On genus expansion of superpolynomials

A. Mironov; A. Morozov; A. Sleptsov; A. Smirnov

doi:10.1016/j.nuclphysb.2014.11.003

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arXiv · 1310.7622

On genus expansion of superpolynomials

A. Mironov·A. Morozov·A. Sleptsov·A. Smirnov

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Abstract

Recently it was shown that the (Ooguri-Vafa) generating function of HOMFLY polynomials is the Hurwitz partition function, i.e. that the dependence of the HOMFLY polynomials on representation R is naturally captured by symmetric group characters (cut-and-join eigenvalues). The genus expansion and expansion through Vassiliev invariants explicitly demonstrate this phenomenon. In the present letter we claim that the superpolynomials are not functions of such a type: symmetric group characters do not provide an adequate linear basis for their expansions. Deformation to superpolynomials is, however, straightforward in the multiplicative basis: the Casimir operators are β-deformed to Hamiltonians of the Calogero-Moser-Sutherland system. Applying this trick to the genus and Vassiliev expansions, we observe that the deformation is fully straightforward only for the thin knots. Beyond the family of thin knots additional algebraically independent terms appear in the Vassiliev and genus expansions. This can suggest that the superpolynomials do in fact contain more information about knots than the colored HOMFLY and Kauffman polynomials. However, even for the thin knots the beta-deformation is non-innocent: already in the simplest examples it seems inconsistent with the postivity of colored superpolynomials in non-(anti)symmetric representations, which also happens in I.Cherednik's (DAHA-based) approach to the torus knots.

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A. Mironov, A. Morozov, A. Sleptsov, A. Smirnov. 2014-09-05. On genus expansion of superpolynomials. https://doi.org/10.1016/j.nuclphysb.2014.11.003

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