Abstract

The Schwarzschild singularity is known to be classically unstable. We demonstrate a simple holographic consequence of this fact, focusing on a perturbation that is uniform in boundary space and time. Deformation of the thermal state of the dual CFT by a relevant operator triggers a nonzero temperature holographic renormalization group flow in the bulk. This flow continues smoothly through the horizon and, at late interior time, deforms the Schwarzschild singularity into a more general Kasner universe. We show that the deformed near-singularity, trans-horizon Kasner exponents determine specific non-analytic corrections to the thermal correlation functions of heavy operators in the dual CFT, in the analytically continued ‘near-singularity’ regime.

Highlights

  • AdS black holes, and will couple gravity to a scalar field

  • We show that the deformed near-singularity, trans-horizon Kasner exponents determine specific non-analytic corrections to the thermal correlation functions of heavy operators in the dual CFT, in the analytically continued ‘near-singularity’ regime

  • We show that the Kasner exponent pt determines specific non-analytic corrections to the correlation function in the regime described by the bouncing geodesic

Read more

Summary

Thermal holographic flows from AdS to Kasner

We can construct explicit examples of holographic flows from the AdS boundary to a Kasner singularity inside a black hole horizon. Integration from the boundary, through the horizon and to the singularity will determine the near-singularity behavior in terms of the ratio φo/T An example of such a solution is shown in figure 2. For every choice of the dimensionless CFT parameter φo/T , we obtain an emergent Kasner scaling determined by the exponent pt This relationship is shown in figure 3. A deformation of the exterior that preserves the spacetime symmetries of the thermal CFT state changes the near-singularity scaling exponents. This can be thought of as a dynamical instability of the Schwarzschild singularity at late interior time r. We describe how to extract these exponents using boundary probes

Probes of the Kasner exponent
E φ2o 4
Non-analyticities in finite mass corrections
Geodesics at all energies
Entanglement entropy probe
Discussion
A Extension across the Einstein-Rosen bridge
Full Text
Published version (Free)

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