavior at low T Kondo insulator

  • ρ ~ -lnT at T ≈ TK
  • gap below ~Tg

insulating behavior at low T

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SLIDE 8

Introduction

Experimental Setup:

4He cryostat

horizontal 7T magnet

  • ptimized for small samples with

low κ ΔT: chromel-AuFe thermocouples U: copper wires, nanovoltmeter

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SLIDE 9

CeNiSn

samples

  • rthorhombic crystal structure

chains of Cerium ions along a easy a axis Czochralski method annealed by SSE energy scales crystal field levels: kBΔCEF ≈ 230K, 460K Kondo temp.: TK ≈ 56 K pseudogap Δ/kB ≈ 10 K below T ≈ 10 K no ordering down to 25 mK

c a b Ce Ni Sn c b a

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SLIDE 10

CeNiSn

gap structure

pseudogap opens around 10K residual states at EF metallic ρ, large Sommerfeld coeff.

gap suppression

  • magnetic fields ~10 T // a
  • pressure ~ 2 GPa
  • substitution (Ce/La and Ni/Cu,Co) ~ 10 %

dI/dV

  • T. Ekino et al., Phys. Rev. Lett. 75, 4262 (1995)
  • K. Izawa et al., J. Phys. Soc. Jpn. 65, 3119 (1996)

V (mV)

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SLIDE 11

CeNiSn - Kondo Insulator?

  • G. Nakamoto et al., J. Phys. Soc. Jpn. 64(12), 4834 (1995)

sensitive dependence on sample purity (ρ, MR, RH) residual DOS near EF (NMR, cP, ρ, κ)

⇒ CeNiSn – Kondo semimetal

  • K. Izawa et al., J. Phys. Soc. Jpn. 65, 3119 (1996)
  • H. Ikeda and K. Miyake, J. Phys. Soc. Jpn. 65, 1769 (1996)
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SLIDE 12

Experimental

Single crystals (#5)

  • Czochralski + SSE
  • best available samples
  • Orientation: Laue, χ, ρ (a/c)
  • ca. 4 x 4 x 0.8 mm³
  • Measurements: q // b; B // a, c

Measurements:

  • Thermal conductivity
  • Thermopower at +B and –B
  • Nernst effect
  • Thermal Hall effect

1.5 5 10 50 50 100 150 200

0 T 1 T 2 T 4 T 7 T

ρ (μΩ cm)

T (K)

CeNiSn No.3 j // b, B // a

  • G. Nakamoto et al., J. Phys. Soc. Jpn. 64(12), 4834 (1995)
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SLIDE 13

Results: Thermopower

1.5 5 10 50 100

  • 40
  • 20

20 40

sample No 1 sample No 3

CeNiSn #5 B = 0 T q//b S (µV/K) T (K)

  • Kondo system with CEF splitting
  • largest negative S ever observed
  • very precise orientation !

CeNiSn #4

  • G. Nakamoto et al., Physica B 306 & 307, 840 (1995)

S (µV/K) 60 40 20 T (K)

0 10 20 30 40

b-axis

  • J. Sakurai et al., Physica B 306 & 307, 834 (1995)

CeNiSn type unknown

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SLIDE 14

Field-dep. Thermopower

1.5 2 3 4 5 6 7 89 10 20 30 40

  • 40
  • 20

20 40 CeNiSn #5, No. 3 q//b, B//a

0 T 1 T 2 T 4 T 7 T

S (µV/K) T (K)

B // a: - enhanced values of |S|

  • shift of the minimum to lower T

B // c:

  • similar, but less pronounced

literature:

  • strong sample

dependence at low T

  • no comparable results

in field

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SLIDE 15

Nernst effect

large values of N below 10 K (opening of the gap)

  • scaling for B // a (easy axis!)
  • shift of minimum for B // c

q // b, B // a B // c

1.5 5 10 50

  • 120
  • 100
  • 80
  • 60
  • 40
  • 20

2 4 6 8 10

  • 20
  • 15
  • 10
  • 5

4 T 7 T 0.5 T 1 T 2 T

N (µV/K) T (K)

ν (µV/KT)

T (K)

1.5 5 10 50

  • 120
  • 100
  • 80
  • 60
  • 40
  • 20

2 4 6 8 10

  • 15
  • 10
  • 5

5.5 T 7 T 1 T 2 T 3 T

N (µV/K) T (K)

ν (µV/KT)

T (K)

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SLIDE 16

Discussion: Thermopower

2 4 6 8 10

  • 40
  • 30
  • 20
  • 10

10 Ulong/ΔT T (K) + 2 T

  • 2 T

variation due to

  • sample dependence
  • misorientation
  • non-negligible Nernst contribution
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SLIDE 17

Discussion: Thermopower

2 4 6 8 10

  • 40
  • 30
  • 20
  • 10

10 Ulong/ΔT T (K) + 2 T

  • 2 T

variation due to

  • sample dependence
  • misorientation
  • non-negligible Nernst contribution

2 4 6 8 10

  • 40
  • 30
  • 20
  • 10

Ulong/ΔT T (K) (U+-U-)/(2ΔT) N(2T)

(U+-U-)/2ΔT N (2T)

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SLIDE 18

Discussion: Thermopower

2 4 6 8 10

  • 40
  • 30
  • 20
  • 10

10 Ulong/ΔT T (K) + 2 T

  • 2 T

variation due to

  • sample dependence
  • misorientation
  • non-negligible Nernst contribution

7 deg

2 4 6 8 10

  • 40
  • 30
  • 20
  • 10

Ulong/ΔT T (K) (U+-U-)/(2ΔT) N(2T)

N (2T) (U+-U-)/2ΔT

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SLIDE 19

Discussion: Thermopower

2 4 6 8 10

  • 40
  • 30
  • 20
  • 10

10 Ulong/ΔT T (K) + 2 T

  • 2 T

variation due to

  • sample dependence
  • misorientation
  • non-negligible Nernst contribution

7 deg

2 4 6 8 10

  • 40
  • 30
  • 20
  • 10

Ulong/ΔT T (K) (U+-U-)/(2ΔT) N(2T)

first systematic study of S(T,B) including:

  • best available samples
  • precise orientation
  • correction for the Nernst signal

N (2T) (U+-U-)/2ΔT

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SLIDE 20

Field-dep. Thermopower

1.5 2 3 4 5 6 7 89 10 20 30 40

  • 40
  • 20

20 40 CeNiSn #5, No. 3 q//b, B//a

0 T 1 T 2 T 4 T 7 T

S (µV/K) T (K)

B // a: - enhanced values of |S|

  • shift of the minimum to lower T

B // c:

  • similar, but less pronounced

literature:

  • strong sample

dependence at low T

  • no comparable results

in field

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SLIDE 21

Discussion: Thermopower

2 4 6 8 1.5 2.0 2.5 3.0 3.5 B // a B // c Tmin (K) B (T)

position of the minimum

  • effect larger for B // a
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SLIDE 22

Discussion: Thermopower

2 4 6 8 1.5 2.0 2.5 3.0 3.5 B // a B // c Tmin (K) B (T)

position of the minimum

  • effect larger for B // a
  • extrapolation // a: Bc = 14 T

(MR: 18 T)

shift ~ closing of the gap

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SLIDE 23

Discussion: Thermopower

position of the minimum

  • effect larger for B // a
  • extrapolation // a: Bc = 14 T

(MR: 18 T)

shift ~ closing of the gap

(ΔE from tunneling spectroscopy)

2 4 6 8 1.5 2.0 2.5 3.0 3.5

8 10 12 14 16 18

B // a B // c Tmin (K) B (T)

ΔE

ΔE (meV)

  • T. Ekino et al., Physica B 230-232, 635 (1997)
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SLIDE 24

Discussion: Thermopower

position of the minimum

  • effect larger for B // a
  • extrapolation // a: Bc = 14 T

(MR: 18 T)

shift ~ closing of the gap

(ΔE from tunneling spectroscopy)

2 4 6 8 1.5 2.0 2.5 3.0 3.5

8 10 12 14 16 18

B // a B // c Tmin (K) B (T)

ΔE

ΔE (meV)

  • T. Ekino et al., Physica B 230-232, 635 (1997)

2 4 6 8

  • 50
  • 45
  • 40
  • 35
  • 30
  • 25

B // a B // c Smin (µV/K) B (T)

value at the minimum

  • effect larger for B // a
  • change of the DOS near EF due

to Zeeman splitting (cP)

  • similar results for S(T) at low T
  • K. Izawa et al., J. Phys. Soc. Jpn. 65, 3119 (1996)
  • S. Paschen et al., Phys. Rev. B 62, 14912 (2000)
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SLIDE 25

Discussion: Thermopower

F

ln

E

N S ε ∂ ∂ ∝

V-shaped DOS in field similar analysis for CP(T,B) (enhanced γ value in field)

increasing B

  • K. Izawa et al., J. Phys. Soc. Jpn. 65, 3119 (1996)
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SLIDE 26

Results: Nernst effect

large values of N below 10 K (opening of the gap)

  • scaling for B // a (easy axis!)
  • shift of minimum for B // c

→ open question: weak sensitivity to magnetic fields // a q // b, B // a B // c

1.5 5 10 50

  • 120
  • 100
  • 80
  • 60
  • 40
  • 20

2 4 6 8 10

  • 20
  • 15
  • 10
  • 5

4 T 7 T 0.5 T 1 T 2 T

N (µV/K) T (K)

ν (µV/KT)

T (K)

1.5 5 10 50

  • 120
  • 100
  • 80
  • 60
  • 40
  • 20

2 4 6 8 10

  • 15
  • 10
  • 5

5.5 T 7 T 1 T 2 T 3 T

N (µV/K) T (K)

ν (µV/KT)

T (K)

slide-27
SLIDE 27

Discussion: Nernst effect

Boltzmann approximation:

F

* 3

2 B 2 n E

m T k N ε τ π ∂ ∂ =

F H 2 B 2 n

tan 3 E Be T k N Θ ≈ π

xx yx

σ σ = ΘH tan

with Hall angle Large Nernst coefficient:

  • Low charge carrier concentration
  • Small Fermi energy

Nernst effect: νa = νn - εyy/κyy Lxy νn: normal Nernst coeff. νa: adiabatic Nernst coeff. due to transverse temp. gradient For CeNiSn, ΔTy ≈ 0, Lxy ≈ 0 (below resolution limit) → νa = νn

νn νn

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SLIDE 28

Discussion: Nernst effect

N

Behnia et al., Phys. Rev. Lett. 98, 076603 (2007)

How to obtain large Nernst coefficients?

slide-29
SLIDE 29

Discussion: Nernst effect

N

Bi normal semimetal

Behnia et al., Phys. Rev. Lett. 98, 076603 (2007)

How to obtain large Nernst coefficients?

slide-30
SLIDE 30

Discussion: Nernst effect

N

Bi normal semimetal PrFe4P12 URu2Si2 correlations, unconventional

  • rder

Behnia et al., Phys. Rev. Lett. 98, 076603 (2007)

How to obtain large Nernst coefficients?

slide-31
SLIDE 31

Discussion: Nernst effect

N

Bi normal semimetal PrFe4P12 URu2Si2 correlations, unconventional

  • rder

CeRu2Si2 CeCoIn5 enhanced mass

Behnia et al., Phys. Rev. Lett. 98, 076603 (2007)

How to obtain large Nernst coefficients?

slide-32
SLIDE 32

Discussion: Nernst effect

N

Bi normal semimetal PrFe4P12 URu2Si2 correlations, unconventional

  • rder

CeRu2Si2 CeCoIn5 enhanced mass NbSe2 bipolar Nernst effect

Behnia et al., Phys. Rev. Lett. 98, 076603 (2007)

How to obtain large Nernst coefficients?

slide-33
SLIDE 33

Discussion: Nernst effect

Boltzmann approximation:

F

* 3

2 B 2 n E

m T k N ε τ π ∂ ∂ =

F H 2 B 2 n

tan 3 E Be T k N Θ ≈ π

BUT: CeNiSn with two types of charge carriers

xx yx

σ σ = ΘH tan

with Hall angle

slide-34
SLIDE 34

Discussion: Nernst effect

Boltzmann approximation:

F

* 3

2 B 2 n E

m T k N ε τ π ∂ ∂ =

F H 2 B 2 n

tan 3 E Be T k N Θ ≈ π

BUT: CeNiSn with two types of charge carriers

xx yx

σ σ = ΘH tan

with Hall angle

B

Hall effect

j

  • V. Oganesyan and I. Ussishkin, Phys. Rev. B 70, 054503 (2004)
  • A. Pourret et al., Phys. Rev. Lett. 96, 176402 (2006)

B

Nernst effect

q

slide-35
SLIDE 35

B

Discussion: Nernst effect

Boltzmann approximation:

F

* 3

2 B 2 n E

m T k N ε τ π ∂ ∂ =

F H 2 B 2 n

tan 3 E Be T k N Θ ≈ π

BUT: CeNiSn with two types of charge carriers

xx yx

σ σ = ΘH tan

with Hall angle

B

Hall effect

B

Nernst effect

q

  • V. Oganesyan and I. Ussishkin, Phys. Rev. B 70, 054503 (2004)
  • A. Pourret et al., Phys. Rev. Lett. 96, 176402 (2006)

j

slide-36
SLIDE 36

Discussion: Nernst effect

1.5 5 10 50

  • 120
  • 100
  • 80
  • 60
  • 40
  • 20

2 4 6 8 10

  • 20
  • 15
  • 10
  • 5

4 T 7 T 0.5 T 1 T 2 T

N (µV/K) T (K)

ν (µV/KT)

T (K)

q // b, B // a

1.5 5 10 50

  • 0.04
  • 0.02

0.00

CeNiSn No.3 j // b, B // a

RH (cm

3/C)

T (K)

1 T 2 T 4 T 7 T

sign change in RH but not in N

slide-37
SLIDE 37

Discussion: Nernst effect

1.5 5 10 50

  • 120
  • 100
  • 80
  • 60
  • 40
  • 20

0.5 T 1 T 2 T 4 T 7 T

N (µV/K) T (K)

q // b, B // a relevant mechanism:

  • pening of the gap ↔

enhanced values of N low Fermi energy TK TK Tgap

slide-38
SLIDE 38

Discussion: Nernst effect

ν ~ T/B tan ΘH Increase below Tg No scaling Hall coefficient stronger suppressed in field

F H 2 B 2 n

tan 3 E Be T k N Θ ≈ π

xx yx

σ σ = ΘH tan

νn

slide-39
SLIDE 39

Discussion: Nernst effect

ν ~ S/B tan ΘH Increase below Tg No scaling Maximum in S tan ΘH shifts in contrast to N/B → Multiband effects must be included

F H 2 B 2 n

tan 3 E Be T k N Θ ≈ π

νn

slide-40
SLIDE 40

Discussion: Nernst effect

CeNiSn N T (K)

CeNiSn

ν

CeNiSn ( = 2 K) T CeNiSn ( = 2 K) T PrFe P

4 12

PrFe P

4 12

T = 1.2 K NB Z T =

mag

CeNiSn (T = 2K) CeNiSn (2K)

νB (µV/K) ZmagT = (N2σT)/κ

ZmagT: Low, since high κ (single crystals) High, since small MR

slide-41
SLIDE 41

Discussion: Nernst effect

CeNiSn N T (K)

CeNiSn ν

ZmagT: Low, since high κ (single crystals) High, since small MR

CeNiSn ( = 2 K) T CeNiSn ( = 2 K) T PrFe P

4 12

PrFe P

4 12

T = 1.2 K NB Z T =

mag

CeNiSn (T = 2K) CeNiSn (2K)

νB (µV/K) ZmagT = (N2σT)/κ

1.5 5 10 50 50 100 150 200

0 T 1 T 2 T 4 T 7 T

ρ (μΩ cm)

T (K)

CeNiSn No.3 j // b, B // a

slide-42
SLIDE 42

Summary

thermopower:

  • first systematic study of S(T,B) taking into account the Nernst signal
  • reported sample dependence partly due to misorientation/ Nernst signal
  • low-T thermopower governed by the pseudogap opening
  • Unusal field dependence due to gap closing and Zeeman splitting
slide-43
SLIDE 43

Summary

thermopower:

  • first systematic study of S(T,B) taking into account the Nernst signal
  • reported sample dependence partly due to misorientation/ Nernst signal
  • low-T thermopower governed by the pseudogap opening
  • Unusal field dependence due to gap closing and Zeeman splitting

Nernst coefficient:

  • large signal below gap opening
  • scaling for B//a
  • high relevance of the pseudogap
  • potential of correlated semiconductors for Ettingshausen cooling (low

ρ(B))