Junction of two topological insulators and a p-wave superconductor

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Junction of two topological insulators and a p-wave superconductor

Oindrila Deb

Centre for High Energy Physics Indian Institute of Science

Bangalore, India

September 3, 2014

Soori, Deb, Sengupta and Sen, Phys. Rev. B 87, 245435 (2013)

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Organization of the talk

Introduction

Scattering at the junction

Hamiltonian and energy dispersion

Probability and charge current

A general boundary condition

Charge conductance

Spin conductance

Summary

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Introduction

Topological insulators are gapped in the bulk but have gapless states on the surface. So the surface states are metallic.

Described by massless Dirac equation, edge states are

robust against static (Time-reversal-invariant) disorder.

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• Transmission across a junction of a normal metal (NM) and a superconductor (SC) has been extensively studied

(Blonder et al, Phys. Rev. B 25, 4515 (1982)1982, K. Sengupta et al,Phys. Rev. B 63, 144531 (2001))

• The sub-gap transport in such junctions is governed by Andreev reflection

• A junction between a topological insulator (TI) and

superconductor (SC) is different and more complex because : 1. Surface states of a TI displayspin-momentum locking 2. Particle and hole are coupledin a superconductor

• Four component spinorformalism to describe both spin and particle-hole degrees of freedom

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Scattering at the junction

• Schematic diagram (3D-pic) of the set-up. Normal or Andreev scatterings of the incident electron on TI-1 and TI-2 and BdG quasiparticle (evanescent) transmissions on the SC side

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Hamiltonian and energy dispersion

• Hamiltonian on a TI-surface:

H1= Z Z

dki dkj ψ~

k [~vFnˆ· (σ ×−→

k) − µTII] ψ~k

whereψis a two component spinor,vF is the Fermi velocity ,ˆn points normal to the 2-D surface ,ki, kj are momenta in the 2-D plane

E = −µTI± ~vF

qki2+kj2

• Wave fns on the SC side are described by a four component

BdG spinor: ΨSC=

 Ψ

Ψ

Ψ Ψ

• SC Hamiltonian :

HSC = Z

−∞

dx Z

0

dyΨ(x,y)h

~2~2 2m − µSC



τz+ ∆(x,y)i Ψ(x,y),

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• SC pair potential∆(x,y)can be s-wave (singlet) or p-wave (triplet)

• SC pair potential∆(x,y)for p-wave (triplet) SC:

∆(x,y) = 0 0f(~k)(~d· ~σ)iσy

−∆0f(~k)(~d· ~σ)iσy 0

!

where f(~k) = −i(axx+ayy)

We choose ax =0 and ay =1 making the pair potential anisotropic

• The choice of~d (= ˆx, ˆy, ˆz)determines the spin-state of the Cooper pair

E = ± q

(2m~2(kx2+ky2) − µSC)2+ ∆20(−→ a ·−→

k)(−→ a·−→

k)

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Probability and charge current

• Let’s assume :Ψ =ψ φ



whereψandφare the upper two and lower two components of the BdG spinorΨ

• Probability density :ρp= ψψ + φφ = ΨΨ Charge density :ρc =e(ψψ − φφ) =τzΨ

• Corresponding currents−→ Jp and−→

Jc satisfy the equation of continuity : ∂tρ +−→

∇ ·−→ J =0

• Using the equations of motion and continuity we can find the currents :

JpTI =vFnˆ× −→σ ψ + φnˆ×−→ σφ]

JpSC= m~Im(Ψτz−→

∇Ψ) +−→ Jpair

• −→

Jpair = ˆx2∆~0Re[axψ(−→

d · −→σ )iσyφ] + ˆy2∆~0Re[ayψ(−→

d · −→σ )iσyφ]

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A general boundary condition

• To get the boundary condition we use conservation ofprobability currentnormal to the junction

• (ˆy·−→

Jp1)y→0− (ˆz·−→

Jp2)z→0 = (ˆy·−→ Jp3)y→0+

• We find that a general boundary condition involves three time-reversal invariant barriers near the junction

• Physically these barriers can arise due to gate voltages and also a lattice mismatch between TIs and SC

• General boundary condition :

1 Ψ3=M11+ βM22 2 mv~

1yΨ3−2χ3Ψ3+~v0

1

0 −ay(−→ d · −→σ )σy ay(−→

d · −→σy 0

!

=x ⊗ τz[M(χ11− βM22] β =q

v2

v1 andM(χ) =cos(χ) −i sin(χ)σx⊗ τz

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Charge conductance

• We want to solve the scattering problem and find the conductance

• Consider an electron incident on the junction from TI-1 with energy E which lies in the SC gap

• The wavefunctions on TI and SC sides will look like :

Ψ1= ψ1p+rNψ1p+rAψ1h, Ψ2=tNψ2p+tAψ2h. Ψ3=t1ψ↑+sc +t3ψ↑−sc +t2ψsc↓++t4ψ↓−sc ,

The scattering amplitudes rN(A), tN(A), t1,2,3,4can be determined using the boundary conditions

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• Conservation of the probability current at the junction implies : v1sinθ1=v1(sinθ1RN+sinθ1hRA) +v2(sinθ2TN+sinθ2hTA)

• Charge current conservation perpendicular to the junction : J3=J1,inJ2,out

• Incoming charge current alongy on TI-1 :ˆ J1,in=ev1[sinθ1(1−RN) +sinθ1hRA]

• Outgoing charge current along−ˆz on TI-2 : J2,out =ev2[sinθ2TN−sinθ2hTA]

• Hence using conservation of probability current we get : J3=2e(v1sinθ1hRA+v2sinθ2hTA)

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A voltage bias V is applied on the TI-1 side maintaining the TI-2 and SC at the same Fermi energy.

The differential conductance G3=dI3/dV on SC-side at an applied bias voltage V .

• Integrating over all angles of incidenceθ1, the differential conductance is:

G3(V) =G0(V) Z π

0

dθ1[sinθ1hRA+sinθ2hTA],

where RN(A)= |rN(A)|2, TN(A) = |tN(A)|2and G0(V) =e2WTI+eV)/(hv1µTI)

and W is the width of the sample

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Zero bias peak

Figure: The sub-gap conductance of a py-wave SC in units of G0, for~d = ˆz andχ1= χ2=0

• The zero bias peak is due to themid-gap bound statei.e E=0 state on SC side

• At E=0 transmission isindependentofχ3

• Peak is sharper at largeχ3

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• Conductance is different for different spin triplet states i.e for different−→

d

• For−→

d = ˆz at E=0: rA=tN=0 and tAand hence the conductance depends only on(χ1− χ2)

• For−→

d = ˆy we found the similar result as−→ d = ˆz

• For−→

d = ˆx we found tA=tN =0 , while|rA|2= (sinθ1)2and

|rN|2= (cosθ1)2areindependent ofχ12

• Electrons and holes seeopposite barrier strengthsχi and−χi

respectively

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Figure: Conductance of a py-wave SC at E=0 for different spin pairings:~d= ˆz (blue dashed line),~d= ˆx (green solid line) and~d= ˆy (red dot-dashed line)

This can be used to distinguish between different

spin-triplet states of the p-wave SC.

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• Typically, in a Schr ¨odinger system, the conductance decays with the barrier strength, while in a Dirac system, conductance is a periodic function of the barrier strength.

• In our setup, the TI-sides are Dirac-like while the SC is Schr ¨odinger-like.

• So, the conductance depends onbarriersχ1,2periodicallyand decays with barrierχ3on SC side

Figure:Conductance of a py-wave SC with~d= ˆz at different energies in the SC gap

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Spin conductance

For a

=

x

,

y, z, the a component of the spin density is given by

ρa = ~

2 Ψ3τz⊗ σaΨ3

The spin current

~Ja

corresponding to the spin density

ρa

can be calculated on the SC side using the equations of motion.

The corresponding spin conductance is given by

Gas =Gs0Rπ

0 dθ1Jya, where Gs0=eW(µTI+eV)/(hv1)2.

Now, there are nine currents corresponding to three spin

components and three possible choices of the

~

d vector.

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~

d

= ˆ

x

~

d

= ˆ

y

~

d

= ˆ

z J

sx

0 non-zero non-zero

J

sy

0 non-zero 0

J

sz

non-zero non-zero 0

Table: Expressions for y component of spin currents for different spin pairings of the p-wave SC.

~

d

= ˆ

x

~

d

= ˆ

y

~

d

= ˆ

z G

xs

0 non-zero non-zero

G

sy

0 0 0

G

zs

0 0 0

Table: Spin conductances for different spin pairings.

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The x -spin conductance is non-zero for the cases

~

d

= ˆ

y and

~

d

= ˆ

z.

Let us look at the features of the x -spin conductance for the case

~

d

= ˆ

z .

Left panel: Gxsas a function of E=eV forχ1= χ2=0,µTI/∆0=5 andµsc/∆0=100.

Right panel: Gxsas a function ofχ = χ1= χ2= χ3and E .

The unusual satellite peak (SP) in addition to the ZBP is a

novel feature.

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To understand the SP, we relate the spin-currents on SC side to the physical quantities on TI-1 and TI-2 using the boundary condition.

The x -spin current on the SC side of the junction is linearly related to the steady state charge densities on the TI-1 and TI-2 sides, all evaluated at the junction:

yˆ· ~Jsx = ~vF

2 [Ψ1τzΨ1− Ψ2τzΨ2] = 1+RN+RNRAΓ1ATN+TAΓ2A

where

RN =Re(rN+rNe−i 2θ1),

Γ1A= ν2Ecos2θ1− νEcosθ1q

νE2cos2θ1−1,Γ2A= |νEcosθ1|

when

νE≡ (µTI+E)/(µTIE)>1.

It is interesting to note that the spin conductance on the SC

side depends on both the phase and magnitude of the

reflection amplitude r

N

.

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The following figure shows the contributions to the spin conductance from the different terms in the previous equation integrated over all incident angles

θ1

.

−0.5 −0.25 0 0.25 0.5

−0.2

−0.1 0 0.1 0.2 0.3 0.4 0.5

E/∆0 Different contributions to Gx s in units of Gs0

χ3 = 0 µTI/∆0 = 5 µSC/∆0=100 Gx

s R‘

N TAΓ2A−RAΓ1A RN−TN

From the figure, it is evident that the Andreev scattering

term,

TAΓ2ARAΓ1A

, and the phase term

RN

contribute

the most to the SP.

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From the contour plot of spin-current y

ˆ·

J

sx

as a function of E and angle of incidence

θ1

, the contribution to the SP from a range of

θ1

is clearly visible.

If

νE

cos

θ1>

1, the Andreev modes on TI-1 and TI-2

become evanescent and do not carry any current.

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At a given

(E, θ1), momentum of the Andreev reflected hole

is:

kyh=

q

TIE)2− (µTI+E)2cos2θ1/(~v1) =µTIE

~v1

q

1 − ν2Ecos2θ1

.

The contribution to the SP comes from region where the Andreev modes exist.

And therefore, the SP appears at a positive bias.

Also, the phase of the reflection amplitude r

N

changes from

−π

to

π

through 0 when E is varied at a fixed

θ1

.

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Summary

• We described a formalism to study thetransportacross junctions of topological insulators and superconductors and derived the appropriateboundary conditions.

• A general boundary condition involvesthree time-reversal invariant barriers

• Charge conductance shows azero bias peak

• Tunneling conductance of TI-SC junction provides a novel method for detection ofdifferent directions of~d of SC (spin-state of Cooper pairs in SC)

• Such junctions can inject spin current into SC for certain triplet-pairings of the Cooper pairs

• The spin conductance shows asatellite peakat finite bias voltages in addition to the zero bias peak

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References

A. Soori, O. Deb, K. Sengupta, D. Sen, Phys. Rev. B 87, 245435 (2013)

D. Sen and O. Deb, Phys. Rev. B, 85, 245402 (2012);

Erratum, Phys. Rev. B 86 (2012) 039902(E).

K. Sengupta, I. Zutic

, H.-J. Kwon, V. M. Yakovenko and S.

Das Sarma, Phys. Rev. B 63, 144531 (2001)

G.E. Blonder, M.Tinkham, and T.M.Klapwijk , Phys. Rev. B

25, 4515 (1982)

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