The non-orientable spacetime of the eternal black hole
arXiv:2508.15005 · doi:10.1016/j.physletb.2025.139767
Abstract
We derive the metric of the BTZ black hole for the special case of interchanging the characteristics of space and time coordinates. We maximally extend the geometry of this interior solution and show that the line element is similar to its exterior solution counterpart. Thus, we assign the thermofield double state dual to this interior geometric construction. As a result, we have two independent thermofield double states corresponding to the BTZ metric: one dual to the exterior solution and one dual to the interior solution. In this scenario, considering both thermofield double states as dual to the full BTZ black hole, we evaluate the partition function of the bulk. The partition function represents a non-orientable spacetime. Additionally, we derive a thermofield double-like state that connects in the gravity dual the regions of spacetime with opposite orientations of space and time.
arXiv comment16 pages, 5 figures
References in corpus (15)
- Eternal Black Holes in AdS
- Cool horizons for entangled black holes
- Open Strings
- Jerusalem Lectures on Black Holes and Quantum Information
- Detection of Symmetry Protected Topological Phases in 1D
- Towards a Formulation of Quantum Theory as a Causally Neutral Theory of Bayesian Inference
- Many-body topological invariants for fermionic short-range entangled topological phases protected by antiunitary symmetries
- Interior of a Schwarzschild black hole revisited
- Many-body topological invariants in fermionic symmetry protected topological phases: Cases of point group symmetries
- Topological Phases Protected By Reflection Symmetry and Cross-cap States
- Geometry of quantum correlations in space-time
- Universal entropy of conformal critical theories on a Klein bottle
- Different instances of time as different quantum modes: quantum states across space-time for continuous variables
- Inside the BTZ black hole
- On The Black Hole Interior Spacetime