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Some Thoughts on the Quantum Theory of de Sitter Space

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

This is a summary of two lectures I gave at the Davis Conference on Cosmic Inflation. I explain why the quantum theory of de Sitter (dS) space should have a finite number of states and explore gross aspects of the hypothetical quantum theory, which can be gleaned from semiclassical considerations. The constraints of a self-consistent measurement theory in such a finite system imply that certain mathematical features of the theory are unmeasurable, and that the theory is consequently mathematically ambiguous. There will be a universality class of mathematical theories all of whose members give the same results for local measurements, within the {\it a priori} constraints on the precision of those measurements, but make different predictions for unmeasurable quantities, such as the behavior of the system on its Poincare recurrence time scale. A toy model of dS quantum mechanics is presented.

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hep-th 2

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2026 2

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representative citing papers

dS$^4$ Metamorphosis

hep-th · 2026-02-23 · conditional · novelty 7.0

Higher spin gravity path integral on S^4 glues to an Sp(N) or superconformal S^3 boundary theory, giving leading contribution 2^N with one-loop cancellations.

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Showing 2 of 2 citing papers.

  • Horizon Edge Partition Functions in $\Lambda>0$ Quantum Gravity hep-th · 2026-03-21 · unverdicted · none · ref 14 · internal anchor

    Horizon edge mode spectra in de Sitter and Nariai spacetimes exhibit universal shift symmetries that produce novel symmetry breaking in one-loop partition functions.

  • dS$^4$ Metamorphosis hep-th · 2026-02-23 · conditional · none · ref 84 · internal anchor

    Higher spin gravity path integral on S^4 glues to an Sp(N) or superconformal S^3 boundary theory, giving leading contribution 2^N with one-loop cancellations.