Introduction
CAQMP2019 (2019.07.16-08.08@ISSP, Kashiwa)
Introduction Naoki KAWASHIMA (ISSP) 2019.07.16 Sponsors Institute - - PowerPoint PPT Presentation
CAQMP2019 2019.07.16-08.08@ISSP, Kashiwa Introduction Naoki KAWASHIMA (ISSP) 2019.07.16 Sponsors Institute for Solid State Physics, University of Tokyo MEXT Project "Challenge of Basic Science" MEXT Project "Creation of
CAQMP2019 (2019.07.16-08.08@ISSP, Kashiwa)
Institute for Solid State Physics, University of Tokyo MEXT Project "Challenge of Basic Science" MEXT Project "Creation of new functional Devices and high-
performance Materials to Support next-generation Industries "
PCoMS "Program for Training Researchers for the Next Generation" (MEXT,Japan)
For a given Hamiltonian we want to compute expectation value of QMC is classical Monte Carlo in the space of world-line configurations
( )
( ) , , ,
1 1 4 4
i j i j k l ij p i j k l
H J S S Q S S S S
=
= − − −
=Q/J
SU(2) broken. Rotation not broken. SU(2) not broken. Rotation broken.
NK and Tanabe (2007)
to DCP Sandvik (2007)
Lou, et al (2009)
Senthil, et al, (2004): "Deconfined Criticality" A new type of phase transition. SU(N) JQ-Model
Pair of spinons are unbound as we approach the QCP
System-size-restricted finite-size scaling yields strongly size dependent estimates of scaling dimensions Harada et al (2013)
See Anders Sandvik's lecture and talk on July 22.
See A. Sandvik and and W.-N. Guo
arXiv:1905.13640 Monte Carlo calculation of RG flow diagram Classical 3D XY model with Z6 anisotropy It may be a good idea to think about the classical counterpart. One of the causes of difficulty may be the presence of the dangerously irrelevant field.
Monte Carlo Method is a general solution for the problem.
= → =
P Z
Paths) Feynman (
Metropolis However, what if ρ(π)<0 ?
3
− = J
3 spins on a triangle
the Hartree-Fock-Bogoliubov type wave function the quantum-number projector Gutzwiller-Jastrow factor X(β) : a matrix linear in F Computation of Pf(X) requires O(N^3) cpu time See M. Imada's lecture, and T. Misawa's talk
Jastrow: PR98 (1955); Gutzwiller: PRL10 (1963); Ceperley, Chester, and Kalos: PRB16 (1977); Sorella: PRB64 (2001); Tahara and Imada: JPSJ77 (2008)
= = =
=
1 1 2 1 , , , 1 TN
1 2 1 2
, , , Cont
S S N S S S S
N N
S S S T
physical (real) index virtual index
1
S
2
S
3
S
N
S
8
T
6
T
5
T
7
T
4
T
3
T
2
T
1
T
The state can be specified by only n tensors (i.e., ndk =O(N) variables) compared to dN variables necessary in general.
=
i i i i
T DPS Something more complicated but still manageable is necessary. Always yields some sort of mean-field approximation.
(0) Initialization (1) Hamiltonian of sub-systems (2) Hamiltonian of the whole system (3) Ground state (4) SVD (5) Renormalization (Doable with O(χ3)) Nishino may talk about this
contains pair Hamiltonian) Vanderstraeten's talk may be related to this For corner transfer matrix method, see Nishino and Okunishi, JPSJ65 (1996)
http://www.huffingtonpost.jp/2016 /03/12/alpha-go_n_9444998.html
2016.03 Alpha-Go defeated the world go-champion Lee Sedol multi-layer neural network
Corleo and Troyer 2016 Restricted Boltzmann machine
reinforced learning = variational principle
Monte Carlo sampling of the energy and its gradient wrt a, b and W, for gradient- descent method.
Why not using NN for quantum many body problems?
Negative-sign problem!
See Nomura's talk and Imada's lecture Extension to multi-layer (deep) neural networks was also investigated.
Back-propagation is tedious in NN coding. If this part can be taken care of by some software, the user only needs to design the network structure (data-flow graph). Automatic differentiation (AD) does this job, and it is supported by some libraries.
(Google) (Facebook)
Our calculation (TN included) is always of the form
See Hai-Jun Liao, Lei Wang, and Tao Xiang Hai-Jun Liao, Jin-Guo Liu, Lei Wang, and Tao Xiang, arXiv:1903.09650 Optimize the energy wrt the elementary tensor T
How about degeneracy? Is truncation of D differentiable?
Non-trivial technical problem, related to matrix diagonalization . Forward calculation A -> U and D
=
p p T
Z Cont
Ising
1
S
2
S
3
S
4
S
1
S
2
S
3
S
4
S
p
T
p
( )
( )
1 4 4 3 3 2 2 1 3 4 2 1
S S S S S S S S K S S S S p
e T
+ + +
=
i
Nishino, Hieida, et al., Prog. Theor. Phys. 105 (2001). Nishio, Maeshima, Gendiar, Nishino, cond-mat/0401115
A E e e
Foong & Kanno: PRL 72 1148 (1994)
... average with the invariant Haar measure ... dim. of Hilbert space of A
A
d m =
Ω A
For a randomly picked-up quantum state,
d d d E
L O L L O L O S =
− −
log
1 1
( )
const L SE + =
2
log 3 1
( )
1 −
=
d E
L O A a S
A
L
Finite-dimensional quantum states are very special
d(>1)-dim. free boson/fermion with a finite gap gapless fermionic chain
"area law" rather than "volume law"
( ) ( )
1 bond a
dim. O D = =
i
1 + i
= = =
−
1 1 1 2 1 1
1 1
T T T
Tensor Network States as Prototype of New Quantum States
AKLT state ... essentially equivalent to the Haldane state of S=1 AFH.
p
Z
p
X
Kitaev and Laumann, "Topological phases and quantum computation" (Oxford)
1 1 , − − =
p i z i p p i x i p z x B p p z A p p x
Z X J J Z J X J H
The simplest solvable model discussed heavily in the context of quantum information, topological phase, Majorana fermion, etc.
i A p x p
P
1 2 1 = = +
j i j i z j p x p
X P
= = = = = = = =
1 , 1 , 1 iff 1, 1
i i i
i
T
(
i i i
i i i
T
=
,
Cont
Exactly solvable model for gapless spin liquid
Kitaev, Ann. Phys. 321 (2006) 2 See Hyun-Yong Lee's seminar. The fact that exact solution is described in terms of Majorana fermions makes its physical picture hard to comprehend.
Exactly at the critical point.
... fully-polarized state in (111) direction
ψ0=LGS ψ1 ψ2 KHM gr. st. # of prmtrs. 1 2 E/J
ΔE/E 0.17 0.02 0.00007
with only two tunable parameters
See H.Y.Lee's seminar
Levin & Nave (2007); Gu, Levin, Wen (2008); Schuch, et al, (2007)
Eckhard-Young-Mirsky theorem: We can obtain the best LRA by truncating the small singular values.
Corboz, Rice, Troyer, PRL 113 (2014) See S. Morita's talk and T. Sakurai's talk
C(X) =
Solution (Corboz, Rice, Troyer, PRL 113 (2014))
Optimization condition for u, v and w RG transformation: converges faster when D increased can get rid of local entanglement
Evenbly and Vidal: Phys. Rev. Lett. 115, 180405 (2015)
By pinching the "information path", we can split the remaining loop, and remove them at the next contraction.
It is essential that this line is thin.
Evenbly and Vidal: PRL115, 180405 (2015) Also see, Yang, Gu, and Wen: PRL118, 110504 (2017), and Harada: PRB97_045124 (2018)
Stoundenmire and Schwab: Advances in Neural Information Processing Systems 29, 4799 (2016) b-dim. test training m= 10 0.05 0.05 m= 20 0.02 0.02 m=120 0.0097 0.0005
MPS and DMRG-like optimization can be used for pattern recognition.
COIL100 2D image classification task 128 x 128 x 3 x 7200 bits "open chain" "ring" Ring decomposition shows better performance.
maximum bond dim. average bond dim. tolerated error score (%) (large training) score (%) (small training)
Zhao, Cichocki ら arXiv:1606.05535 KNN classifier (K=1) applied to the image specifier core (Z4).
... but can we do that easily?
In TRG algorithm, a loop structure emerges in the tensor network. Such a loop entanglement is
However, once such a loop appears, it never vanishes.
Z1 Z2 Z3 Z4
(1) random initial tensors Zi (2) for i=1,2,3,4, update Zi by 2
T
Z1 Z2 Z3 Z4
-
min
Zi (3) repeat until the error converges
However, ALS is trapped by local loops.
( )
, , i pq i I p q
= 𝑓𝑗𝜚
When the given tensor T is a CDL, i.e., it must have the following form:
U V W
This tells us how we can
H.-Y. Lee and N.K. arXiv:1807.03862
4 16 16 16 16 4 4 4
2D Ising Model above Tc
Okuma, et al: Nat. Comm. (2019) Experiments + TN (PEPS + CTM) Characterization of magnetic plateaus. Effect of DM interaction.
Gapped/Gapless? What kind of spin liquid?
"Directed percolation" (Wikipedia) System with essential anisotropy (ν⊥≠ν||) Related topic: Kenji Harada (17th morning) 1/z≒0.63 Rényi entropy can be estimated! TEBD with TN representation
Surface physics can be dealt with.
also W.-N. Guo will talk about QMC approach on surface physics
surface magnetization scaling dimensions
Iino, Morita, NK, arXiv:1905.02351
Phase diagram of Finite-density QCD (early universe, neutron star, etc) ・ 1+1D relativistic fermion + U(1) gauge field (Schwinger model) ・ the next target may be 2+1D SU(2) gauge model
See Kuramashi's talk 2D φ4 model 4D Ising model
■Quantum Monte Carlo
■Variational Monte Carlo
■Tensor Network
■Machine Learming
■New Types of Quantum States
There'll be many other interesting topics.
Enjoy the event!