Quantum Mechanics of a Spherically Symmetric Causal Diamond in Minkowski Spacetime

We construct the phase space of a spherically symmetric causal diamond in (d+2)-dimensional Minkowski spacetime. Utilizing the covariant phase space formalism, we identify the relevant degrees of freedom that localize to the d-dimensional bifurcate horizon and, upon canonical quantization, determine their commutators. On this phase space, we find two Iyer-Wald charges. The first of these charges, proportional to the area of the causal diamond, is responsible for shifting the null time along the horizon and has been well documented in the literature. The second charge is much less understood, being integrable for d≥2 only if we allow for field-dependent diffeomorphisms and is responsible for changing the size of the causal diamond.

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Publication Details

Journal
Physical Review Letters
Published
2025-03-25
DOI
https://doi.org/10.1103/physrevlett.134.121501
Citations
5
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
9.35

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article

Quantum Mechanics of a Spherically Symmetric Causal Diamond in Minkowski Spacetime

Temple He, Kathryn M. Zurek, Prahar Mitra, Mathew W. Bub et al.
5 citations
Physical Review Letters
Black Holes and Theoretical Physics
9.35
article

Quantum Mechanics of a Spherically Symmetric Causal Diamond in Minkowski Spacetime

Temple He, Kathryn M. Zurek, Prahar Mitra, Mathew W. Bub, Yiwen Zhang
article en
5 citations

Abstract

We construct the phase space of a spherically symmetric causal diamond in (d+2)-dimensional Minkowski spacetime. Utilizing the covariant phase space formalism, we identify the relevant degrees of freedom that localize to the d-dimensional bifurcate horizon and, upon canonical quantization, determine their commutators. On this phase space, we find two Iyer-Wald charges. The first of these charges, proportional to the area of the causal diamond, is responsible for shifting the null time along the horizon and has been well documented in the literature. The second charge is much less understood, being integrable for d≥2 only if we allow for field-dependent diffeomorphisms and is responsible for changing the size of the causal diamond.

Physical Review LettersVol. 134(12)
California Institute of Technology (US), University of Amsterdam (NL)
U.S. Department of Energy, Simons Foundation, Heising-Simons Foundation, Office of Science, Horizon 2020 Framework Programme, Walter Burke Institute for Theoretical Physics, Natural Sciences and Engineering Research Council of Canada, European Research Council, High Energy Physics
Openalex Percentile: Top 3%
Black Holes and Theoretical Physics
9.35
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Quantum Mechanics of a Spherically Symmetric Causal Diamond in Minkowski Spacetime — Temple He, Kathryn M. Zurek, et al. · Physical Review Letters (2025) | TGRS Research Map | TGRS