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Correlations and order parameters in infinite matrix product states - - PowerPoint PPT Presentation

Correlations and order parameters in infinite matrix product states Ian McCulloch Jason Pillay University of Queensland School of Mathematics and Physics December 6, 2019 Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 1 / 38


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Correlations and order parameters in infinite matrix product states

Ian McCulloch Jason Pillay

University of Queensland School of Mathematics and Physics

December 6, 2019

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 1 / 38

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Outline

1

Approaches to detecting quantum criticality

2

Cumulants

3

Examples Ising model

4

More complicated examples string order parameters SPT and time reversal BKT transition

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 2 / 38

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Approaches to detecting criticality

Bipartite fluctuations

Bipartite entropy Entanglement spectrum Bipartite fluctuations in quantum numbers (eg J. Stat. Mech. (2014) P10005 from Karyn le Her’s group; Kjall, Phys. Rev. B 87, 235106 (2013))

Transfer matrix spectrum

Eigenvalues λi λ0 = 1 by construction (normalization condition) Spectrum of correlation lengths ξi = −

1 ln λi

Or consider ǫi = − ln λi = 1/ξi – Behaves like an energy scale Choice of which quantity to use as the scaling variable

Scaling with respect to the bond dimension Scaling with respect to the correlation length – diverges at critical point Scaling with respect to δ = ǫ2 − ǫ1 (or some other combination of ǫi)

Order parameter and order parameter fluctuations (higher moments)

Lots of history behind finite-size scaling, can be modified for finite-entanglement scaling

  • J. Pillay and IPM, arXiv:1906.03833 (to appear in PRB)

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 3 / 38

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0.98 0.99 1 1.01 1.02 lambda 0.1 0.2 0.3 0.4 0.5 1/length

Inverse correlation length spectrum m=5

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 4 / 38

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0.98 0.99 1 1.01 1.02 lambda 0.1 0.2 0.3 0.4 0.5 1/length

Inverse correlation length spectrum m=6

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 4 / 38

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0.98 0.99 1 1.01 1.02 lambda 0.1 0.2 0.3 0.4 0.5 1/length

Inverse correlation length spectrum m=13

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 4 / 38

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0.98 0.99 1 1.01 1.02 lambda 0.1 0.2 0.3 0.4 0.5 1/length

Inverse correlation length spectrum m=16

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 4 / 38

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0.98 0.99 1 1.01 1.02 lambda 0.1 0.2 0.3 0.4 0.5 1/length

Inverse correlation length spectrum m=20

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 4 / 38

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0.98 0.99 1 1.01 1.02 lambda 0.1 0.2 0.3 0.4 0.5 1/length

Inverse correlation length spectrum m=25

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 4 / 38

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0.98 0.99 1 1.01 1.02 lambda 0.1 0.2 0.3 0.4 0.5 1/length

Inverse correlation length spectrum m=30

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 4 / 38

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0.98 0.99 1 1.01 1.02 lambda 0.1 0.2 0.3 0.4 0.5 1/length

Inverse correlation length spectrum m=40

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 4 / 38

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Higher moments

It is straight forward to evaluate a local order parameter, eg M =

  • i

Mi The first moment of this operator gives the order parameter, M = m1(L) It is also useful to calculate higher moments, eg M2 = m2(L)

  • r generally

Mk = mk(L) These are polynomial functions in the system size L.

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 5 / 38

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Cumulant expansions

Express the moments mi in terms of the cumulants per site κj, m1(L) = κ1L m2(L) = κ2

1L2 + κ2L

m3(L) = κ3

1L3 + 3κ1κ2L2 + κ3L

m4(L) = κ4

1L4 + 6κ2 1κ2L3 + (3κ2 2 + 4κ1κ3)L2 + κ4L

κ1 is the order parameter itself κ2 is the variance (related to the susceptibility) κ3 is the skewness κ4 is the kurtosis The cumulants per site κk are well-defined for a translationally invariant iMPS The moments (and hence cumulants) can be obtained directly as a polynomial-valued expectation value (arXiv:1008.4667) (I don’t know of a good way to calculate the cumulants per site for a finite system!)

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 6 / 38

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The cumulants have power-law scaling at a critical point, κi ∝ mαi Ising model example

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 7 / 38

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Scaling functions

For finite systems, scale with respect to system size L Control parameter h ≡ λ−λc

λc

Critical exponents

Exponent relation ν ξ ∝ |h|−ν β M ∝ (−h)β γ σ2 = M2 − M2 ∝ |h|γ Scaling relation 2β + γ = νd Note: no fluctuation-dissipation theorem: γ is not related to dM/dH.

Finite-size scaling functions

ξ = L X(h L1/ν) M = L−β/ν M(h L1/ν) σ2 = Lγ/ν G(h L1/ν) UL = U(h L1/ν) (Binder ratio)

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 8 / 38

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Finite entanglement

Effective ’system size’ L → mκ New scaling functions that scale with t mκ/ν.

Finite-entanglement scaling functions

ξ = mκ X(h mκ/ν) M = m−βκ/ν M(h mκ/ν) σ2 = mγκ/ν G(h mκ/ν) UL = U(h mκ/ν)

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 9 / 38

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Cumulant exponent relation

Following V. Privman and M.E. Fisher, Phys. Rev. B 30, 322 (1984)

Singular part of the free energy: f ≃ L−d Y

  • C1tL1/ν, C2hL(β+γ)/ν

Finite-entanglement version: f ≃ m−κd Y

  • C1tmκ/ν, C2hL(β+γ)κ/ν

Order parameter: κ1 = − ∂f ∂h = C2m−βκ/νY′ C1tmκ/ν, C2hL(β+γ)κ/ν Higher cumulants: κn = − ∂nf ∂hn = Cn

2m((n−2)β+(n−1)γ)κ/ν

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 10 / 38

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Cumulant exponent relation

This gives relation for all of the exponents (recall κn ∼ mαn) αn = [(n − 2)β + (n − 1)γ] κ ν α1 = −β α2 = γ This also works for α0 = −(2β + γ)κ/ν = dκ which is the correlation length exponent!

Alternative self-contained expression

αn = −(n − 2)α1 + (n − 1)α2

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 11 / 38

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Ising model example

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 12 / 38

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Ising model cumulant scaling functions

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 13 / 38

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Ising model correlation length scaling function

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 14 / 38

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Binder cumulant scaling

For finite systems, the Binder cumulant of the order parameter cancels the leading-order finite size effects UL = 1 − m4 3m22

0.25 0.5 0.75 1 0.18 0.2 0.22 0.24 L = 50 L = 100 L = 150 L = 200 iDMRG finite size scaling

|∆NL/2| Ω 0.2 0.4 0.6 0.8 0.18 0.2 0.22 0.24

L = 50 L = 100 L = 150 L = 200

UL Ω

0.4 0.425 0.215 0.216

The 2-component Bose-Hubbard model, with a linear coupling between components, has an Ising-like transition from immersible (small Ω) to miscible (large Ω).

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 15 / 38

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Binder Cumulant for iMPS

Naively taking the limit L → ∞ for the Binder cumulant doesn’t produce anything useful: if the order parameter κ1 = 0, UL = 1 − m4L 3m22

L

→ 2 3 if κ1 = 0, then m4(L) = 3k2

2L2 + k4L

Hence UL = 1 − 3k2

2L2 + k4L

3k2

2L2

→ 0 Finally, a step function that detects whether the order parameter is non-zero Better approach, in the spirit of finite-entanglement scaling: Evaluate the moment polynomial using L ∝ correlation length

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 16 / 38

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Choice of scaling parameter L = sξ is important!

s = 2 (top) and s = s∗ = 5.31 (bottom) chosen by optimisation For Ising model the point of intersection doesn’t depend so much on s, but important in other models!

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 17 / 38

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String parameters

Order parameters do not have to be local

Mott insulator string order parameter O2

P =

lim

|j−i|→∞Πj k=i(−1)nk

We can write this as a correlation function of ‘kink operators’, pi = Πk<i (−1)nk−1 This turns the string order into a 2-point correlation function: O2

P =

lim

|j−i|→∞ pi pj

Or as an order parameter: P =

  • i

pi MPO: P =

  • (−1)n−1

I I

  • Then O2

p = 1 L2 P2

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 18 / 38

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Example: Kondo lattice

J Pillay, IPM, Phys. Rev. B 97, 205133 (2018), arXiv:1906.03833 (PRB)

Simplified model of topological Kondo insulators suggested by Piers Coleman’s group M. Dzero, K. Sun, V. Galitski, and P

. Coleman, Phys. Rev. Lett. 104, 106408 (2010)

Kondo lattice with local + topological couplings, n = 1 particle per site H⊥ = J⊥

  • j
  • Sj ·

sj HK = JK

  • j
  • Sj ·

πj where π is a vector of non-local spins,

  • πj = 1

2

  • α,β

p†

j,α

σα,βpj,β pj,σ = 1 √ 2 (cj+1,σ − cj−1,σ)

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 19 / 38

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Topological Kondo chain

J⊥/JK large: topologically trivial insulator, Kondo singlet formation JK/J⊥ large: SPT protected by spatial reflection Phase transition between these two limits: charge gap vanishes but spin gap remains finite

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 20 / 38

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Order parameter for the insulating phases

The kink operators measure charge fluctuations crossing the boundary In this case, need to use pi = Πk<i (−1)

nk−1 2

to capture (spinless) 2-particle fluctuations O2

string = 1

L2 P2 gives scaling exponent β

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 21 / 38

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TKI cumulants

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 22 / 38

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TKI cumulant scaling functions

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 23 / 38

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TKI Correlation length scaling function

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 24 / 38

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TKI Binder Cumulant

The Binder cumulant is more problematic. s = 2 (top), s = s∗ = 5.29 (bottom)

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 25 / 38

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SPT transitions

Can use conventional string order parameter Sz(0) Πx−1

j=1 (−1)Sz(x) Sz(x)

Not universal – can deform state, string order parameter arbitrarily small Proper way to understand SPT: symmetry fractionalization

figure shamelessly stolen from Pollman and Turner, PRB 86, 125441 (2012)

Dihedral: UxUy = ±UyUx Time reversal: UτUτ∗ = ±1 Space refection: URUR∗ = ±1 Requires entanglement spectrum spectroscopy – not observable from the physical degrees of freedom

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 26 / 38

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Kink operator for time reversal

Time reversal operator τ = UK, τsατ −1 = −sα K = complex conjugation U = some basis-dependent unitary Normal basis: U = exp iπSy For an MPS, we can treat this as a local action τ(As) =

t s | U | t A∗t

Kink operator for time evolution: pτ(x) =

  • j<x

τ(j)

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 27 / 38

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String correlator pτ(0)pτ(x) Trivial phase: symmetric under time reversal, pτ(0)pτ(x) = 0 SPT phase: antisymmetric under time reversal, pτ(0)pτ(x) = 0 Order parameter: Pτ =

x pτ(x) has MPO form Pτ =

  • eiπSyK

I I

  • Can calculate P2

τ straightforwardly, and higher moments, P4 τ, etc

Example: S = 1 chain with single-ion anisotropy H = J

  • <i,j>

Si · Sj + D

  • i

(Sz

i)2

Transition from Haldane SPT to trivial phase at D ≃ 0.96845(8) Hu, Normand, Wang, Yu, PRB

84, 220402 (2011) Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 28 / 38

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S = 1 chain time-reversal order parameter cumulants

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 29 / 38

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S = 1 chain time-reversal cumulant scaling functions

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 30 / 38

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S = 1 chain time-reversal correlation length scaling function

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 31 / 38

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S = 1 chain time-reversal Binder cumulant

(a) s = 2, (b) s = 3, (c) s = s∗ = 3.12, (d) s = 4

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 32 / 38

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Bose-Hubbard model BKT transition

In 1D, there is no superfluid order, so the transition is from an ordered state (Mott insulator) to a critical region. String order parameter for the Mott transition: O2

Mott =

lim

|j−k|→∞

  • ✶j exp

 iπ

k

  • l=j

(ˆ nl − 1)   ✶k

  • ,

In the insulating phase, fluctuations in the density are short-ranged and O2

Mott = 0

In the superfluid phase, there are long-range (power-law) density fluctuations which drives O2

Mott → 0 (but not exactly zero for an MPS because correlation

length is finite! – we preserve U(1) particle number) At the BKT transition, the correlation length diverges more strongly than power-law ξ ∼ exp

  • 1

|J − Jc|ν

  • Ian McCulloch Jason Pillay (UQ)

iMPS December 6, 2019 33 / 38

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Bose-Hubbard model cumulants

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 34 / 38

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Bose-Hubbard model cumulant scaling functions

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 35 / 38

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Bose-Hubbard model correlation length scaling function

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 36 / 38

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Bose-Hubbard model BKT transition

Scaling function collapse of the Mott string order parameter predicts Jc = 0.2850 ± 0.0005 (1) κ = 1.275 ± 0.001 (2) β = 0.375 ± 0.001 (3) γ = 0.350 ± 0.005 (4) The obtained κ differs from the expected c = 1 result by ∼ 5.1%. Jc differs quite significantly from other recent works, eg Jc = 0.3048(3)

  • btained by Rams et al with m = 4000 states and ǫ scaling.

Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 37 / 38

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Summary

MPO techniques for higher moments Scaling functions work very well for detecting critical points Correlation length scaling function is simplest case, perhaps easiest Binder cumulant – not as easy to use as we hoped String order parameters – same scaling properties as local order parameters Time reversal as a string order parameter Spatial reflection can be considered in a similar way Our approach still involves scaling with respect to bond dimension – want to avoid this!

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Ian McCulloch Jason Pillay (UQ) iMPS December 6, 2019 38 / 38