Numerical Analysis of Discretized N=(2,2) SYM on Polyhedra Syo - - PowerPoint PPT Presentation

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Numerical Analysis of Discretized N=(2,2) SYM on Polyhedra Syo - - PowerPoint PPT Presentation

Numerical Analysis of Discretized N=(2,2) SYM on Polyhedra Syo Kamata (Keio Univ. ) Collaborators : So Matsuura Keio Univ. Tatsuhiro Misumi Akita Univ., Keio Univ. Kazutoshi Ohta (Meijigaukin Univ.) Anomaly and Sign problem


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Numerical Analysis of Discretized N=(2,2) SYM on Polyhedra

Syo Kamata (Keio Univ. ) Collaborators : So Matsuura(Keio Univ.) Tatsuhiro Misumi (Akita Univ., Keio Univ.) Kazutoshi Ohta (Meijigaukin Univ.) Lattice2016 July 26th 2016 @ Southampton Univ.

“Anomaly and Sign problem in N=(2,2) SYM on Polyhedra : Numerical Analysis”, arXiv:1607.01260

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SUSY theory on Lattice

  • SUSY + Lattice

{Q, Q} ∝ P boson ⇔ fermion

 Non-perturbative analysis of SUSY theory  First principles calculation  Numerical simulation

  • Motivated by

Gauge/Gravity correspondence String theory Condensed matter Mathematical contexts

  • Problems for preserving SUSY on Lattice

SUSY is quantumly broken by lattice spacing. Fine-tuning Locality (SLAC type differential op.) The sign problem

[Dondi et.al., 1977] [Kato et.al., 2013]

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2 dim. N=(2,2) SYM on discretized spacetime

  • N=(2,2) Sugino model on flat spacetime

 Gauge symmetry  (Discrete) Translation and Rotation  Internal symmetry (U(1)v ,U(1)A )  Locality (Ultra local)  No doublers  Exact SUSYs on Lattice

  • Regular lattice

⇒ discretized spacetime with non-trivial topology.

  • Preserving one exact (0-form) SUSY
  • Field contents are defined on sites, links, and faces.
  • U(1)A anomaly ⇒ This effect is Hidden in the Pfaffian Phase.

[Sugino, 2004] [Matsuura et.al., 2014]

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2 dim. N=(2,2) SYM on discretized spacetime

  • Action on flat spacetime ( 4 dim. N=1 ⇒ 2 dim. N=(2,2) )
  • SUSY transform

[Sugino, 2004]

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2 dim. N=(2,2) SYM on discretized spacetime

  • Action on flat spacetime (Q-exact form)
  • SUSY transform up to gauge trf.

[Sugino, 2004]

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2 dim. N=(2,2) SYM on discretized spacetime

  • Action on discretized curved spacetime
  • SUSY transform

Site → Site Link → Link Face → Face

U, λ Φ, Φ, η Y, χ Φ, Φ, η U, λ U, λ [Matsuura et.al., 2014] Φ, Φ, η

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U(1)A anomaly and Pfaffian phase

  • U(1)A symmetry is broken by quantum effect

(fermion zero-modes) on general curved background.

  • Pfaffian has two kinds of phases:

The partition function is ill-defined due to rotation Naïve phase quenched method ⇒ the anomaly is ignored.

Dirac op. (vanishes in the cont. lim.(?)) U(1)A anomaly

How to define observables? How to take into account anomaly?

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Anomaly-Phase-Quenched method

  • Introduce a compensate operator which cancels the U(1)A

phase from the fermion measure.

Examples:

  • Definition of observables : the APQ method.
  • The PCSC relation of the exact SUSY.

Insert A [S.K. et.al., 2016]

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Set-up for numerical simulations

  • Background topology : S (tetra,octa,…), T (3 , 4 , 5 ), F
  • Gauge group : SU(2)
  • ’t Hooft coupling and surface area :
  • Boson mass term (for lifting flat direction) :
  • Pseudo-fermion method and rational approximation.
  • Lattice action without the admissibility condition for

avoiding unphysical degenerate vacua of link variables.

  • Measure the PCSC relation and the Pfaffian phase.

2 2 2 2 2 2 [Matsuura et.al., 2014] Can we separate into and ? The sign problem ? 2

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Set-up for numerical simulations

  • Background topology : S (tetra,octa,…), T (3 , 4 , … ), F
  • Gauge group : SU(2)
  • ’t Hooft coupling and surface area :
  • Boson mass term (for lifting flat direction) :

2 2 2 2 2 2

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PCSC relation

  • Consistent with

the theoretical prediction.

  • APQ method works well.
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Histgram of phase ( )

Massless limit ( Scalar SUSY restored ) ⇒ peaks appear !!

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Eigenvalue distribution of Dirac op.

Pseudo zero-modes (|dim(G) ・Eul|) Fourier modes Others We estimate the Pfaffian phase not including pseudo zero-modes. What happens in the phase histgram ?

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Histgram of phase of

(not including pseudo-zero modes)

Sharp peaks appear for both h=0 and h=2.

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Summary and Conclusion

  • We performed the numerical simulation of the N=(2,2)

SYM on discretized spacetime with non-trivial toplogy.

  • U(1)A symmetry is generally broken by anomaly.
  • We numerically calculated the PSCS relation for

the exact SUSY using the anomaly-phase-quenched method.

  • The results are consistent with the theoretical prediction,

and the APQ method works.

  • The residual phase has peaks

⇒ the sign problem vanishes.

 Continuum limit  More general background  SQCD (fundamental matter contents)