The partition is 

Z = ∫D[g]exp(-i[S_∂M + S_M])

where the sum is over not just metric configurations of the manifold M, but 
its boundary as well. This tends to suggest the boundary conditions are 
themselves dynamics. A pocket world in an internal inflating spacetime 
would have this feature. I though conjecture this may be a transient state 
of affairs. The boundary action may transition into an action over a field 
theory. This has some holographic content, and it would replace these 
boundary dynamics with a quantum field. Further, the pocket world becomes a 
complete manifold without boundary.

LC

On Monday, October 7, 2019 at 1:20:05 AM UTC-5, Philip Thrift wrote:
>
>
> https://arxiv.org/abs/1808.10448
>
>
> Action Principle for Isotropic General Relativity
> Thomas C. Bachlechner 
> <https://arxiv.org/search/hep-th?searchtype=author&query=Bachlechner%2C+T+C>
> (Submitted on 30 Aug 2018)
>
> We study the generally covariant theory governing an isotropic spacetime 
> region with uniform energy density. Gibbons, Hawking and York showed that 
> fixing the induced boundary metric yields a well-posed variational problem. 
> However, as we demonstrate, fixing the boundary metric violates general 
> covariance and allows the mass of a back hole to vary. This observation has 
> dramatic consequences for path integrals: A sum over spacetimes with fixed 
> boundary metrics is a sum over classically distinct black holes. Instead, 
> we merely demand that coordinates exist such that the metric at the 
> boundary is the Schwarzschild-(A)dS metric of fixed mass M and two-sphere 
> radius R. We derive the action that yields a well-posed variational problem 
> for these physical boundary conditions. The action vanishes for all 
> stationary and isotropic spacetimes. A vanishing action implies that both a 
> Schwarzschild black hole and pure de Sitter space each have one unique 
> semiclassical state. Our results provide a novel and radically conservative 
> approach to several long-standing issues in quantum gravity, such as the 
> wavefunction of the universe, the black hole information paradox, vacuum 
> decay rates and the measure problem of eternal inflation.
>
>
>
> @philipthrift
>

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