PIRSA:17050066

Video URL

https://pirsa.org/17050066

Towards a general AdS/Ricci-flat correspondence

Skenderis, K. (2017). Towards a general AdS/Ricci-flat correspondence. Perimeter Institute for Theoretical Physics. https://pirsa.org/17050066

Skenderis, Kostas. Towards a general AdS/Ricci-flat correspondence. Perimeter Institute for Theoretical Physics, May. 08, 2017, https://pirsa.org/17050066 

          @misc{ scivideos_PIRSA:17050066,
            doi = {10.48660/17050066},
            url = {https://pirsa.org/17050066},
            author = {Skenderis, Kostas},
            keywords = {Quantum Fields and Strings},
            language = {en},
            title = {Towards a general AdS/Ricci-flat correspondence},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2017},
            month = {may},
            note = {PIRSA:17050066 see, \url{https://scivideos.org/index.php/pirsa/17050066}}
          }

Kostas Skenderis University of Southampton

Talk numberPIRSA:17050066
DOI10.48660/17050066
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

The AdS/Ricci-flat (AdS/RF) correspondence is a map between families of asymptotically locally AdS solutions on a torus and families of asymptotically flat spacetimes on a sphere. In this talk I will discuss how to relax these restrictions for linearized perturbations around solutions connected via the original AdS/RF correspondence.
To this end we perform a Kaluza-Klein (KK)  reduction, keeping all (massive) KK modes,  of AdS on torus and of Minkowski on a sphere.  We show that in the limit of large dimension of the compact manifolds (torus and sphere), the AdS/RF correspondence maps individual KK modes from one side to the other.
When the dimension is finite, the correspondence maps single modes to infinite superpositions of modes. One may further take appropriate limits so that there is either no torus (AdS side) or no sphere (Minkowski side) to map perturbations of solutions that possess no symmetry, thus completely relaxing the original restrictions.
This correspondence should allow us to develop a detailed holographic dictionary for asymptotically flat spacetimes.