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QUANTUM SIMULATION OF LATTICE GAUGE THEORIES WITH COLD ATOMS Benni Reznik Tel-Aviv University In collaboration with E. Zohar (Tel-Aviv) and J. Ignacio Cirac, (MPQ ) YITP workshop on quantum information, August 2 th 2014 1 OUTLINE


  1. QUANTUM SIMULATION OF LATTICE GAUGE THEORIES WITH COLD ATOMS Benni Reznik Tel-Aviv University In collaboration with E. Zohar (Tel-Aviv) and J. Ignacio Cirac, (MPQ ) YITP workshop on quantum information, August 2 th 2014 1

  2. OUTLINE • Preliminaries --Quantum Simulations --Ultracold Atoms --Structure of HEP (standard) models --Hamiltonian Formulation of Lattice Gauge Theory • Simulating Lattice gauge theories • Local gauge invariance from microscopic physics • Examples: Abelian (cQED), Non Abelian (YM SU(2)) , . • outlook.

  3. QUANTUM ANALOG SIMULATION

  4. QUANTUM ANALOG SIMULATION

  5. SIMULATED PHYSICS • Condensed matter ( e.g. for testing model for high TC superconductivity)  Hubbard and spin models  External (classical) artificial gauge potential Abelian/non-Abelian.

  6. SIMULATED PHYSICS • Gravity: BH, Hawking/Unruh, cosmological effects .. Discrete version of a black hole Horstman, BR, Fagnocchi, Cirac, PRL (2010)

  7. SIMULATED PHYSICS High Energy physics (HEP)?

  8. SIMULATING SYSTEMS • Bose Eienstein Condensates • Atoms in optical lattices • Rydberg Atoms • Trapped Ions • Superconducting devices • …

  9. COLD ATOMS

  10. COLD ATOMS OPTICAL LATTICES Laser Standing waves: dipole trapping

  11. COLD ATOMS OPTICAL LATTICES Atom 𝜀 In the presence 𝑭 𝑠, 𝑢 the atoms has a time dependent dipole moment 𝑒 𝑢 = 𝛽 𝜕 𝑭 𝑠, 𝑢 of some non resonant excited states. Stark effect: V r ≡ ΔE r = 𝛽 𝜕 〈 𝑭 𝑠 𝑭 𝑠 〉/𝜀

  12. COLD ATOMS OPTICAL LATTICES  Superfluid to Mott insulator, phase transition (I. Bloch) s

  13. “Super lattice!” Resolved (hyperfine levels) potentials Spatial direction

  14. THE STANDARD MODEL: CONTENTS Matter Particles: Fermions Quarks and Leptons: Mass, Spin, Flavor Coupled by force Carriers / Gauge bosons, Massless, chargeless photon (1): Electromagnetic, U(1) Massive, charged Z, W’s ( 3): Weak interactions, SU(2) Massless, charged Gluons (8): Strong interactions, SU(3)

  15. GAUGE FIELDS Abelian Fields Non-Abelian fields Maxwell theory Yang-Mills theory Massless Massless Long-range forces Confinement Chargeless Carry charge Linear dynamics Self interacting & NL

  16. QED: THE CONVENIENCE OF BEING ABELIAN 𝑅𝐹𝐸 𝑠 ∝ 1 𝛽 𝑅𝐹𝐸 ≪ 1 , 𝑊 𝑠 We (ordinarily) don’t need second quantization and quantum field theory to understand the structure of atoms: 𝑛 𝑓 𝑑 2 ≫ 𝐹 𝑆𝑧𝑒𝑐𝑓𝑠𝑕 ≃ 𝛽 𝑅𝐹𝐸 2 𝑛 𝑓 𝑑 2 Also in higher energies (scattering, fine structure corrections), where QFT is required, perturbation theory (Feynman diagrams) works well.

  17. CALCULATE! e.g. , the anomalous electron magnetic moment: (g-2)/2= …. …+ + +… 891 vertex diagrams

  18. …+ 12672 self energy diagrams (g-2)/2= 1 159 652 180 . 73 ( 0 . 28 ) × 10 − 12  g − 2 measurement by the Harvard Group using a Penning trap T. Aoyama et. al. Prog. Theor. Exp. Phys. 2012 , 01A107

  19. THE LOW ENERGY PHYSICS OF HIGH ENERGY PHYSICS, OR THE DARK SIDE OF ASYMPTOTIC FREEDOM 𝛽 𝑅𝐷𝐸 > 1 , 𝑊 𝑅𝐷𝐸 𝑠 ∝ 𝑠 non-perturbative confinement effect! No free quraks: they construct Hadrons: Q Q Mesons (two quarks), V ( r ) Confinement Baryons (three quarks), Static pot. for a pair … of heavy quarks Color Electric flux-tubes: “a non -abelian Meissner effect”. r ASYMPTOTIC FREEDOM Coulomb Q Q

  20. THE LOW ENERGY PHYSICS OF HIGH ENERGY PHYSICS, OR THE DARK SIDE OF ASYMPTOTIC FREEDOM 𝛽 𝑅𝐷𝐸 > 1 , 𝑊 𝑅𝐷𝐸 𝑠 ∝ 𝑠 non-perturbative confinement effect! No free quraks: they construct Hadrons: Q Q Mesons (two quarks), V ( r ) Confinement Baryons (three quarks), Static pot. for a pair … of heavy quarks Color Electric flux-tubes: “a non -abelian Meissner effect”. r Shut up and Calculate! Coulomb Q Q

  21. Compared with CM simulations, several additional requirements when trying to simulate HEP models

  22. REQUIREMENT 1 One needs both bosons and fermions Fermion fields : = Matter Bosonic, Gauge fields:= Interaction mediators Ultracold atoms: One can have bosonic and fermionic species

  23. REQUIREMENT 2 The theory has to be relativistic = have a causal structure. The atomic dynamics (and Hamiltonian) is nonrelativistic. We can use lattice gauge theory. The continuum limit will be then relativistic.

  24. REQUIREMENT 3 The theory has to be local gauge invariant. local gauge invariance = “charge” conservation Atomic Hamiltonian conserves total number – seem to have only global symmetry It turns out that local gauge invariance can be obtained as either : I) – a low energy approximate symmetry. II) – or “fundamentally” from symmetries of atomic interactions.

  25. LATTICE GAUGE THEORY • A very useful nonperturbative approach to gauge theories, especially QCD. • Lattice partition and correlation functions computed using Monte Carlo methods in a discretized Euclidean spacetime (Wilson). • However: Limited applicability with too many quarks / finite chemical potential (quark-gluon plasma, color superconductivity): Grassman integration  the computationally hard “sign problem” • Euclidean correlations – No real time dynamics

  26. LATTICE GAUGE THEORIES HAMILTONIAN FORMULATION

  27. LATTICE GAUGE THEORIES DEGREES OF FREEDOM Gauge field degrees of freedom: U(1), SU(N), etc, unitary matrices LINKS Matter degrees of freedom : Spinors VERTICES

  28. Gauge fields on the links Gauge group elements: U r is an element of the gauge group (in the representation r ), on each link Left and right generators: [J, m, m’ i Gauge transformation: Generators: Dynamical! Left and right “electric” fields

  29. LATTICE GAUGE THEORIES NON-ABELIAN HAMILTONIAN Gauge field dynamics (Kogut-Susskind Hamiltonian): Local gauge invariance: acting on a single vertex Strong coupling limit: g >> 1 Weak coupling limit: g << 1 Matter dynamics:

  30. Local Gauge invariance A symmetry that is satisfied for each link separately

  31. Example compact – QED (cQED)

  32. U(1) gauge theory Start with a hopping fermionic Hamiltonian, in 1 spatial direction † 𝜔 𝑜 † 𝜔 𝑜+1 + 𝐼. 𝑑. 𝐼 = 𝑁 𝑜 𝜔 𝑜 + 𝛽 𝑜 𝜔 𝑜 𝑜 This Hamiltonian is invariant to global gauge transformations, † ⟶ 𝑓 𝑗Λ 𝜔 𝑜 † 𝜔 𝑜 ⟶ 𝑓 −𝑗Λ 𝜔 𝑜 ; 𝜔 𝑜

  33. U(1) gauge theory Promote the gauge transformation to be local: † ⟶ 𝑓 𝑗Λ 𝑜 𝜔 𝑜 † 𝜔 𝑜 ⟶ 𝑓 −𝑗Λ 𝑜 𝜔 𝑜 ; 𝜔 𝑜 Then, in order to make the Hamiltonian gauge invariant, add unitary operators, 𝑉 𝑜 , † 𝜔 𝑜 † 𝑉 𝑜 𝜔 𝑜+1 + 𝐼. 𝑑. 𝐼 = 𝑁 𝑜 𝜔 𝑜 + 𝛽 𝑜 𝜔 𝑜 𝑜 𝑉 𝑜 = 𝑓 𝑗𝜄 𝑜 ; 𝜄 𝑜 ⟶ 𝜄 𝑜 + Λ 𝑜+1 - Λ 𝑜

  34. Dynamics Add dynamics to the gauge field: 𝐼 𝐹 = 𝑕 2 2 2 𝑀 𝑜,𝑨 𝑜 is the angular momentum operator conjugate to 𝑀 𝑜 𝜄 𝑜 , representing the (integer) electric field.

  35. Plaquette In d>1 spatial dimensions, interaction terms along plaquettes − 1 1 2 1 2 𝑕 2 cos 𝜄 𝑛,𝑜 + 𝜄 𝑛+1,𝑜 − 𝜄 𝑛,𝑜+1 − 𝜄 𝑛,𝑜 𝑛,𝑜 In the continuum limit, this corresponds to 𝛼 × 𝑩 2 - gauge invariant magnetic energy term. Figure from ref [6]

  36. cQED -> QED 𝛼 × 𝑩 2 E is quantized! = L z plaquette + + J ¢ A Gauge-Matter interaction

  37. End Example (cQED) Next: we move on to atomic lattices

  38. QUANTUM SIMULATION COLD ATOMS Fermion matter fields Bosonic gauge fields Superlattices: Atom internal levels

  39. QUANTUM SIMULATION LOCAL GAUGE INVARIANCE • Generators of gauge transformations: Sector w. fixed charge … …

  40. QUANTUM SIMULATION LOCAL GAUGE INVARIANCE • Generators of gauge transformations: … …

  41. QUANTUM SIMULATION LOCAL GAUGE INVARIANCE • Generators of gauge transformations: … …

  42. QUANTUM SIMULATION LOCAL GAUGE INVARIANCE • Generators of gauge transformations: local gauge invariance!! … …

  43. Local Gauge Invariance at low enough energies Gauss’s law is added as a constraint. Leaving the gauge invariant sector of Hilbert space costs too much Energy. Low energy effective gauge invariant Hamiltonian. .. Not Gauge invariant Δ ≫ 𝜀𝐹 Gauge invariant sector … 𝜀𝐹 E. Zohar, BR, Phys. Rev. Lett. 107, 275301 (2011)

  44. LGI is exact : emerging from some microscopic symmetries Links  atomic scattering : gauge invariance is a fundamental symmetry • Plaquettes  gauge invariant links  virtual loops of ancillary fermions. •

  45. GLOBAL GAUGE INVRAIANT = FERMION HOPPING F F

  46. GLOBAL GAUGE INVRAIANT = FERMION HOPPING

  47. GLOBAL GAUGE INVRAIANT = FERMION HOPPING

  48. LOCAL GAUGE INVARIANCE: ADD A MEDIATOR !

  49. EXAMPLE – cQED LINK INTERACTIONS F B F

  50. EXAMPLE – cQED LINK INTERACTIONS LOCAL GAUGE INVARIANCE: ADD A MEDIATOR F A,B C D

  51. EXAMPLE – cQED LINK INTERACTIONS 𝑀 → 𝑀 − 1 F A,B C D

  52. EXAMPLE – cQED LINK INTERACTIONS 𝑀 → 𝑀 + 1 F A,B C D

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