Kerr-Schild perturbations of coset CFTs as scale invariant integrable $\sigma$-models
Georgios Itsios, Konstantinos Sfetsos, Konstantinos Siampos

TL;DR
This paper explores Kerr-Schild perturbations of coset conformal field theories in string theory, constructing scale-invariant integrable sigma models that relate to black hole solutions and supergravity embeddings.
Contribution
It introduces a novel application of Kerr-Schild perturbations to coset CFTs, resulting in new scale-invariant integrable sigma models derived from limiting procedures of lambda-deformed theories.
Findings
Constructed explicit Kerr-Schild perturbations of coset CFTs.
Identified scale but not Weyl invariance in resulting sigma models.
Connected models to two-dimensional scale-invariant black holes and supergravity embeddings.
Abstract
Kerr-Schild perturbations in General Relativity provide a fruitful way of constructing new exact solutions starting from known ones, elucidating also the structure of the spacetimes. We initiate such a study in the context of string theory and supergravity. Specifically, we explicitly construct Kerr-Schild perturbations of coset CFTs based on low dimensionality orthogonal groups. We show that these give rise to scale, but not Weyl, invariant integrable -models. We explicitly demonstrate that these models can also be derived from a particular limiting procedure of -deformed coset CFTs based on non-compact groups. The target space of the simplest -model describes a two-dimensional scale invariant black hole for which we also provide two different embeddings to type-II supergravity.
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