Abstract

In this work, we extend the 2d topological gravity model of [1] to have as its bulk action any open/closed TQFT obeying Atiyah’s axioms. The holographic duals of these topological gravity models are ensembles of 1d topological theories with random dimension. Specifically, we find that the TQFT Hilbert space splits into sectors, between which correlators of boundary observables factorize, and that the corresponding sectors of the boundary theory have dimensions independently chosen from different Poisson distributions. As a special case, we study in detail the gravity model built from the bulk action of 2d Dijkgraaf-Witten theory, with or without end-of-the-world branes, and for arbitrary finite group G. The dual of this Dijkgraaf-Witten gravity model can be interpreted as a 1d topological theory whose Hilbert space is a random representation of G and whose aforementioned sectors are labeled by the irreducible representations of G.These holographic interpretations of our gravity models require projecting out negative-norm states from the baby universe Hilbert space, which in [1] was achieved by the (only seemingly) ad hoc solution of adding a nonlocal boundary term to the bulk action. In order to place their solution in the completely local framework of a TQFT with defects, we couple the boundaries of the gravity model to an auxiliary 2d TQFT in a non-gravitational (i.e. fixed topology) region. In this framework, the difficulty of negative-norm states can be remedied in a local way by the introduction of a defect line between the gravitational and non-gravitational regions. The gravity model is then holographically dual to an ensemble of boundary conditions in an open/closed TQFT without gravity.

Highlights

  • The purpose of this subsection is to describe a practical way to compute the partition function of “twisted” 2d Dijkgraaf-Witten

  • In this work, we extend the 2d topological gravity model of [1] to have as its bulk action any open/closed TQFT obeying Atiyah’s axioms

  • We find that the TQFT Hilbert space splits into sectors, between which correlators of boundary observables factorize, and that the corresponding sectors of the boundary theory have dimensions independently chosen from different Poisson distributions

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Summary

Review of a simple gravity model

The model of [1] describes a gravity path integral built from a sum over spacetime topology. The authors of [1] consider the above model with the addition of so-called endof-the-world (EofW) branes These are boundaries on which spacetime ends, but unlike the Z boundaries we have discussed above, they are taken to be dynamical, in that the gravity path integral includes a sum over all configurations of such branes. Given a configuration of fixed boundaries, there are many ways we can partition them into “future” and “past” boundaries, and reinterpret the gravity path integral correlator as an inner product of states in the baby universe Hilbert space. The authors of [1] find a dual description of this sort for the gravity path integral (1.3) From this point of view, the correlator Z is no longer a correlator, but the average value of a partition function Z in a 1d topological theory. Before describing the gravity path integral, we will first briefly review DijkgraafWitten theory and present the results of Dijkgraaf-Witten theory in two-dimensions that will be relevant to our construction

Review of Dijkgraaf-Witten theory
A Dijkgraaf-Witten gravity path integral
Boundary interpretation
Background
The gravity path integral
General 2d TQFTs
End-of-the-world branes for Dijkgraaf-Witten
Boundaries and the ensemble problem
Future directions
A State sum formulation of Dijkgraaf-Witten theory
Review of state sum for DW with defects
Generalization and importance for our methods
Full Text
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