Top Banner
Arnaud Koetsier Floris van Liere Henk Stoof The imbalanced antiferromagnet in an optical lattice
20

The imbalanced antiferromagnet in an optical lattice

May 11, 2015

Download

Education

Made with powerpoint + TeX4ppt. Source and high-resolution images available upon request.
Welcome message from author
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
Page 1: The imbalanced antiferromagnet in an optical lattice

ArnaudKoetsier

Floris van Liere

Henk Stoof

The imbalanced antiferromagnet in an optical lattice

Page 2: The imbalanced antiferromagnet in an optical lattice

2

Introduction

• Fermions in an optical lattice• Described by the Hubbard model• Realised experimentally [Esslinger ’05]• Fermionic Mott insulator recently seen [Esslinger ’08, Bloch ’08]• There is currently a race to create the Néel state

• Imbalanced Fermi gases• Experimentally realised [Ketterle ’06, Hulet ’06]• High relevance to other areas of physics (particle physics, neutron stars, etc.)

• Imbalanced Fermi gases in an optical lattice ??

Page 3: The imbalanced antiferromagnet in an optical lattice

3

Fermi-Hubbard Model

Sums depend on:Filling NDimensionality (d=3)

On-site interaction: U Tunneling: t

Consider nearest-neighbor tunneling only.

The positive-U (repulsive) Fermi-Hubbard Model, relevant to High-Tc SC

H = −tPσ

Phjj0i

c†j,σcj0,σ + UPjc†j,↑c

†j,↓cj,↓cj,↑

Page 4: The imbalanced antiferromagnet in an optical lattice

4

Quantum Phases of the Fermi-Hubbard ModelFi

lling

Frac

tion

0

0.5

1

Mott Insulator (need large U)

Band Insulator

Conductor

Conductor

Conductor

• Positive U (repulsive on-site interaction):

• Negative U: Pairing occurs — BEC/BCS superfluid at all fillings.

Page 5: The imbalanced antiferromagnet in an optical lattice

5

• At half filling, when and we are deep in the Mott phase.Hopping is energetically supressedModel simplifies: only spin degrees of freedom remain (no transport)

• Integrate out the hopping fluctuations, then the Hubbard model reduces to the Heisenberg model:

U À t

Mott insulator: Heisenberg Model (no imbalance yet)

kBT ¿ U

J =4t2

U

Szi =1

2

³c†i,↑ci,↑ − c†i,↓ci,↓

´S+i =c

†i,↑ci,↓

S−i =c†i,↓ci,↑

H =J

2

Xhjki

Sj · Sk

Spin ½ operators: S = 12σ

Superexchange constant (virtual hops):

Page 6: The imbalanced antiferromagnet in an optical lattice

6

Néel State (no imbalance yet)

• The Néel state is the antiferromagnetic ground state for

• Néel order parameter measures amount of “anti-alignment”:

• Below some critical temperature Tc, we enter the Néel state and becomes non-zero.

0 Tc0

0.5

T

⟨n⟩

0 ≤ h|n|i ≤ 0.5

h|n|i

h|n|i

nj = (−1)jhSji

J > 0

Page 7: The imbalanced antiferromagnet in an optical lattice

7

• Until now, • Now take — spin population imbalance. • This gives rise to an overal magnetization

N↑ 6= N↓

• Add a constraint to the Heisenberg model that enforces

Heisenberg Model with imbalance

Effective magnetic field (Lagrange multiplier):

H =J

2

Xhjki

Sj · Sk −Xi

B · (Si −m)

m = (0, 0,mz)

mz = SN↑ −N↓N↑ +N↓

(fermions: )S = 12

N↑ = N↓ = N/2

hSi =m

B

Page 8: The imbalanced antiferromagnet in an optical lattice

8

• ground state is antiferromagnetic (Néel state)Two sublattices:

• Linearize Hamiltonian:

• Magnetization:

• Néel order parameter:

• Obtain the on-site free energy subject to the constraint (eliminates )

J > 0⇒

Mean field analysis

A, B

m =hSAi+ hSBi

2

n =hSAi− hSBi

2

SA(B)i = hSA(B)i i+ δS

A(B)i

f(n,m;B)

∇Bf = 0 B

B

A B

A

A

B

AB

B

B

A

A

Page 9: The imbalanced antiferromagnet in an optical lattice

9

Phase Diagram in three dimensions

0 Tc0

0.5

T

⟨n⟩

Add imbalance0.0

0.2

0.4mz0 0.3 0.6

0.91.2kBT�J

0.0

0.2

0.4n

mz

k B T

/J

0 0.1 0.2 0.3 0.4 0.50

0.5

1

1.5

m

nIsing:

m

n

Canted:

n 6= 0

n = 0

Page 10: The imbalanced antiferromagnet in an optical lattice

10

Spin waves (magnons)

• Spin dynamics can be found from:

• Imbalance splits the degeneracy:

−π2

π

2kd

h̄ω/Jz

00

0.1

0.2

0.3

0.4

0.5No imbalance: Doubly degenerate antiferromagnetic dispersion

Antiferromagneticmagnons: ω ∝ |k|

ω ∝ k2Ferromagneticmagnons:

dS

dt=i

~[H,S]

Gap:(Larmorprecessionof n)

Page 11: The imbalanced antiferromagnet in an optical lattice

11

Long-wavelength dynamics: NLσM

• Dynamics are summarised a non-linear sigma model with an action

• The equilibrium value of is found from the Landau free energy:

• NLσM admits spin waves but also topologically stable excitations in the local staggered magnetisation .

S[n(x, t)] =

Zdt

Zdx

dD

½1

4Jzn2

µ~∂n(x, t)

∂t− 2Jzm× n(x, t)

¶2− Jd

2

2[∇n(x, t)]2

¾

F [n(x),m] =

Zdx

dD

½Jd2

2[∇n(x)]2 + f [n(x),m]

¾

• lattice spacing:• number of nearest neighbours:• local staggered magnetization:

d = λ/2z = 2Dn(x, t)

n(x, t)

n(x, t)

Page 12: The imbalanced antiferromagnet in an optical lattice

12

• The topological excitaitons are vortices; Néel vector has an out-of-easy-plane component in the core

• In two dimensions, these are merons:• Spin texture of a meron:

• Ansatz:

• Merons characterised by:Pontryagin index ±½VorticityCore size λ

Topological excitations

n =

⎛⎝ pn2 − [nz(r)]2 cosφ

nvpn2 − [nz(r)]2 sinφ

nz(r)

⎞⎠nv = 1

nv = −1nv = ±1

nz(r) =n

[(r/λ)2 + 1]2

Page 13: The imbalanced antiferromagnet in an optical lattice

13

Meron size

• Core size λ of meron found by plugging the spin texture into and minimizing (below Tc):

• The energy of a single meron diverges logarithmically with the system area A at low temperature as

merons must be created in pairs.

0 0.1 0.20.3

0.4mz0.3

0.60.9

1.21.5

kBT�J0

2

4

d

F [n(x),m]

Jn2π

2ln

A

πλ2

mz

k B T

/J

0 0.1 0.2 0.3 0.4 0.50

0.5

1

1.5

Meronspresent

Meron core size

Page 14: The imbalanced antiferromagnet in an optical lattice

14

Meron pairs

Low temperatures:A pair of merons with opposite vorticity, has a finite energy since the deformation of the spin texture cancels at infinity:

Higher temperatures:Entropy contributions overcome the divergent energy of a single meronThe system can lower its free energy through the proliferation of single merons

Page 15: The imbalanced antiferromagnet in an optical lattice

15

Kosterlitz-Thouless transition

• The unbinding of meron pairs in 2D signals a KT transition. Thisdrives down Tc compared with MFT:

• New Tc obtained by analogy to an anisotropic O(3) model (Monte Carlo results: [Klomfass et al, Nucl. Phys. B360, 264 (1991)] )

mzk B

T/J

0 0.05 0.10

0.02

0.04

0.06

n 6= 0

mz

k B T

/J

0 0.2 0.40

0.2

0.4

0.6

0.8

1

KT transition

MFT in 2D

Page 16: The imbalanced antiferromagnet in an optical lattice

16

Experimental feasibility

• Experimental realisation:Imbalance: drive spin transitions with RF fieldNéel state in optical lattice: adiabatic cooling [AK et al. PRA77, 023623 (2008)]

• Observation of Néel stateCorrelations in atom shot noiseBragg reflection (also probes spin waves)

• Observation of KT transitionInterference experiment [Hadzibabic et al. Nature 441, 1118 (2006)]In situ imaging [Gericke et al. Nat. Phys. 4, 949 (2008); Würtz et al.arXiv:0903.4837]

Page 17: The imbalanced antiferromagnet in an optical lattice

17

Conclusion

• Tc calculated for entering an antiferromagnetically ordered state in mean field theory

• Topological excitations give rise to a KT transition in 2D which significantly lowers Tc compared to MFT.

• The imbalanced antiferrromagnet is a rich systemferro- and antiferromagnetic propertiescontains topological excitationsmodels quantum magnetism, bilayers, etc.merons possess an internal Ising degree of freedom associated toPontryagin index — possible application to topological quantum computation

• Future work:include fluctuations beyond MFT for better accuracy in three dimensionsinvestigate topological excitations in 3D (vortex rings)incorporate equilibrium in the NLσMgradient of n gives rise to a magnetization

Page 18: The imbalanced antiferromagnet in an optical lattice

18

• On-site free energy:

where• Constraint equation:

• Critical temperature:

• Effective magnetic field below the critical temperature:

Results

f(n,m;B) =Jz

2(n2 −m2) +m ·B

− 12kBT ln

∙4 cosh

µ |BA|2kBT

¶cosh

µ |BB |2kBT

¶¸BA (B) = B− Jzm± Jzn

B = 2Jzm

m =1

4

∙BA|BA|

tanh

µ |BA|2kBT

¶+BB|BB |

tanh

µ |BB |2kBT

¶¸

Tc =Jzmz

2kBarctanh(2mz)

Page 19: The imbalanced antiferromagnet in an optical lattice

19

Anisotropic O(3) model

• Dimensionless free energy of the anisotropic O(3) model [Klomfass et al, Nucl. Phys. B360, 264 (1991)] :

• KT transition:

• Numerical fit:

βf3 = −β3Xhi,ji

Si · Sj + γ3Xi

(Szi )2

γ3(β3) =β3

β3 − 1.06exp[−5.6(β3 − 1.085)].

1.0 1.2 1.4 1.6 1.8 2.00.0

0.2

0.4

0.6

0.8

1.0

b3

g 3êH1+g

3L

Page 20: The imbalanced antiferromagnet in an optical lattice

20

Analogy with the anisotropic O(3) model

• Landau free energy:

0.0 0.1 0.2 0.3 0.4 0.50.0

0.5

1.0

1.5

2.0

2.5

3.0

m

gHm,bLê

J

βF =− βJ

2

XhI,ji

ni · nj + βXi

f(m,ni,β)

'− βJn2

2

XhI,ji

Si · Sj + βn2γ(m,β)Xi

(Szi )2

β3 =Jβn2

2

γ3 =2β3Jγ(m,β)

Mapping of our model toAnisotropic O(3) model:

Numerical fit parameter

0.02

1/Jβ =

0.2

0.4

0.60.8

Tc