# Energy spectrum of a quantum spacetime with boundary

**Authors:** Shoichiro Miyashita

arXiv: 1906.11838 · 2019-07-30

## TL;DR

This paper calculates the density of states for a quantum spacetime with boundary using minisuperspace path integrals, revealing a new high-energy behavior distinct from previous results and highlighting the role of multiple contributions beyond saddle points.

## Contribution

It introduces a direct calculation of the density of states for a quantum spacetime with boundary, accounting for contributions beyond saddle points, and explores high-energy behavior.

## Key findings

- DOS exhibits exponential Bekenstein-Hawking entropy within a specific energy range.
- At high energies, DOS approaches a positive constant, unlike previous models.
- Multiple contributions to the path integral are significant beyond the saddle point approximation.

## Abstract

In this paper, I revisit the microcanonical partition function, or density of states (DOS), of general relativity. By using the minisuperspace path integral approximation, I directly calculate the $S^2 \times Disc$ topology sector of the DOS of a (quantum) spacetime with an $S^2\times \mathbb{R}$ Lorentzian boundary from the microcanonical path integral, in contrast with previous works in which DOSs are derived by inverse Laplace transformation from various canonical partition functions. Although I found there always exists only one saddle point for any given boundary data, it does not always dominate the possible integration contours. There is another contribution to the path integral other than the saddle point. One of the obtained DOSs has behavior similar to that of the previous DOSs; that is, it exhibits exponential Bekenstein--Hawking entropy for the limited energy range $ (1-\sqrt{2/3}) <GE/R_{b}< (1+\sqrt{2/3})$, where energy $E$ is defined by the Brown--York quasi-local energy momentum tensor and $R_{b}$ is the radius of the boundary $S^2$. In that range, the DOS is dominated by the saddle point. However, for sufficiently high energy, where the saddle point no longer dominates, the DOS approaches a positive constant, different from the previous ones, which approach zero.

## Full text

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## Figures

11 figures with captions in the complete paper: https://tomesphere.com/paper/1906.11838/full.md

## References

21 references — full list in the complete paper: https://tomesphere.com/paper/1906.11838/full.md

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Source: https://tomesphere.com/paper/1906.11838