Improvement of the higher-order tensor renormalization group method - - PowerPoint PPT Presentation

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Improvement of the higher-order tensor renormalization group method - - PowerPoint PPT Presentation

Improvement of the higher-order tensor renormalization group method Satoshi Morita (ISSP , Univ. Tokyo) 2 Outline Introduction Real-space renormalization based on TN How to calculate a projector in HOTRG Calculation of


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Satoshi Morita (ISSP , Univ. Tokyo)

Improvement of the higher-order tensor renormalization group method

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Outline

○ Introduction

➢ Real-space renormalization based on TN ➢ How to calculate a projector in HOTRG

○ Calculation of higher-order moments by HOTRG

➢ Renormalization of multi-impurity tensors ➢ Finite-scaling analysis on q-state Potts model

○ Entanglement filtering in HOTRG

➢ HOTRG + Full Environment Truncation (FET)* ➢ Benchmark on 2d Ising model*

○ Summary

2

* Unpublished results are removed in this PDF.

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Tensor network methods

○ Hamiltonian mechanics

➢ Wave function of many-body systems

○ Lagrangian mechanics

➢ Partition function (Action)

𝑃 𝑒𝑂 coefficients 𝑃 𝑒𝑂 terms Tensor network representations reduce exponential computational cost to polynomial order.

  • Approx. by tensor decomp.

Representation by tensor decomp.

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TN representation of the partition function

Sum over states Tensor contraction

  • Tensor index corresponds to spin direction.
  • One tensor contains two spin.
  • In higher dimensional systems, a tensor has many indices (=2𝑒).

𝑇1 𝑇2 𝑇4 𝑇3 𝑇1 𝑇2 𝑇4 𝑇3

𝐵𝑇1𝑇2𝑇3𝑇4 = 𝑓𝐿 𝑇1𝑇2+𝑇2𝑇3+𝑇3𝑇4+𝑇4𝑇1

Ising model 𝐵

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TN representation of the partition function

5

Sum over states Tensor cont. Local Boltzmann factors

  • Bond index is index of eigenvalue.
  • Spin is already traced out.
  • One tensor contains one spin.
  • # of indices is 2𝑒.

𝜀 𝑦 𝑧′ 𝑧 𝑦′ 𝜏 𝜀𝑦𝑧𝑦′𝑧′

𝜏

= 𝜀𝜏𝑦𝜀𝜏𝑧𝜀𝜏𝑦′𝜀𝜏𝑧′ 𝑋 𝑋 𝑊 𝑊 𝜀 𝜀 𝑋

=

Λ 𝑉 𝑉† ED

=

𝑌 = 𝑉 Λ 𝑌† 𝑌† 𝑌 𝑌 𝜀 𝑊 𝑌† 𝑈

=

Kronecker’s delta

𝑈 𝑈 𝑈 𝑈

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Real-space renormalization group

○ TRG

Tensor Renormalization Group

○ HOTRG

Higher-order Tensor Renormalization Group

Levin, Nave (2007) Xie, et al. (2012)

https://github.com/smorita/TN_animation

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Real-space renormalization

○ TRG (Tensor Renormalization Group)

Levin, Nave (2007)

Decomposition & Contraction 𝑃 𝜓6 𝐵 Contraction Truncated SVD 𝑃 𝜓5

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TRG-base methods

○ TNR (Tensor Network

Renormalization)

○ Loop-TNR ○ TNR+

Bal, et al. (2017) Evenbly, Vidal (2015) Yang, Gu, Wen (2017)

○ 𝑃 𝜓5 algorithms

➢ TRG + Randomized SVD

SM, Igarashi, Zhao, Kawashima (2018)

➢ Projectively Truncated TRG

Nakamura, Oba, Takeda (2019)

Only for 2-d systems

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HOTRG

○ Higher-order Tensor Renormalization Group

Xie, et al. (2012)

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Advantage of HOTRG

TRG HOTRG 2D Ising 𝜓 = 24

➢Higher-dimensional systems

𝑃 𝜓11

➢Accuracy

➢ Conservation of lattice structure ➢ No tensor decomposition

✓ 3-state Potts model on cubic lattice

Wang, et al., (2014) [arXiv:1405.1179]

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Key parts of HOTRG

○ Renormalization

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○ HOSVD (Higher-Order Singular Value Decomposition)

➢ truncated Tucker decomposition 𝑉 𝑉† 𝐵𝑢 𝐵𝑢 𝐵𝑢+1 =

=

CPU cost: 𝑃 𝜓7 Memory: 𝑃(𝜓4)

𝑉 𝑉′

𝑇

HOSVD

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Key parts of HOTRG

○ Renormalization

12

○ HOSVD (Higher-Order Singular Value Decomposition)

➢ truncated Tucker decomposition 𝑉 𝑉† 𝐵𝑢 𝐵𝑢 𝐵𝑢+1 =

𝑉 𝑊† Σ

truncated SVD

𝐵𝑢

CPU cost: 𝑃 𝜓7 Memory: 𝑃(𝜓4)

𝐵𝑢 𝐵𝑢

𝐵𝑢

† CPU cost: 𝑃 𝜓6 𝜓 𝜓

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Optimal Projector for 2x2 Cluster

○ Problem

13 𝑄𝑀 𝑄𝑆

Δ = min

𝑄, 𝑅 Lower bound

=

𝑉𝑢 𝑊

𝑢 †

Σ𝑢

Truncated SVD Δ ≥ ෍

𝑗>𝜓

𝜏𝑗

2

2

𝑄𝑀 𝑄𝑆

𝑉𝑢 Σt 𝑊

𝑢 †

Σt

= =

How do we obtain 𝑄𝑀 and 𝑄𝑆 satisfying the follow conditions? 𝑈

1

𝑈2 𝑈3 𝑈

4

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Algorithm based on QR decomposition

14

𝐵𝑀

=

𝑅𝑀 𝑆𝑀 𝐵𝑆

=

𝑅𝑆 𝑆𝑆 𝑆𝑀 𝑆𝑆

෩ 𝑉𝑢 ෨ 𝑊

𝑢 †

Σ𝑢 truncated SVD

𝑄𝑀

𝑆𝑆 ෨ 𝑊

𝑢

Σ𝑢

− Τ 1 2

= 𝑄𝑆 =

𝑆𝑀 Σ𝑢

− Τ 1 2

෩ 𝑉𝑢

Wang, Verstraete, arXiv:1110.4362, Corboz, Rice, Troyer, PRL 113, 046402 (2014)

QR RQ

𝑄𝑀𝑄𝑆 is an “oblique” projector

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Derivation of “Oblique” Projector

15 ≡

𝐵𝑀 𝐵𝑆

𝐵𝑀𝐵𝑆 = 𝑉 Σ 𝑊† ≈ 𝑉𝑢 Σ𝑢 𝑊

𝑢 † SVD truncation

𝐵𝑀𝑄𝑀 = 𝑉𝑢 Σ𝑢 𝐵𝑀 = 𝑅𝑀𝑆𝑀 𝐵𝑆 = 𝑆𝑆𝑅𝑆

QR decomp. RQ decomp.

𝑆𝑀𝑆𝑆 = ෩ 𝑉 Σ ෨ 𝑊† = ෩ 𝑉𝑢 Σ𝑢 ෨ 𝑊

𝑢 † SVD truncation

= 𝑉Σ𝑊† 𝑊

𝑢Σ𝑢 − Τ 1 2

= 𝐵𝑀𝐵𝑆 𝑊

𝑢Σ𝑢 − Τ 1 2

= 𝐵𝑀 𝑆𝑆𝑅𝑆 𝑊

𝑢Σ𝑢 − Τ 1 2

= 𝐵𝑀 𝑆𝑆 ෨ 𝑊

𝑢Σ𝑢 − Τ 1 2

𝑉𝑢 = 𝑅𝑀 ෩ 𝑉𝑢 𝑊

𝑢 † = ෨

𝑊

𝑢 †𝑅𝑆

෨ 𝑊

𝑢 = 𝑅𝑆𝑊 𝑢

𝑄𝑀 𝑄𝑆 = Σ𝑢

− Τ 1 2 ෩

𝑉𝑢

†𝑆𝑀

෩ 𝑉𝑢

† = 𝑉𝑢 †𝑅𝑀 In the same way, we obtain We can easily prove 𝑄𝑀𝑄

𝑆 = 𝑄𝑀𝑄𝑆 2.

Comparing two SVDs, we obtain × Σ𝑊†𝑊Σ𝑢

− Τ 1 2

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Computational Cost

16

𝐵𝑀

=

𝑅𝑀 𝑆𝑀 𝐵𝑆

=

𝑃 𝜓8 𝑅𝑆 𝑆𝑆 𝑆𝑀 𝑆𝑆

෩ 𝑉𝑢 ෨ 𝑊

𝑢 †

Σ𝑢 truncated SVD 𝑃 𝜓6 Cost

𝑄𝑀

𝑆𝑆 ෨ 𝑊

𝑢

Σ𝑢

− Τ 1 2

= 𝑄𝑆 =

𝑆𝑀 Σ𝑢

− Τ 1 2

෩ 𝑉𝑢

𝑃 𝜓4

Wang, Verstraete, arXiv:1110.4362, Corboz, Rice, Troyer, PRL 113, 046402 (2014)

For HOTRG, 𝑃(𝜓8) cost is unacceptable. We can avoid the QR decomp by using ED because 𝑅𝑀 and 𝑅𝑆 is unnecessary. QR RQ

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Modified Algorithm for “Oblique” Projector

17

𝑃 𝜓8 Cost

  • cf. Iino, SM, Kawashima, arXiv:1905.02351, to be published in PRB

𝐵𝑀

𝐵𝑀 𝑉 𝑉† Λ

=

ED 𝑆𝑀

𝑉 Λ Use Λ 𝑉 instead of 𝑆𝑀

HOSVD Oblique Modified HOSVD Oblique Modified

➢ Benchmark on random tensors

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Boundary Tensor Renormalization Group

○ HOTRG with open boundaries

18

Iino, SM, Kawashima, arXiv:1905.02351, to be published in PRB

Index

Scaling dimension of boundary CFT

Ising model 𝑈 = 𝑈

𝑑

𝜓 = 72

Iino’s talk

July 22, 15:30-

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19

1st Part:

Higher-order moments by Higher-order Tensor Renormalization Group

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Finite-size scaling analysis

Binder ratio

  • K. Binder: Z. Phys. B 43, 119 (1981)

✓ Dimensionless quantity ✓ Step function in 𝑂→∞ ✓ Crossing point → 𝑈

𝑑

(Ising model) 2D Ising MC 𝑢𝑀 Τ

1 𝜉

𝜉 = 1

Magnetization 2D Ising MC

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Order parameter 𝒏

  • 1. Derivative of free energy

➢ Error from numerical differential approximation. ➢ External field breaks symmetry of tensor.

  • 2. Impurity tensor

Tr 𝑇𝑗 𝑓−𝛾𝐼 = tTr Multi-point correlations are necessary for high-order moments 𝑛𝑜 .

2D Ising model, 𝑈 = 𝑈

𝑑

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Multipoint correlation functions

+ + + … + + + …

1 𝑂 1 𝑂2

𝑇1𝑇1 𝑇1𝑇2 𝑇1𝑇3 𝑇1 𝑇2 𝑇3 𝑂 terns 𝑂2 terns

We calculate the renormalized tensor of the summation of multipoint correlation functions by using HOTRG.

➢ 1st-order moment ➢ 2nd-order moment

𝐵𝑢

1

𝐵𝑢

2

≃ ≃

“the average of the local operators”

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Renormalization of multi-impurity tensors

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  • Use the same isometry 𝑉(𝑢) for the local tensor 𝑈(𝑢)
  • Generalization for multiple kinds of impurities

Renormalization of multi-impurity tensors

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2D 𝑟-state classical Potts model

○ Phase transition at

➢ 𝑟 ≤ 4 : 2nd-order ➢ 𝑟 > 4 : 1st-order ➢ Correlation length 26

We consider ℎ = 0. Weakly 1st-order

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TN representation

○ Local tensor

27

Eigen value of local Boltzmann factor

𝑎𝑟 symmetry

○ Order parameter

➢ Complex magnetization ➢ Impurity tensor for 𝑛𝑙𝑛∗𝑙′

Covariant with spin rotation (charge 𝑙 − 𝑙′)

𝑦 + 𝑧 − 𝑦′ − 𝑧′ ≡ 0 mod 𝑟 𝑦 + 𝑧 − 𝑦′ − 𝑧′ ≡ 𝑙 − 𝑙′ mod 𝑟

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Magnetization

28

𝑂 = 240 𝜓 = 48 ➢ Ising model (𝑟 = 2) ➢ 𝑟-state Potts model

𝑈(𝑢) 𝑂 = 2𝑢 Periodic BC 𝑂 = 220 𝜓 = 32

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𝜓-dependence

Ising model Τ 𝑈 𝑈

𝑑

Binder ratio

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Transition temperature

Bisection search

Τ 𝑈 𝑈

𝑑 = 0.999951171

Τ 𝑈 𝑈

𝑑 = 1.000007324

Τ 𝑈 𝑈

𝑑 = 1.00000313922

Τ 𝑈 𝑈

𝑑 = 1.00000313960

  • Estimated values converge to the exact value with oscillation
  • Relative error seems to decay in proportion to 𝜓−3.5

𝜓-dependence

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Finite-size scaling analysis

31

4-state Potts model 5-state Potts model Τ 1 𝜉 = 2 𝛾 = 0

Τ 1 𝜉 = Τ 3 2 𝛾 = Τ 1 12

Exact

✓ Fitting by Bayesian scaling (Harada, 2011) ✓ Effect of logarithmic correction is small ✓ No fitting ✓ Plateau indicate the 1st-order phase transition.

Δ𝑛 2

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Slope of Binder ratio

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Summary of the 1st part

○ Renormalization of tensors with multiple impurities

𝑂 = 240 𝐸 = 48 Magnetization of Potts model

SM and N. Kawashima, Comput. Phys. Comm 236, 65 (2019)

# of states

✓ Beyond the system size which the Monte-Carlo method can treat. ✓ Finite-size scaling analysis of the magnetization and the Binder ratio. ✓ Distinguish weakly first-order and continuous phase transitions

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34

2nd Part:

HOTRG with entanglement filtering

Unpublished results are removed in this part.

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Internal Correlations

➢ Irrelevant correlations with 𝑃(1) length scale ➢ Converge to a fictitious fixed-point tensor

  • Corner Double Line structure

We need to remove internal correlations within a loop. “Entanglement Filtering”

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Internal Correlations

➢ Irrelevant correlations with 𝑃(1) length scale ➢ Converge to a fictitious fixed-point tensor

  • Corner Double Line structure

We need to remove internal correlations within a loop. “Entanglement Filtering”

Gu, Wen (2009)

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TRG with Entanglement Filtering

○ TRG-base methods

➢ TEFT [Gu, Wen (2009)] ➢ TNR [Evenbly, Vidal (2015)] ➢ loop-TNR [Yang, Gu, Wen (2017)] ➢ TNR+ [Bal, et al, (2017)] Only for 2-d systems

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Entanglement Filtering

○ TRG-base methods

➢ TEFT [Gu, Wen (2009)] ➢ TNR [Evenbly, Vidal (2015)] ➢ loop-TNR [Yang, Gu, Wen (2017)] ➢ TNR+ [Bal, et al, (2017)]

○ General methods

➢ Graph Independent Local Truncation [Hauru, Delcamp, Mizera (2017)] ➢ Tensor Network Skeletonization [Ying (2016)] ➢ Entanglement Branching [Harada (2018)] ➢ Full Environment Truncation [Evenbly (2018)] Only for 2-d systems We consider a combination with HOTRG and FET.

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Full Environment Truncation (FET)

Optimize isometries 𝑣, 𝑤 and bond diagonal matrix ෤ 𝜏

𝐵𝐶 to minimize

the difference

Evenbly (2018)

✓ Simple criterion ✓ TRG + FET

TRG TRG+FET

෤ 𝜓 < 𝜓

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Thank you for your attention!