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Emergent large N matrices from a nonlocal spin system Victoria Martin Stanford University July 6-31 2015 Based on: arXiv:1412.1092 [hep-th] By: Dionysios.

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Presentation on theme: "Emergent large N matrices from a nonlocal spin system Victoria Martin Stanford University July 6-31 2015 Based on: arXiv:1412.1092 [hep-th] By: Dionysios."— Presentation transcript:

1 Emergent large N matrices from a nonlocal spin system Victoria Martin Stanford University July 6-31 2015 Based on: arXiv:1412.1092 [hep-th] By: Dionysios Anninos, Sean Hartnoll, Liza Huijse, VM Holographic duality for condensed matter physics KITPC Beijing

2 Dionysios Anninos, IASLiza Huijse, SITPSean Hartnoll, SITP Emergent large N matrices from a nonlocal spin system

3 Introduction Large NxN MatricesEmergent Spacetime For example, [hep-th/9610043]

4 Introduction Large NxN MatricesEmergent Spacetime

5 Introduction Large NxN MatricesEmergent Spacetime Quantum Spin System

6 Introduction Large NxN MatricesEmergent Spacetime Quantum Spin System Why? 1) Use matrix integral techniques to study spin systems 2) Understand emergent locality, etc using known results of quantum information 3) Study nontrivial emergence of continuous symmetry (SO(N)) from discrete 4) Study novel phase transition involving topological order, not symmetry breaking

7 Outline Introduce the system and its symmetries Emergence of matrix integral with SO(N) symmetry Solving the matrix integral; Results Monte Carlo verification Discussion

8 The system: A nonlocal Ising model N N Note: 1)We will study the ferromagnetic case, λ<0 2)We use the trace structure to make connection with bosonic matrices later

9 The system: A nonlocal Ising model N N

10 N N Discrete symmetries: 1)S N x S N – Permuting rows or columns 2)Z 2 N x Z 2 N – Flipping all spins in a row or column

11 Finite Temperature Partition Function

12 H-S Field

13 Finite Temperature Partition Function H-S Field Denef, arXiv:1104.0254 [hep-th]

14 Finite Temperature Partition Function

15 Partition Function: Focus on z(Q)

16 H-S Vector

17 Partition Function: Focus on z(Q) H-S Vector

18 Partition Function: Focus on z(Q)

19

20

21

22 We see: From: We see: From:

23 Partition Function: Focus on z(Q) Rescale z(Q): This removes part of the trace of Q: Cugliando, Kurchan, Parisi, Ritort [cond-mat/9407086]

24 Partition Function: Focus on z(Q) Rescale z(Q): This removes part of the trace of Q: Cugliando, Kurchan, Parisi, Ritort [cond-mat/9407086] cf:

25

26 Solving the Matrix Integral Rotate eigenvalue basis: Brezin, Itzykson, Parisi, Zuber 1978. Note:

27 Solving the Matrix Integral Introduce eigenvalue distribution: EOM in large N limit: Brezin, Itzykson, Parisi, Zuber 1978.

28 Solving the matrix integral Evidence of metastability

29 Solving the matrix integral Evidence of metastability

30 Monte Carlo First order phase transition

31 Monte Carlo For a first order phase transition, the canonical distribution is doubly peaked near the transition temperature. The transition temperature occurs when the peaks are the same height. Canonical distributionDensity of states Matrix integral saddleGround states

32 Monte Carlo

33 Order and Disorder Low temperature saddle -> ordered phaseMatrix integral saddle -> disordered phase

34 Ferromagnetic vs Antiferromagnetic model 1)High temperature phase related to a matrix integral 2)Low temperature phase exhibits frustration and glassiness 3)Existence of phase with disconnected eigenvalue distribution Cugliando, Kurchan, Parisi, Ritort 1994 AF F

35 Conclusions

36 Future Directions


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