One-loop corrections to AdS5× S5superstring partition function via Pohlmeyer reduction

DOI10.1088/1751-8113/43/34/345403zbMath1195.81104arXiv1005.4386OpenAlexW3104424892MaRDI QIDQ5747572

Yukinori Iwashita

Publication date: 13 September 2010

Published in: Journal of Physics A: Mathematical and Theoretical (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1005.4386

Mathematics Subject Classification ID

Supersymmetric field theories in quantum mechanics (81T60) Quantum field theory on curved space or space-time backgrounds (81T20) String and superstring theories; other extended objects (e.g., branes) in quantum field theory (81T30) Semiclassical techniques, including WKB and Maslov methods applied to problems in quantum theory (81Q20) Kaluza-Klein and other higher-dimensional theories (83E15)

Related Items (14)

Quantum corrections to short folded superstring in \(\mathrm{AdS}_3\times S^3\times M^4\). ⋮ On the perturbative S-matrix of generalized sine-Gordon models ⋮ Review of AdS/CFT integrability, chapter II.1: Classical \(AdS _{5} \times S ^{5}\) string solutions ⋮ Review of AdS/CFT integrability, chapter II.2: Quantum strings in AdS\(_{5} \times\)S\(^{5}\) ⋮ On string theory on \(AdS_3 \times S^3 \times T^4\) with mixed 3-form flux: tree-level S-matrix ⋮ The AdS\({}_{5}\) {\(\times\)} S\({}^{5}\) semi-symmetric space sine-Gordon theory ⋮ The semi-classical spectrum of solitons and giant magnons ⋮ Towards the quantum S-matrix of the Pohlmeyer reduced version of \(AdS_5 \times S^5\) superstring theory ⋮ Worldsheet supersymmetry of Pohlmeyer-reduced \(\mathrm{AdS}_{n} {\times} S^{n}\) superstrings ⋮ General Leznov-Savelev solutions for Pohlmeyer reduced AdS\({}_{5}\) minimal surfaces ⋮ Integrability vs supersymmetry: Poisson structures of the Pohlmeyer reduction ⋮ Classical and quantum solitons in the symmetric space sine-Gordon theories ⋮ The structure of non-abelian kinks ⋮ \(q\)-deformation of the \(\operatorname{AdS}_{5} \times \operatorname{S}^{5}\) superstring S-matrix and its relativistic limit

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