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2010
DOI: 10.1215/00277630-2009-003
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Periodicities of T-systems and Y-systems

Abstract: Abstract. The unrestricted T-system is a family of relations in the Grothendieck ring of the category of the finite-dimensional modules of Yangian or quantum affine algebra associated with a complex simple Lie algebra. The unrestricted T-system admits a reduction called the restricted T-system. In this paper we formulate the periodicity conjecture for the restricted T-systems, which is the counterpart of the known and partially proved periodicity conjecture for the restricted Y-systems. Then, we partially prov… Show more

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Cited by 37 publications
(21 citation statements)
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“…Equation (4.4) was studied in [CGT,(3.32)] by using the parameterization of y i (u) by the T-system. However, it is known that this does not give a "general" solution of the Y-system (see [IIKNS,remark after Proposition 3.8]). Therefore, we use F -polynomials instead of the T-system.…”
Section: ])mentioning
confidence: 99%
“…Equation (4.4) was studied in [CGT,(3.32)] by using the parameterization of y i (u) by the T-system. However, it is known that this does not give a "general" solution of the Y-system (see [IIKNS,remark after Proposition 3.8]). Therefore, we use F -polynomials instead of the T-system.…”
Section: ])mentioning
confidence: 99%
“…Subsequently the Tsystem has been formulated and proved [19,28] as identities of q-characters. It has been shown further [21] that the T -system is actually the defining relations of the Grothendieck ring, which is a polynomial ring [17], of finite-dimensional modules of quantum affine algebras. Notice that, from the construction by trace, the q-characters and the transfer matrices are both ring homomorphisms defined on the Grothendieck ring.…”
Section: Introductionmentioning
confidence: 99%
“…In this proceeding paper, we discuss the contribution of gamma-ray loud radio galaxies (not blazars) to EGRB based on [5]. Furthermore, we also discuss the EGRB contribution from various AGN populations such as radio-quiet AGNs and blazars based on our previous studies [19,3]. Throughout this paper, we adopt the standard cosmological parameters of (h, Ω M , Ω Λ ) = (0.7, 0.3, 0.7).…”
Section: Introductionmentioning
confidence: 99%