
TL;DR
The paper explores how string theory's perturbative partition function inherently sums over semi-classical geometries, including wormholes, by analyzing tensionless strings on specific backgrounds and their dual symmetric orbifold theories.
Contribution
It demonstrates that string perturbation theory encodes a sum over geometries and clarifies the role of stringy corrections and boundary factorization in this process.
Findings
Partition function includes a sum over semi-classical geometries.
String perturbation theory computes the grand canonical partition function.
Wormhole geometries factorize into boundary factors.
Abstract
We examine the question how string theory achieves a sum over bulk geometries with fixed asymptotic boundary conditions. We discuss this problem with the help of the tensionless string on (with one unit of NS-NS flux) that was recently understood to be dual to the symmetric orbifold . We strengthen the analysis of arXiv:2008.07533 and show that the perturbative string partition function around a fixed bulk background already includes a sum over semi-classical geometries and large stringy corrections can be interpreted as various semi-classical geometries. We argue in particular that the string partition function on a Euclidean wormhole geometry factorizes completely into factors associated to the two boundaries of spacetime. Central to this is the remarkable property of the moduli space integral of…
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