Quantum heterodyne Hall effect from oscillating magnetic fields - - PowerPoint PPT Presentation

quantum heterodyne hall effect from oscillating magnetic
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Quantum heterodyne Hall effect from oscillating magnetic fields - - PowerPoint PPT Presentation

Quantum heterodyne Hall effect from oscillating magnetic fields Takashi Oka Max Planck institute PKS and CPfS (Dresden) Nonequilibrium Quantum Matter 1. Introduction 2. Classical heterodyne Hall effect 3. Quantum heterodyne Hall effect


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SLIDE 1

Quantum heterodyne Hall effect from

  • scillating magnetic fields

Takashi Oka Max Planck institute PKS and CPfS (Dresden) “Nonequilibrium Quantum Matter”

  • 1. Introduction
  • 2. Classical heterodyne Hall effect
  • 3. Quantum heterodyne Hall effect
  • 4. Quantum Dirac heterodyne Hall effect

TO, Bucciantini, PRB’16 TO, Kitamura, Nag, Saha, Bucciantini in prep

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SLIDE 2

What is a heterodyne?

Bluetooth Wifi, TV, radio

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SLIDE 3

What is a heterodyne?

Bluetooth Wifi, TV, radio

2.40xGHz

superheterodyne device

kHz

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SLIDE 4

What is a heterodyne? fLO fS1-fLO

fS1-fLO

fS

from wikipedia “heterodyne” Local oscillator = periodically driven system

2.401GHz 2.402GHz

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SLIDE 5

Linear response theory ja(t) =

  • dt′σab(t, t′)Eb(ω)e−iωt′

w: signal frequency

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SLIDE 6

Linear response theory ja(t) =

  • dt′σab(t, t′)Eb(ω)e−iωt′

w: signal frequency If static, σ(t − t′)

= σab(ω)Eb(ω)e−iωt′

ac-conductivity

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SLIDE 7

Linear response theory for periodically driven system

ja(t) =

  • dt′σab(t, t′)Eb(ω)e−iωt′

Ω

Periodic driving input signal

Heterodyne (Floquet state)

  • utput signal

ω ω + l Ω

=

  • n

σn

ab(ω)e−i(ω+nΩ)tEb(ω)

w: signal frequency W: drive frequency

TO, Bucciantini, PRB’16

n

w + n W

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SLIDE 8

Heterodyne Hall effect

TO, Bucciantini, PRB’16

Application: Dissipationless frequency conversion Ultra-low power consuming Bluetooth!?

σn

xy(ω)

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SLIDE 9

Heterodyne Hall effect

TO, Bucciantini, PRB’16

In the following, I will focus on the resonant case

w=W

σn

xy(ω)

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SLIDE 10

B(t) = B cos Ωt

time dependent magnetic field

Example 1: Classical particle in an oscillating B field m d dt + η

  • v(t) = e
  • E(t) + 1

c v × B(t)

  • Newton’s equation

z

TO, Bucciantini, PRB’16

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SLIDE 11

wc/W=3.0 6.0 5.0

B(t) = B cos Ωt

wc=qB/mec

cyclotron frequency

TO, Bucciantini, PRB’16

no E-field

Example 1: Classical particle in an oscillating B field

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SLIDE 12

wc/W=3 6 5

(t=0.05, Ey=1) dc-conductivity with static Ey-field

ja(t) =

  • dt′σab(t, t′)Eb(ω)e−iωt′

=

  • n

σn

ab(ω)e−i(ω+nΩ)tEb(ω)

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SLIDE 13

Periodic orbits

wc/W=2.41 8.66 5.52

(t=0.0, Ey=0)

(i) (iii) (ii) winding per half cycle a=1 a=2 a=3

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SLIDE 14

Heterodyning Hall current

wc/W =3 6 5

TO, Bucciantini, PRB’16

exact results

σn,m

ab

= σn−m

ab

(mΩ)

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SLIDE 15

Summary: Example I

TO, Bucciantini, PRB’16 ja(t) =

  • n

σn

ab(ω)e−i(ω+nΩ)tEb(ω)

Classical particle in an oscillating B-field @ magic frequencies ((i), (ii), (iii),.. zeros of J0(B/W))

σ0

xx(0) = 0

σ−1

xy (Ω) ∼ 1

B

heterodyne Hall ``insulator”

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SLIDE 16

B(t) = B cos Ωt

time dependent magnetic field

Example 2: Quantum particle in oscillating B field

m d dt + η

  • v(t) = e
  • E(t) + 1

c v × B(t)

  • Newton’s equation

z

TO, Bucciantini, PRB’16

Schrodinger equation

H = 1 2m

  • ˆ

px

2 + (py − B0 cos(Ωt)x)2

Ay

=

Solvable by Husimi transformation

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SLIDE 17

Quantization: static B

ϕn(x) = e−x2/2l2

BHn(x/lB)

lB = B−1/2

H = 1 2m

  • ˆ

px

2 + (py − Bx)2 x

momentum-position locking

X = py B

Ay

=

wc=qB/mec

level spacing

y

k

E

n=0 n=2 n=1 n

cyclotron frequency

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SLIDE 18
  • A. THz metamaterial
  • Y. Mukai, K. Tanaka, et al. (Kyoto grp.) New J. Phys.’16

1 Tesla, 1 THz!!

enhancement factor of B

cf) E-field enhancement (Liu, Nelson, Averitt, et al. Nature 12)

How to realize ?

Ay = B cos(Ωt)x

① incoming laser ② resonating current

B(t)

③ resonating electromagnet

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SLIDE 19

H = 1 2m

  • ˆ

px

2 + (py − B0 cos(Ωt)x)2

Ay

=

Bz = B cos(Ωt) Ey = BΩ sin(Ωt)x

EM-fields

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SLIDE 20

Quantization: time-oscillating B

H = 1 2m

  • ˆ

px

2 + (py − B0 cos(Ωt)x)2

B0=0.2, W=1, py=5

|Φα(x, t)|2

[H − i∂t] |Φα⟩ = εα|Φα⟩

Floquet state

x

Ay

= dotted line wave function

Floquet theory see A. Eckardt RMP’16 Solvable by Husimi transformation

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SLIDE 21

Quantization: time-oscillating B

H = 1 2m

  • ˆ

px

2 + (py − B0 cos(Ωt)x)2 [H − i∂t] |Φα⟩ = εα|Φα⟩

B0=1.89, W=1, py=5

Floquet state

|Φα(x, t)|2

x

Ay

=

periodic micromotion

dotted line

Floquet theory see A. Eckardt RMP’16

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SLIDE 22

εn(py) = En + p2

y

2m∗

e

Floquet quasi-energy Spectrum

Floquet quasi-energy B

εn Ω

ωeff(n + 1/2)

En

temporal mixture n-th Landau levels

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SLIDE 23

εn(py) = En + p2

y

2m∗

e

Floquet quasi-energy Spectrum

new Landau quantization

inverse effective mass

me/m*

e

c

ω /Ω

r=r1

q

r=r2

q

r=r3

q

r=1.89 5.07 8.22

flat band y

k

E

n=0 n=2 n=1 n

m∗ → ∞

py e

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SLIDE 24

me/m*

e

c

ω /Ω

r=r1

q

r=r2

q

r=r3

q

quantum r=1.89 5.07 8.22 flat band classical r=wc/W =1.89 r=5.07 r=8.22 r=wc/W =2.40 r=8.66 r=5.52 x

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SLIDE 25

B(t) = B cos Ωt B E jdc

Dissipationless Heterodyne Hall current

jdc

y

k

E

n=0 n=2 n=1

E =0

x 1

n

σ0,1

yx = e2

h Qν, where ν = Ne/NΦ

LL filling

Integer heterodyne Hall effect pre-factor Q is non-universal

jdc

y = σ0,1 yx E1 x E1

x cos Ωt

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SLIDE 26

B(t) = B cos Ωt

time dependent magnetic field

Example3: 2D Dirac electron in oscillating B field

z

TO, Kitamura, Nag, Saha, Bucciantini, in prep

Dirac equation

Ay

= graphene, surface of 3D TI, …

HDirac = σxˆ px + σy(py − B cos Ωtx)

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SLIDE 27

honeycomb, zigzag edge W=0.6, B/a=0.000, Ex=0.0

Spectrum ky

A(k, ω) = −1 π ImTrˆ Pstatic 1 ω − ˆ Hk + iδ

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SLIDE 28

honeycomb, zigzag edge W=0.6, B/a=0.0010, Ex=0.0

Spectrum ky

A(k, ω) = −1 π ImTrˆ Pstatic 1 ω − ˆ Hk + iδ

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SLIDE 29

honeycomb, zigzag edge W=0.6, B/a=0.0020, Ex=0.0

Spectrum ky

A(k, ω) = −1 π ImTrˆ Pstatic 1 ω − ˆ Hk + iδ

slide-30
SLIDE 30

honeycomb, zigzag edge W=0.6, B/a=0.0030, Ex=0.0

Spectrum ky

A(k, ω) = −1 π ImTrˆ Pstatic 1 ω − ˆ Hk + iδ

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SLIDE 31

zigzag W=0.6, B/a=0.0030, Ex=0.0

Spectrum W/2

  • W/2

W

  • p-Flat bands at e=±W/2
  • A series of bands around them
  • electron-hole resonant state

preserved

A(k, ω) = −1 π ImTrˆ Pstatic 1 ω − ˆ Hk + iδ

“p-Landau levels”

Dirac node

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SLIDE 32

W/2

  • W/2

W Effective Hamiltonian “p-Landau levels”

HDirac = σxˆ px + σy(py − B cos Ωtx)

rotating frame transformation Landau levels of 2D Dirac system n=0 n=1 n=-1

“p-flat band”

n=0 n=1 n=-1

“p-flat band”

x

two n=0 states two n=1 states |y|2

x x x

εn =

  • Ω2 − p2

z

√ Bn ± Ω/2 The flat band is protected by time-glide symmetry (Morimoto-Po-Vishwanath’17)

localized @ center

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SLIDE 33

B(t) = B cos Ωt

time dependent magnetic field

z

Ex = E1

x cos Ωt

Heterodyne Hall effect additional ac-electric field

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SLIDE 34

Heterodyne Hall effect (add B and E)

honeycomb, zigzag edge W=0.6, B/a=0.0020, Ex=0.20

ky

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SLIDE 35

honeycomb, zigzag edge W=0.6, B/a=0.0020, Ex=0.20

ky W/2

  • W/2

W

p-Flat bands at e=±W/2 tilts = p-chiral “center” mode → current in y-direction axial chiral magnetic effect-like band → current in (-y)-direction

“p-Landau levels”

Dirac node

CME: 3D Weyl in E,B fields

Fukushima-Kharzeev-Warringa’08

Heterodyne Hall effect (add B and E)

cf) p-edge state: Rudner-Lindner-Berg-Levin ‘13

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SLIDE 36

Heterodyne Hall effect

honeycomb, zigzag edge W=0.6, B/a=0.0020, Ex=0.20

ky

chiral center state axial CME state

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SLIDE 37

Summary

TO, Bucciantini, PRB’16 TO, Kitamura, Nag, Saha, Bucciantini in prep

σn

xy(ω)

y

k

E

n=0 n=2 n=1

E =0

x 1

n

  • Heterodyne Hall effect in three examples was studied
  • They are characterized by the heterodyne response functions

classical particle quantum 2DEG quantum 2DDirac

  • ngoing: Relation with topology, interaction (fractional state)
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SLIDE 38

Heterodyne Kubo formula

Jn

i (ω) = σn ij(ω)Ej(ω)

σn

ij(ω) = 1

  • k,α,β,m

fβ [εkα − εkβ − mΩ][(εkα − εkβ) + (n − m)Ω] (εkα − εkβ) + (n − m)Ω − ω − iδ Am

βiαA(n−m) αjβ

−[εkβ − εkα − mΩ][(εkβ − εkα) + (n − m)Ω] (εkβ − εkα) + (n − m)Ω − ω − iδ Am

αiβA(n−m) βjα

  • ⟨φkβ(t)|∂kiφkα(t)⟩ =
  • m

eimΩtAm

βiα

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SLIDE 39

time dependent problem

Floquet theory (non-perturbative in driving)

review: A. Eckardt, RMP’16

eigenvalue problem

ψ(t) = e−iεtφ(t)

φ(t + T) = φ(t)

Floquet state

Hφα = εαφα

H = H(t) − i∂t

~ absorption of m “photons”

e: Floquet quasi-energy

Floquet Hamiltonian

Fourier transformation

φ(t) =

  • m

φme−imΩt

general theory 1/3

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SLIDE 40

How to construct the effective Hamiltonian?

Heff = i ln U(T)/T

  • Mathematically ill defined in many-body systems
  • Many expansion schemes (non-convergent)

Pershan, van der Ziel, Malmstrom Phys. Rev. 1966

(i) 2nd order perturbation (ii) 1/W expansions (van Vleck, Floquet-Magnus, Brillouin-Wigner)

Heff = H0 +

  • m>0

[H−m, Hm] mΩ + . . .

(iii) 1/(DEab-nW), 1/(U-nW) expansions (Brillouin-Wigner, …) general theory 2/3 relations between schemes: Mikami, et al. PRB ’16

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SLIDE 41

Brillouin-Wigner expansion

higher order monopoles in the Floquet Weyl semimetal

general theory 3/3

HW,±

eff

=

  • |k| − Ω + A2 |k|2 + k2

3 ± Ωk3

|k|(4|k|2 − Ω2)

  • σ3 − A2(|k| + k3)±1

2|k|Ω(2|k| − Ω)(k2∓1

+

σ+ + h.c.)

Bucciantini, Roy, Kitamura, Oka, arXiv’16 (appendix)

Projection I Projection II

1/W expansions

Heff = H0 +

  • m>0

[H−m, Hm] mΩ + . . .

Mikami et al. PRB’16

P P=

different from Magnus expansion

Q=1-P

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SLIDE 42

Husimi transformation

= driven Harmonic oscillator with an oscillating potential

(ii) Classical driven oscillator (i) Quantum oscillator without driving Husimi (Taniuti) PTP ’53 solution pseudo-energy

+

L = 1 2me ˙ X2 − 1 2meω(t)2X2 + XF(t)

Ψn(x, t) = e− i

Enteikyyϕn(x − X(t), t) exp

i {me ˙ X(t)(x − X(t)) + t dt′L(t′) − L0t}

  • En = εn + 2k2

y

2m∗

En = εn + 2k2

y

2me − 1 T T L(t′)dt′