Abstract

Supersymmetric models with spontaneous supersymmetry breaking suffer from the notorious sign problem in stochastic approaches. By contrast, the tensor network approaches do not have such a problem since they are based on deterministic procedures. In this work, we present a tensor network formulation of the two-dimensional lattice mathcal{N} = 1 Wess-Zumino model while showing that numerical results agree with the exact solutions for the free case.

Highlights

  • Introduction of auxiliary fieldsThe boson action SB in eq (2.12) is transformed into a nearest-neighbor form using two real auxiliary fields G and H: ZB = DφDGDHe−SB, (3.16) SB SB,naiveG2n + Hn2 − rW ′ + αGn + βHn φn+ˆ1 + φn−ˆ1 − 2φn n∈Γ− rW ′ + αGn − βHn φn+ˆ2 + φn−ˆ2 − 2φn (3.17)√ with SB,√naive given in eq (2.13), α = (1 − 2r2)/2, and√β = 1/ 2

  • We present a tensor network formulation of the two-dimensional lattice N = 1 Wess-Zumino model while showing that numerical results agree with the exact solutions for the free case

  • In general, two auxiliary fields are necessary for the next-nearest-neighbor interactions in two directions, it is somewhat √surprising to find that G is decoupled from the other fields for particular values r = ±1/ 2, and the required auxiliary field turns out to be only H

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Summary

Continuum theory

Two-dimensional N = 1 Wess-Zumino model is a supersymmetric theory that consists of a real scalar field φ (x) and a Majorana fermion field ψ (x). In the Euclidean space-time, the corresponding action is given by. Showing the indices in the spinor space explicitly, γμ and ψ (x) are written as (γμ)αβ and ψα (x) for α, β = 1, 2. The spinor index α and the space-time coordinate x are often suppressed without notice. W (φ) is an arbitrary real function of φ, which is referred to as the superpotential in the superfield formalism, and gives the Yukawa- and φn-type interactions with common coupling constants. For any W (φ), the action in eq (2.1) is invariant under the supersymmetry transformation δφ (x) = ǫψ (x) , δψ (x) = γμ∂μφ (x) − W ′ (φ (x)) ǫ,. Where ǫ is a global Grassmann parameter with two components and ǫsatisfies eq (2.3)

Lattice theory
Tensor network representation of partition function
Introduction of auxiliary fields
Symmetric property of local Boltzmann weight
Discretization of non-compact field
Construction of tensor
Miscellaneous remarks
Total tensor network
Numerical test in free theory
Some details
Free Majorana-Wilson fermion
Free Wilson boson
Summary and outlook
A Coarse-graining step in Grassmann TRG

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