1. Information recovery from pure state geometries in 3D
- Author
-
Joris Raeymaekers, Orestis Vasilakis, and Ondrej Hulik
- Subjects
High Energy Physics - Theory ,Physics ,Nuclear and High Energy Physics ,Black Holes ,Conformal Field Theory ,010308 nuclear & particles physics ,Conformal field theory ,Scalar (physics) ,FOS: Physical sciences ,Semiclassical physics ,Function (mathematics) ,AdS-CFT Correspondence ,01 natural sciences ,Microstate (statistical mechanics) ,AdS/CFT correspondence ,Theoretical physics ,General Relativity and Quantum Cosmology ,High Energy Physics - Theory (hep-th) ,0103 physical sciences ,lcsh:QC770-798 ,lcsh:Nuclear and particle physics. Atomic energy. Radioactivity ,010306 general physics ,Complex plane ,BTZ black hole - Abstract
It is a well-studied phenomenon in AdS$_3$/CFT$_2$ that pure states often appear 'too thermal' in the classical gravity limit, leading to a version of the information puzzle. One example is the case of a heavy scalar primary state, whose associated classical geometry is the BTZ black hole. Another example is provided by a heavy left-moving primary, which displays late time decay in chiral correlators. In this paper we study a special class of pure state geometries which do not display such information loss. They describe heavy CFT states created by a collection of chiral operators at various positions on the complex plane. In the bulk, these take the form of multi-centered solutions from the backreaction of a collection of spinning particles, which we construct for circular distributions of particles. We compute the two-point function of probe operators in these backgrounds and show that information is retrieved. We observe that the states for which our geometric picture is reliable are highly extended star-like objects in the bulk description. This may point to limitations of the semiclassical fuzzball picture of black hole microstates., Comment: 48 pages, 12 figures, published version
- Published
- 2020