English

Omega-deformed SYM on a Gibbons-Hawking Space

High Energy Physics - Theory 2014-11-11 v1 Mathematical Physics math.MP

Abstract

We study an N=2\mathcal{N}=2, pure U(1)U(1) SYM theory on a Gibbons-Hawking space Ω\Omega-deformed using the U(1)U(1) isometry. The resultant 3D theory, after an appropriate "Nekrasov-Witten" change of variables, is asymptotically equivalent to the undeformed theory at spatial infinity but differs from it as one approaches the NUT centers which are fixed points under the U(1)U(1) action. The 3D theory may be recast in the form of a generalized hyperk\"ahler sigma model introduced in \cite{Dey:2014lja} where the target space is a one-parameter family of hyperk\"ahler spaces. The hyperk\"ahler fibers have a preferred complex structure which for the deformed theory depends on the parameter of Ω\Omega-deformation. The metric on the hyperk\"ahler fiber can be reduced to a standard metric on C×T2\mathbb{C} \times T^2 with the modular parameter of the torus depending explicitly on the Ω\Omega-deformation parameter. The contribution of the NUT center to the sigma model path integral, expected to be a holomorphic section of a holomorphic line bundle over the target space on grounds of supersymmetry, turns out to be a Jacobi theta function in terms of certain "deformed" variables.

Keywords

Cite

@article{arxiv.1411.2326,
  title  = {Omega-deformed SYM on a Gibbons-Hawking Space},
  author = {Anindya Dey},
  journal= {arXiv preprint arXiv:1411.2326},
  year   = {2014}
}

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42 pages