Transition between Schwarzschild black hole and string black hole
arXiv:2502.05965 · doi:10.1103/mxdb-2j39
Abstract
In this paper, we aim to study the quantum transition between a Schwarzschild black hole and a string black hole in the large limit. Classically, such a transition between these two distinct black hole geometries is forbidden. The only feasible discussion is centered on how a black hole evaporates, loses mass, and transitions into highly excited fundamental strings. Building upon our previous work on T-duality between the Schwarzschild and string black holes, we reduce the problem to two dimensions, where the corresponding Wheeler-De Witt equation can be derived. Using this equation, we identify the two black hole geometries as distinct wave function states. This allows us to easily compute the transition probability between these two geometries, driven by the string coupling.
v1: 15 pages, 3 figures; v2: 16 pages, 3 figures, comments added
References in corpus (16)
- Pre-Big-Bang in String Cosmology
- The Pre-Big Bang Scenario in String Cosmology
- A Correspondence Principle for Black Holes and Strings
- Duality and Dilaton
- Self Gravitating Fundamental Strings
- White Holes as Remnants: A Surprising Scenario for the End of a Black Hole
- Graceful exit in quantum string cosmology
- Large D gravity and low D strings
- Strings on Curved Spacetimes: Black Holes, Torsion, and Duality
- Birth of the Universe as quantum scattering in string cosmology
- Naked singularities in low energy, effective string theory
- The correspondence between rotating black holes and fundamental strings
- Low-energy quantum string cosmology
- Two and three loop alpha' corrections to T-duality: Kasner and Schwarzschild
- Quantum string cosmology
- Large gravity and low string via corrections