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Cosmological quantum states of de Sitter-Schwarzschild are static patch partition functions

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arxiv 2304.06865 v1 pith:X6WTUTZE submitted 2023-04-13 hep-th gr-qc

classification hep-thgr-qc
keywords partitioncosmologicaldualquantumtheoryalgebrablackds-schwarzschild
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abstract

We solve the Wheeler-DeWitt equation in the 'cosmological interior' (the past causal diamond of future infinity) of four dimensional dS-Schwarzschild spacetimes. Within minisuperspace there is a basis of solutions labelled by a constant $c$, conjugate to the mass of the black hole. We propose that these solutions are in correspondence with partition functions of a dual quantum mechanical theory where $c$ plays the role of time. The quantum mechanical theory lives on worldtubes in the 'static patch' of dS-Schwarzschild, and the partition function is obtained by evolving the corresponding Wheeler-DeWitt wavefunction through the cosmological horizon, where a metric component $g_{tt}$ changes sign. We establish that the dual theory admits a symmetry algebra given by a central extension of the Poincar\'e algebra $\mathfrak{e}(1,1)$ and that the entropy of the dS black hole is encoded as an averaging of the dual partition function over the background $g_{tt}$.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. The spectrum of pure dS$_3$ gravity in the static patch

    hep-th 2025-05 conditional novelty 6.0 of 10

    The static-patch partition function of three-dimensional de Sitter gravity is identified with the future-boundary wavefunction, giving a dense discrete spectrum with negative degeneracies.

  2. Gravitational Observatories in AdS$_4$

    hep-th 2024-12 conditional novelty 6.0 of 10

    With conformal boundary conditions in AdS4, linearized gravity has a new boundary Weyl mode; for a spherical boundary the mode has complex frequencies (exponential growth) at large angular momentum, while for a planar...

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