Black hole to cosmic horizon microstates in string/M theory: timelike boundaries and internal averaging
Eva Silverstein

TL;DR
This paper explores how averaging over internal dimensions and timelike boundaries in string/M theory can reconcile dS holography with black hole microstates, providing new insights into quantum gravity and horizon entropy.
Contribution
It demonstrates the role of internal averaging and timelike boundaries in connecting AdS and dS solutions within string/M theory, advancing the understanding of horizon microstates.
Findings
Microstate count matches Gibbons-Hawking entropy for dS3.
Boundary deformation relates black hole horizon to dS cosmic horizon.
Internal averaging washes out differences in extra dimensions.
Abstract
In this note, we resolve an apparent obstacle to string/M theory realizations of dS observer patch holography, finding a new role for averaging in quantum gravity. The solvable deformation recently provided a detailed microstate count of the cosmic horizon, reproducing the refined Gibbons-Hawking entropy computed by Anninos et al along with the correct radial bulk geometry. On the gravity side, the deformation brings in the boundary to just outside a black hole horizon, where it is indistinguishable from the dS cosmic horizon, enabling a continuous passage to a bounded patch of dS. In string/M theory, the relationship between AdS/CFT and dS involves uplifts that change the internal topology, e.g. replacing an internal sphere with an internal hyperbolic space (and incorporating varying warp and conformal factors). We connect these…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
