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Quantum simulations of high-energy physics models MAX-PLANCK INSTITUT FÜR PHYSIK January 27th, 2015 In collaboration with J. Pachos (Leeds) S. Kühn B.

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Presentation on theme: "Quantum simulations of high-energy physics models MAX-PLANCK INSTITUT FÜR PHYSIK January 27th, 2015 In collaboration with J. Pachos (Leeds) S. Kühn B."— Presentation transcript:

1 Quantum simulations of high-energy physics models MAX-PLANCK INSTITUT FÜR PHYSIK January 27th, 2015 In collaboration with J. Pachos (Leeds) S. Kühn B. Reznik (Tel-Aviv) E. Zohar M.C. Banuls

2 When we get to the very, very small world we have a lot of new things that would happen that represent completely new opportunities for design. „There is plenty of room at the bottom“ Ricard Feynman, 29.12.1959. Annual meeting of the American Physical Society, CALTECH Atoms on a small scale behave like nothing on a large scale, for they satisfy the laws of quantum mechanics. We are working with different laws, and we can expect to do different things. QUANTUM PHYSICS

3 PROGRESS

4 QUANTUM SIMULATION

5 OUTLINE Simulating many-body systems Analog quantum simulation Cold atoms in optical lattices Quantum simulation of HEP models Tensor Networks and HEP models

6 SIMULATING MANY-BODY SYSTEMS

7 PHYSICAL SYSTEMMODEL Model Hamiltonian MANY-BODY SYSTEM MODELS Computation time/memory scales exponentially with the number of constituents Thermal equilibrium (T) Dynamics

8 Impossible if N>100 ConfigurationEnergy There are different configurations EXAMPLE: classical spins MANY-BODY SYSTEM CLASSICAL MODELS Which is the spin configuration at T=0?

9 Ferromagnetic Symmetries: simple EXAMPLE: classical spins + SYMMETRIES The problem is difficult in general (NP-Hard) In practice, it may turn to be simple MANY-BODY SYSTEM CLASSICAL MODELS Which is the spin configuration at T=0?

10 PHYSICAL SYSTEMMODEL Model Hamiltonian Which is the spin configuration at T=0? MANY-BODY SYSTEM QUANTUM MODELS

11 N. spinesMemory 128 bytes 150 Tbytes 10 29 bytes 10 150 bytes Quantum spins: QUANTUM SIMULATIONS QUANTUM SYSTEMS Symmetries do not help much

12 Quantum superpositions are responsible for many physical phenomena: Superconductivity Superfluidity Giant magnetoresistence Nuclear reactions Insulators (Mott, Anderson, topological) Quark confinement Chemical reactions QUANTUM SIMULATIONS QUANTUM SYSTEMS There are many theoretical techniques In some relevant problems they fail

13 ANALOG QUANTUM SIMULATION

14 QUANTUM SIMULATORS

15 QUANTUM SIMULATOR MODEL Model Hamiltonian QUANTUM SIMULATORS ANALOG

16 Questions: Ground state: Dynamics: Physical properties: Thermal state: QUANTUM SIMULATORS

17 Dynamics: How does it work? Ground state: HamiltoniansStates QUANTUM SIMULATORS ANALOG

18 COLD ATOMS IN OPTICAL LATTICES

19 COLD ATOMS Trapping: Cooling: lasersevaporation Internal manipulation lasers RF fields purification coherence detection Magnetic fields lasers Interactions Control: External fields tune scattering length

20 Degeneracy: bosons and fermions (BE/FD statistics) Coherence: interference, atom lasers, four-wave mixing, … Superfluidity: vortices Disorder: Anderson localization Fermions: BCS-BEC + many other phenomena Many-body phenomena COLD ATOMS ACHIEVEMENTS

21 Cold atoms are described by simple quantum field theories: We can have bosons or fermions (or both). The external potential, V, and interaction coefficients, u, can be engineered using lasers, and electric and magnetic fields. In certain limits, one obtains effective theories that are interesting in other fields of Physics. Quantum Simulations We can have different internal states (spin). COLD ATOMS

22 OPTICAL LATTICES Laser standing waves: dipole-trapping

23 COLD ATOMS OPTICAL LATTICES Laser standing waves: dipole-trapping Lattice theory: Bose/Fermi-Hubbard model

24 COLD ATOMS OPTICAL LATTICES Laser standing waves: dipole-trapping Lattice theory: Bose/Fermi-Hubbard model

25 COLD ATOMS QUANTUM SIMULATION Bosons/Fermions: Spins: CONDENSED MATTER PHYSICS

26 HIGH ENERGY PHYSICS? COLD ATOMS QUANTUM SIMULATION

27 QUANTUM SIMULATIONS OF HEP MODELS

28 QUANTUM SIMULATION HEP MODELS INGREDIENTS Matter + Gauge Fields Relativistic theory Gauge invariant Hamitonian formulation: Gauss law

29 QUANTUM SIMULATION HEP MODELS INGREDIENTS Problem: choose V(r), u, v, etc such that (in some limit), we have corresponding to

30 Matter + Gauge Fields We need bosonic and fermionic atoms We need interactions among themselves QUANTUM SIMULATION HEP MODELS INGREDIENTS

31 Relativistic Use a superlattice: it possesses the right limit in the continuum QUANTUM SIMULATION HEP MODELS INGREDIENTS (staggered fermions)

32 QUANTUM SIMULATION HEP MODELS INGREDIENTS LatticeFermion-gauge field coupling Gauge field dynamics Matter + Gauge Fields Relativistic theory Hamitonian formulation: Gauge invariance: abelian, non-abelian Gauss law Bosonic and Fermionic atoms Low energy sector Lattices Angular momentum Interactions / Initial conditions + perturbation theory

33 HEP LATTICE MODELS HAMILTONIAN FORMULATION Matter (Fermions): can move Gauge fields (Bosons): Static Hamiltonian:

34 HEP LATTICE MODELS HAMILTONIAN FORMULATION Gauge invariance: Gauge group: U(1), Z N,SU(N), etc Hamiltonian: Matter (Fermions): can move Gauge fields (Bosons): Static

35 HEP LATTICE MODELS HAMILTONIAN FORMULATION Gauge invariance: Gauge group: U(1), Z N,SU(N), etc Gauss law: Hamiltonian: Matter (Fermions): can move Gauge fields (Bosons): Static

36 Example: compact-QED in 1D Hamiltonians: HEP LATTICE MODELS HAMILTONIAN FORMULATION SCHWINGER MODEL Gauge invariance: Gauss law: (ie, compact)

37 QUANTUM SIMULATION SCHWINGER MODEL 1+1 Fermions: internal states 2M Staggered Fermions: Even sites: hole = particle Odd sites: fermion = antiparticle

38 Bosons: Schwinger rep: internal states QUANTUM SIMULATION SCHWINGER MODEL 1+1 If is small (eg 2 atoms), we obtain a truncated version One can also use a single atom with few internal levels ( is the gauge group)

39 Bosons: Schwinger rep: internal states QUANTUM SIMULATION SCHWINGER MODEL 1+1

40 Interactions: conserves angular momentum locally internal states 2M QUANTUM SIMULATION SCHWINGER MODEL 1+1 Gauge invariance

41 Physical processes: TABLE non-interacting vacuum pe pe pe pe QUANTUM SIMULATION SCHWINGER MODEL 1+1

42 TABLE non-interacting vacuum pe switch on interactions interacting vacuum Excitations: vector + scalar Time-dependent phenomena Confinement First experiments: few bosonic atoms QUANTUM SIMULATION SCHWINGER MODEL 1+1 Preparation:

43 QUANTUM SIMULATION HIGHER DIMENSIONS, NON-ABELIAN Plaquette interactions: Non-abelian gauge theories: Link LR {a 1,a 2 }{b 1,b 2 } bosonic modes

44 COLD ATOMS EXPERIMENTAL CONSIDERATIONS Cold bosons in optical lattices Mott insulator – superfluid transition Exchange interaction (2nd order perturbation theory) Dynamics Anderson-Higgs mechanism in 2D Cold fermions in optical lattices Mott insulator in 2D Cold fermions and bosons in optical lattices Mean-field dynamics Challanges: temperature, decoherence, control … Tuning of interactions: Magnetic/optical Feschbach resonances Lattice geometry Time of flight measurements Single-site addressing: initializaton Single-site measurement Techniques

45 QUANTUM SIMULATION HIGH ENERGY MODELS WARNING

46 NEW METHODS: TENSOR NETWORKS

47 NUMERICAL METHODS SCHWINGER MODEL 1+1 Method: Tensor networks Results

48 NUMERICAL METHODS SCHWINGER MODEL 1+1 Truncation + adiabatic evolution Broken gauge invariance:

49 ROAD MAP 1D QED 2D QED (matter & fields) 2D QED (fields only) 1D (2D) QCD STANDARD MODEL ??? See also: Gauge fields: Lewenstein et al Banerjee,…, Wiese, Zoller, PRL110, 125303 (2013) Banerjee,…, Wiese, Zoller, PRL109, 175302 (2013) Kapit,Mueller, PRA83, 033625 (2011) QUANTUM SIMULATION HIGH ENERGY MODELS IC, Maraner, Pachos, PRL 105, 19403 (2010) Zohar, IC, Reznik, PRL 107, 275301 (2011) Zohar, IC, Reznik, PRL 109, 125302 (2012) Zohar, IC, Reznik, PRL 110, 125304 (2013) Zohar, IC, Reznik, PRA 88, 023617 (2013) Banuls, Cichy, IC, Jansen, JHEP 11,158 (2013) Kühn, IC, Banuls, PRA 90, 042305 (2014)


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