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K.B. Efetov, C. Pepin , H. Meier

K.B. Efetov, C. Pepin , H. Meier . 1. 2. 1. 1. 2. RUB Bochum, Germany , CEA Saclay, France. Exact bosonization for interacting fermions in arbitrary dimensions. (New route to numerical and analytical calculations).

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K.B. Efetov, C. Pepin , H. Meier

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  1. K.B. Efetov, C. Pepin , H. Meier 1 2 1 1 2 RUB Bochum, Germany, CEA Saclay, France Exact bosonization for interacting fermions in arbitrary dimensions. (New route to numerical and analytical calculations) Bosonization:mapping of electron models onto a model describing collective excitations (charge, spin excitations, diffusion modes, etc).

  2. Origin of the word: 1D electron systems. The main idea:writing the electronic operators as Bosonization:for Tomonaga-Luttinger model (long range interaction) (Luttinger, Tomonaga (196?)) A simple Hamiltonian H The most general form conjectured by K.E. & A. Larkin (1975) -Density fluctuations operator K-compressibility, N-average density Microscopic theory Haldane (1982) Importance of long wave length excitations! …………………

  3. Formal replacement of electron Green functions by propagators for collective excitations! Very often direct expansions with electronic Green functions are not efficient(infrared divergences, high energy cutoffs respecting symmetries). Equivalent representation Spin excitations Transformation from electrons to collective excitations: Bosonization

  4. Difficulties in Monte Carlo simulations for fermionic systems:negative sign problem exponential growth of the computation time with the size of the system. (From a lecture by M. Troyer) NP-nondeterministic polynomial

  5. Can one bosonize in higher dimensions? Earlier attempts: A. Luther 1979: Special form of Fermi surface (square, cube, etc.). Almost 1D. F.D.M. Haldane 1992: Patching of the Fermi surface, no around corner scattering Further development of the patching idea: A. Houghton & Marston 1993; A.H.Castro Neto & E. Fradkin 1994; P. Kopietz & Schonhammer 1996; Khveshchenko, R. Hlubina, T.M. Rice 1994 et al; C. Castellani, Di Castro, W. Metzner 1994…… Main assumption of all these works: long range interaction.

  6. I.L. Aleiner & K. B. Efetov 2006,Method of quasiclassical Green functions supplemented by integration over supervectors Logarithmic contributions to specific heat and susceptibility are found. Good agreement with known results in 1D. No restriction on the range of interaction but not a full account of effects of the Fermi surface curvature ind>1. In all the approaches only low energy excitations are considered: no chance for using in numerics. Present work: Exact mapping fermion models onto bosonic ones. New possibilities for both analytical and numerical computations.

  7. Starting Hamiltonian H The interaction, tunneling and dimensionality are arbitrary! Small simplification of the formulas

  8. Hubbard-Stratonovich Transformation with a real field

  9. Another representation for Basis of auxiliary field Monte Carlo simulations (Blankenbecler, Scalapino, Sugar (1981)) Procedure: subdividing the interval into time slices and calculation for each slice recursively. However, can in such a procedure be both positive and negative: sign problem! Not convenient for analytical calculations either.

  10. Good news: can exactly be obtained from a bosonic model! Derivation of the model (main steps): -fermionic Green function in the external field. Boundary conditions

  11. Looking for the solution: (in spirits of a Schwinger Ansatz) Bosonic periodic boundary conditions: is the Green function of the ideal Fermi gas Equations forand Solving these equations is not convenient. Solution is not unambiguous.

  12. New function A: -Fourier transform of the Fermi distribution or Then, the “partition function” is What is good in that? How to find A without solving equation for T?

  13. “Free lunch”: a) b) an operator 1. Act withon a) and multiply by from the right. 2. Multiply b) by from the left. 3. Subtract the obtained equations from each other.

  14. Final equation for A Partition function Boundary conditions Purely bosonic problem! Linear (almost separable) real equation for A New possibilities for both numerical and analytical studies!

  15. How can one calculate numerically?(Non-expert’s view) Introduce the Green function g for the linear equation and represent it in the form: where the operator P is Possibility to do recursion in time (as usual)! Compensation of the Bose-denominator no singularities in g. In the absence of singularities, the exponent remains real for any subdivision of the interval into slices is positive:no sign problem!

  16. Perturbation theory:expanding inand subsequent integration over this field. Main order: RPA-like formula (first order in the expansion in collective excitations).

  17. Analytical calculations:BRST (Becchi, Rouet, Stora, Tyutin)-possibility of integration over the auxiliary field before doing approximations How to calculate if is the solution of the equation ? A well known trick: Next step: -Grassmann variables

  18. Description with a supersymmetric action and superfields Introducing new Grassmann variablesand superfields is anticommuting (!) The “partition function” as the functional integral over Gaussian averaging over can immediately be performed!

  19. Final superfield theory (still exact). -partition function of the ideal Fermi gas is the bare action (fully supersymmetric)

  20. The terms and are invariant under the transformation of the fields : (Almost) supersymmetry transformation. -anticommuting variables What to calculate? Logarithmic contributions exist in any dimensions and they can be studied by RG. Reduction of the exact model to a low energy one is convenient. Variety of phenomena for, e.g., cuprates and other strongly correlated systems can be attacked in this way.

  21. Conclusions. The model of interacting fermions can be bosonized in any dimension for any reasonable interaction: free lunch but….. What about a free dinner?Can the bosonization be the key to the ultimate solution of the sign problem? Can one solve non-trivial models (e.g., models for high temperature cuprates or for quantum phase transitions) using the supersymetric model for collective excitations? To be answered

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