Abstract

We find general deformations of BTZ spacetime and identify the corresponding thermofield initial states of the dual CFT. We deform the geometry by introducing bulk fields dual to primary operators and find the back-reacted gravity solutions to the quadratic order of the deformation parameter. The dual thermofield initial states can be deformed by inserting arbitrary linear combination of operators at the mid-point of the Euclidean time evolution that appears in the construction of the thermofield initial states. The deformed geometries are dual to thermofield states without deforming the boundary Hamiltonians in the CFT side. We explicitly demonstrate that the AdS/CFT correspondence is not a linear correspondence in the sense that the linear structure of Hilbert space of the underlying CFT is realized nonlinearly in the gravity side. We also find that their Penrose diagrams are no longer a square but elongated horizontally due to deformation. These geometries describe a relaxation of generic initial perturbation of thermal system while fixing the total energy of the system. The coarse-grained entropy grows and the relaxation time scale is of order β/2π. We clarify that the gravity description involves coarse-graining inevitably missing some information of nonperturbative degrees.

Highlights

  • The dual thermofield initial states can be deformed by inserting arbitrary linear combination of operators at the mid-point of the Euclidean time evolution that appears in the construction of the thermofield initial states

  • We explicitly demonstrate that the AdS/CFT correspondence is not a linear correspondence in the sense that the linear structure of Hilbert space of the underlying CFT is realized nonlinearly in the gravity side

  • In this note we have considered the deformation of BTZ black holes in the context of AdS/CFT correspondence

Read more

Summary

Einstein scalar system

One may turn on linear combination of the above bulk scalar fields or even other bulk fields with non-zero spins. We shall limit our consideration to the case of scalar fields. Where d is the spacetime dimension of the boundary CFT which equals 2 for the present case. For the m2 = 0 case, this theory can be fully consistently embedded into type IIB gravity [7]. For non-zero m2 that corresponds to integral dimensions, the solution can be consistently embedded into IIB supergravity only for the leading order fluctuations including the gravity back reaction. Any resulting solutions involving nontrivial scalar field will be deformations of the well known AdS3 × S3 × M4 background where M4 may be either T 4 or K3 [10]. Our construction is based on this full microscopic AdS/CFT correspondence. The central charge of the boundary conformal field theory is related to the Newton constant by.

Linearized perturbation
Boundary stress tensor and horizon area
Convenient form of coordinates
Field theory construction
Other examples of micro-geometries
Bulk dynamics
Conclusions

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.