Achieving the Neel state in an optical lattice

24
Rembert Duine Arnaud Koetsier Immanuel Bloch Henk Stoof

Transcript of Achieving the Neel state in an optical lattice

Rembert Duine

Arnaud Koetsier

Immanuel Bloch

Henk Stoof

2

Motivation

• Can use ultracold fermionic atoms in an optical lattice to map out the Hubbard Model.

• High-Tc SC: Electrons in a doped 2D lattice conjectured to undergo d-wave superconducting transition — not understood in the context of the Hubbard model.

• Also interesting for studying many aspects of quantum magnetism including frustration effects.

• Advantage of using cold atoms: Experimentalists can easily vary:

‣ lattice dimensionality/symmetry‣ interaction strength‣ lattice impurities‣ etc…

‣ doping‣ density

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,↑

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.

5

What is the Néel State?

• The Néel State is the antiferromagnetic ground state of the Fermi-Hubbard Model at half filling (i.e. 1 particle per site), in the limit (tight binding limit):

• 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

U À t

6

1. Start with harmonically trapped 2-component fermi gas of cold atoms. The entropy is:

How to reach the Néel state: 1

Total number of particles: NFermi temperature in the trap: kBTF = (3N )1/3~ω

SFG = NkBπ2 T

TF

V =1

2mω2r2

Trapping potential:

7

2. Adiabatically turn on the optical lattice. We enter the Mott phase: 1 particle per site.

Entropy remains constant: temperature changes!

How to reach the Néel state: 2

8

3. When the temperature becomes cold enough, the fermions antialign. The entropy remains constant throughout.

How to reach the Néel state: 3

Prepare the system so that the initial entropy in the trap equals the final entropy below Tc in the lattice:

We need to know the entropy of the Néel state in the lattice.

To reach the Néel state:

SFG(Tini) = SLat(T ≤ Tc)

9

• Consider half filling, when we are deep in the Mott phase.

• Then, at low temperatures , the Hubbard model reduces to the Heisenberg model:

• Entropy of Néel state: perform mean-field analysis with as the mean field

Heisenberg Model

Usual spin-½ operator:

Superexchange constant (describes virtual hops):

hni

H =J

2

Xhjki

Sj · Sk

U À t

kBT ¿ U

S = 12σ

J =4t2

U

H ' J

2

Xhiji

½(−1)inSj + (−1)jnSi − Jn2

¾

10

0.02 0.04 0.06 0.080.0

0.2

0.4

0.6

ln(2)

T/TF

S/Nk B

Lattice EntropyTrap Entropy

Entropy of the Néel State

• Landau free energy:

Self-Consistency

Entropy

Heating

Cooling

S = −N ∂fL(hni)∂T

∂fL(n)

∂n

¯n=hni

= 0

hni

Lattice depth,6ER

Tc = 0.036 TF

kBTc = 3J/2

Mott

fL(n) =Jz

2n2 − 1

βln

∙cosh(

β|n|Jz2

)

¸− 1βln(2).

Née

l

11

Mean-Field Theory not accurate enough

0.02 0.04 0.06 0.080.0

0.2

0.4

0.6

ln(2)

T/TF

S/Nk B

Lattice EntropyTrap Entropy

No temperature dependence above Tc

is the correct limit.

Incorrect low temperature behavior

• Entropy exponentially suppressed.

• Model neglects spin wave excitations which dominate near T=0. They lead to power law suppression.

NkB ln(2) T →∞

12

2-Site Mean-Field Theory

1 2

• First Term: Treats interactions between two neighboring sites exactly,

• Second Term: Treats interactions between other neighbors within mean-field theory

H = JS1 · S2 + J(z − 1)|n|(Sz1 − Sz2) + J(z − 1)n2

Improve on standard mean-field approach by including 2 sites exactly:

13

2-Site Mean-Field Theory: Entropy

Successes:

•Correct temperature dependence at high temperatures.

Initial temperature to reach the Néel state is lower

Shortcomings:•Incorrect critical exponent and universal amplitude ratio

•Incorrect low temperature behavior: spin waves ( )absentT/T F

S/Nk B

0 0.02 0.04 0.06 0.080

0.1

0.2

0.3

0.4

0.5

0.6

0.7

1-site2-sitetrap

• Comparison with 1-site theory:

ωk ∝ |k|

14

Three temperature regimes:

• Low T: entropy of magnon gas

• High T: 2-site mean field theory result

• Intermediate T: non-analytic critical behaviour

Where, from renormalization group theory [Zinn-Justin]

S(T À Tc) = NkB

∙ln(2)− 3J2

64k2BT2

¸

S(T ¿ Tc) = NkB4π2

45

µkBT

2√3Jhni

¶3

d = 3, ν = 0.63, A+/A− ' 0.54

t =T − TcTc

→ 0±S(T = Tc) = S(Tc)±A±|t|dν−1

Tc = 0.957J/kBFrom quantum Monte-Carlo [Staudt et al. ’00]:

15

Achieving the Néel state in an Optical Lattice

Correct high-T, low-T and critical behavior of entropy in the latticeFinal temperature in the lattice can be found for all Tini < TF

0.02 0.04 0.06 0.080.0

0.2

0.4

0.6

ln(2)

T/TF

S/Nk B

Lattice, MFTLattice, fluc.Trap

Mott

Née

l

16

Concluding Remarks

• Néel state is reached with cold atoms by adiabatically ramping up an optical lattice. Corrections to mean-field theory reduce the initial temperature by ~20% but it remains experimentally accesible.

• Initial temperature close to limit of what is experimentally viable, accurate determination of the critical temperature is therefore crucial; fluctuations important.

• In principle our results form a lower bound to since we underestimate the entropy of the edge states of the Mott insulator.

Future research:• d=2 case: Start with d=3 Néel state then

decrease tunneling in one direction.• Doped lattices: population imbalance• Impurity scattering: introduce atoms of different species in the lattice

Insight into high-Tc SC

Tini

17

Maximum Number of Particles

For smooth traps, tunneling is not site-dependent, overfilling leads to double occupancy:

The trap limits the number of particles to avoid double occupancy:

Destroys Mott-insulator state in the centre!

N ≤ Nmax =4π

3

µ8U

mω2λ2

¶3/2Example:

atoms with a lattice depth ofand

40K

λ = 755 nm

8ER

⇒ Nmax ' 3 × 106

18

2-Site Mean-Field Theory: Order Parameter

0 0.5 1 1.50

0.1

0.2

0.3

0.4

0.5

k BT/J⟨n⟩

2-site1-site

Comparison with 1-site theory:

• Depletion at zero temperature due to quantum fluctuations

Tc ' 1.44kBJ

• Lowering of Tc:

19

Entropy, T>Tc

First term: Critical behavior

Other terms: To retrieve correct high-T limit of 2-site theory. → Found by expanding critical term and subtracting all terms of lower order than in T than high-T expression, which is .

•Result:

•Function with the correct properties above Tc:

S(T ≥ Tc)NkB

' α1

∙µT − TcT

¶κ− 1 + κTc

T

¸+ ln(2)

α1 =3J2

(32κ(κ − 1)k2BT 2c )κ = 3ν − 1 ' 0.89

∼ 1/T 2

20

Entropy, T<Tc

First term and last term: Critical behavior and continuousinterpolation with T>Tc result.

Other terms: Retrieve low-T behavior of magons, again found by expanding critical term and subtracting all terms of lower order than .

• Function for with the correct properties below Tc:

S(T ≤ Tc)NkB

= −α2∙µ

Tc − TTc

¶κ− 1 + κ

T

Tc− κ(κ− 1)

2

T 2

T 2c

¸+ β0

T 3

T 3c+ β1

T 4

T 4c

T 3

21

Entropy, T<Tc: Coefficients

• Result:

α1 =3J2

(32κ(κ− 1)k2BT 2c )κ = 3ν − 1 ' 0.89

(same as high-T expression):

α2 =6

(κ− 1)(κ− 2)(κ− 3)

µ4π2k3BT

3c

135√3J3− α1(κ− 1) + β1 − ln(2)

¶β0 =

κ

(κ− 3)

µ4π2k3BT

3c

45√3κJ3

+ α1(κ− 1)− β1 + ln(2)

¶β1 = ln 2− J2

6(A+/A− + 1) + κ(κ− 5)64κk2BT

2c A

+/A−− 4π

2k3BT3c

135√3J3

22

[MFT Details 1: Path Integral for Spins]

• For the unit vector:

• we define spin-coherent states obeying

• The partition function of Heisenberg model in terms of these states is a path integral for spins:

• is the vector potential of a monopole.

Ω =

⎛⎝sin θ cosφsin θ sinφcos θ

⎞⎠hΩ|S|Ωi = ~SΩ

Z =

ZDΩ(τ) exp

½−1~

Z ~β

0

∙Xj

i~SA(Ωj(τ))·∂Ω

∂τ+Xjk

Jjk2S2Ωj(τ)·Ωk(τ)

¸¾

|Ωi =mS=SXmS=−S

q2SCS+mS

eimSφ cosS+mS (θ/2) sinS−mS (θ/2)|S,mSi

A(Ωj(τ)) = ∇×Ωj(τ))

23

[MFT Details 2: Hubbard-Stratonovich]

• Hubbard-Stratonovich transformation to auxiliary field whichis on average related to the spins as

Result:

Where is the effective magnetic field at site j due to

all the other spins.

hmj(τ )i = hSΩj(τ)i

mj(τ)

Bj = −Xk

Jjkmk(τ)

Z =

ZDΩDm exp

(−1~

Z ~β

0

dτXj

"−Xk

Jjk2mj(τ)mk(τ)

− SBj ·Ωj(τ) + i~SA(Ωj(τ)) ·∂Ωj(τ)

∂τ

#)

24

[MFT Details 3: Free Energy]

To study antiferromagnets occurring when U>0,

• Introduce the staggered or “Néel” order parameter

• Consider nearest-neighbor interactions only: , etc.

• Next, integrate out the fields. For S= ½, this yieldsΩj(τ)

mj = (−1)jn

Jhjki = J

ZAFM 'ZDn exp

½− βNJzn2

2+N ln

∙2 cosh

β|nJz|2

¸¾≡ZDn e−βNfL