Microscopic origin of the entropy of black holes in general relativity
Vijay Balasubramanian, Albion Lawrence, Javier M. Magan, Martin Sasieta
TL;DR
The paper tackles the microscopic origin of black hole entropy in general relativity with negative cosmological constant by constructing infinite families of semiclassical microstates with distinct interiors behind fixed exterior black holes. Wormhole saddle points in the gravitational path integral generate universal, nonzero overlaps among these microstates, ensuring the Hilbert space spanned by the families has dimension $e^{S_{BH}}$ rather than diverging with the family size. This framework also clarifies the interior geometry of the microstates and shows that Einstein-Rosen bridge volumes can be expressed as superpositions of shorter wormholes, leading to a saturation of complexity-related volume at $ ext{O}(e^{S_{BH}})$. By connecting to ETH-like ideas and the Page curve, the work provides a broad, gravity-based mechanism for black hole entropy universality that does not rely on string theoretic constructions or End-of-The-World branes, and it suggests nonlinear, state-dependent observables for interior geometry.
Abstract
We construct an infinite family of microstates with geometric interiors for eternal black holes in general relativity with negative cosmological constant in any dimension. Wormholes in the Euclidean path integral for gravity cause these states to have small, but non-zero, quantum mechanical overlaps that have a universal form. The overlaps have a dramatic consequence: the microstates span a Hilbert space of log dimension equal to the Bekenstein-Hawking entropy. The semiclassical microstates we construct contain Einstein-Rosen bridges of arbitrary size behind their horizons. Our results imply that all these bridges can be interpreted as quantum superpositions of wormholes of size at most exponential in the entropy.
