Quantum Hamiltonian Complexity Itai Arad Centre of Quantum - - PowerPoint PPT Presentation

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Quantum Hamiltonian Complexity Itai Arad Centre of Quantum - - PowerPoint PPT Presentation

Quantum Hamiltonian Complexity Itai Arad Centre of Quantum Technologies National University of Singapore QIP 2015 1 18 / Quantum Hamiltonian Complexity condensed complexity QHC matter theory physics Local Hamiltonians 2 18 / Local


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1 18 /

Quantum Hamiltonian Complexity Itai Arad

Centre of Quantum Technologies National University of Singapore

QIP 2015

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2 18 / Quantum Hamiltonian Complexity

condensed matter physics complexity theory QHC Local Hamiltonians

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3 18 / Local Hamiltonians

Describe the interaction of quantum particles (spins) that sit on a lattice

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4 18 / Thermal equilibrium

Heat bath at temperature T

Thermal contact

partition function In the diagonalizing basis of H:

Much like a classical k-SAT system!

Gibbs state

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5 18 / Main questions in quantum Hamiltonian complexity:

What is the complexity of: Approximating the ground energy Approximating the Gibbs state at temperature T (and local

  • bservables)

Approximating the time evolution Valuable insights into the physics of the systems:

  • structure of entanglement
  • correlations
  • phase transitions and criticality
  • different phases of matter

Develop algorithms (classical and quantum) to study these systems

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6 18 /

Formal definition:

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7 18 / Examples

Heisenberg model:

... ... ... ... ... ... ... ...

Ising model w. transverse field:

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8 18 / Local Hamiltonians as quantum generalizations of k-SAT forumas

Classical Classical (quantum notation) Quantum

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9 18 / The Local Hamiltonian Problem (LHP)

In other words: LHP

Central result: the "quantum Cook-Levin" theorem (Kitaev, '00)

The LHP with is QMA complete (QMA = quantum NP)

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10 18 / Classifying the landscape of local Hamiltonians

Kitaev's 5-local Hamiltonian:

... ...

hard Hamiltonians (QMA) Easy to show for: easy Hamiltonians (P,NP) Easy to show for: non-interacting, classical, many-symmetries Physically interesting Hamiltonians

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10 18 / Classifying the landscape of local Hamiltonians

Kitaev's 5-local Hamiltonian:

... ...

hard Hamiltonians (QMA) Easy to show for: easy Hamiltonians (P,NP) Easy to show for: non-interacting, classical, many-symmetries Physically interesting Hamiltonians

(Kempe, Kitaev & Regev '04) (Hallgren et al '13) (Aharonov et. al. '07) (Oliveira & Terhal '05) (Cubitt & Montanaro, '13) (Schuch \& Verstraete '07) (Bravyi & Vyalyi '03) (Bravyi '06) (Hastings '07) (Landau et al '13)

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11 18 / A (bold) conjecture

In 1D this has been proved by Landau, Vazirani & Vidick '13 In higher D the problem is wide open.

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12 18 / An intermediate outline

Why gaps matter: AGSPs The detectability-lemma AGSP and the exponential decay

  • f correlations

The Chebyshev AGSP and the 1D area-law Matrix-Product-states, and why the 1D problem is inside NP 1D algorithms 2D and beyond: tensor-networks, PEPs and possible directions to proceed

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13 18 / The grand plan

To show that a class of LHP is inside NP (or P), we can try to show that the ground state admits an efficient classical description: In such case we can simply use as a classical witness for the LHP problem since:

local operators

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14 18 / Locality in ground states: AGSPs

How can we find an efficient classical description? product state general state If has a simple local structure then this could teach us about the local structure of AGSP (Approximate Ground Space Projector) We need locality to bridge that gap

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15 18 /

Exp' decay of correlations (Hastings '05) In the G.S. of a gapped system the correlation function decays exponentially

Exponential decay of correlations

We will use an AGSP to prove this for gapped frustration-free systems:

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Proof:

The detectability lemma

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17 18 / Conclusion:

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18 18 / Exponential decay of correlations using the detectability-lemma AGSP

...

Even layer: Odd layer:

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... ... ... ... ... ... ... ... ... ...

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1 18 / Area laws

Schmidt decomp': Entanglement entropy: Volume law Area law

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2 18 / The area law conjecture

Conjecture Ground states of gapped local Hamiltonians on a lattice satisfy the area law Intuitive explanation: Exponential decay

  • f correlations

However, So far, only the 1D case has been proved rigoursly (Hastings' 07) Only the degrees of freedom along the boundary are entangled

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3 18 / An AGSP-based proof for the 1D area-law

(w. Aharonov, Kitaev, Landau & Vazirani)

... ... The 1D area-law: Outline: AGSP Our main object:

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AGSP Assume: Then:

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5 18 / The bootstrapping lemma

Lemma Proof:

Then on the one hand: On the other hand: (1) Plugging into (1), we get:

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6 18 / Good AGSPs are hard to find...

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The detectability lemma AGSP Only one projector increases the S.R., but still...

A different approach: Example: Can we do better?

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7 18 / Chebyshev-based AGSP

(rescaled)

Chebyshev Polynomial

Compare with:

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8 18 / Other ingredients in the proof

Schmidt rank: Taking all these points together, one constructs a Chebyshev-based AGSP with

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9 18 / Constructing a Matrix-Product-State (MPS)

... ... ...

...

we can truncate at each cut Canonical MPS: (Vidal '03) This is a poly(N) description. But is it also efficient?

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10 18 / MPS as tensor-networks

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vertices ↔ tensors

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connected edges ↔ contracted indices. Tensor-network: edges ↔ indices

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11 18 / Calculating with MPS

... ... ... ...

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... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ...

Contracting a tensor-network: the swallowing bubble

At every step of the algorithm the bubble

  • nly cuts a constant

number of edges, whose total indices span over at most a polynomial range Calculating a local observable of an MPS can be done efficiently!

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13 18 / Summary of the 1D is inside NP argument

The MPS can be used as a classical witness to show that 1D gapped LHP is inside NP

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14 18 / Algorithms for finding the g.s. of gapped 1D systems

Density Matrix Renormalization Group (DMRG) (White '92) Equivalent for locally optimizing the MPS (Rommer & Ostlund '96)

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TEBD (Vidal '03) Dynamical programing (Landau, Vazirani & Vidick '13) A random algorithm that rigrously converges to the g.s. with high

  • probability. Based on applying Dynamical Programming to MPSs
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15 18 / 2D and beyond

We cannot hope for an efficient problem because already the classical problem (SAT in 2D) is NP hard However, by finding an efficient classical representation we may revolutionize the field like DMRG did in 1D Current approaches: use 2D tensor networks such as PEPS (taken from Orùs '13)

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16 18 / The difficulties in 2D

PEPS states naturally satisfy the 2D area-law. However, the 2D area-law proof is still missing... Even if we had a 2D area-law proof, it would still not prove that the g.s. is well-approximated by a PEPS Even if the g.s. was known to be approximated by a PEPS, it is still not clear how to efficiently compute local observables with PEPS

general states Area-law states PEPS states Gapped g.s. (conjecture)

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17 18 / But there's hope

general states Area-law states PEPS states Gapped g.s. (conjecture)

A 2D area-law proof would (if found) surely teach us much more about the structure of the g.s. than merely the area-law itself. Contracting a PEPS exactly is #P hard. However, we are not fully using the fact that we are interested in very special PEPS: Those that represent gapped g.s. Some numerical evidences suggest that this can be done efficiently (Cirac et al '11) There is much more structure (i.e., exp' decay of correlations), which can be used to prove efficient contraction.

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Thank you !