Generalized type IIB supergravity equations and non-Abelian classical r-matrices
Domenico Orlando, Susanne Reffert, Jun-ichi Sakamoto, Kentaroh Yoshida

TL;DR
This paper investigates Yang-Baxter deformations of the $AdS_5 imes S^5$ superstring using non-Abelian classical r-matrices, deriving backgrounds that satisfy generalized supergravity equations and exploring conditions under which they reduce to standard type IIB supergravity solutions.
Contribution
It provides explicit examples of non-Abelian r-matrix deformations and analyzes their associated supergravity backgrounds, including T-dualized solutions that satisfy standard supergravity equations.
Findings
All backgrounds satisfy generalized supergravity equations.
Some T-dualized backgrounds satisfy standard type IIB supergravity.
Certain deformations are locally equivalent to undeformed $AdS_5 imes S^5$ after coordinate transformations.
Abstract
We study Yang-Baxter deformations of the superstring with non-Abelian classical -matrices which satisfy the homogeneous classical Yang-Baxter equation (CYBE). By performing a supercoset construction, we can get deformed backgrounds. While this is a new area of research, the current understanding is that Abelian classical -matrices give rise to solutions of type IIB supergravity, while non-Abelian classical -matrices lead to solutions of the generalized supergravity equations. We examine here some examples of non-Abelian classical r-matrices and derive the associated backgrounds explicitly. All of the resulting backgrounds satisfy the generalized equations. For some of them, we derive "T-dualized" backgrounds by adding a linear coordinate dependence to the dilaton and show that these satisfy the usual type IIB supergravity equations.…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
