Entanglement Bounds on Cardy Growth in Higher Dimensions

We propose bounds relating thermal entropy to entanglement in unitary conformal field theories: $f\le4π^2a$ in four dimensions and $f\le2.99830949\ldots\,F$ in three dimensions. Here $f$ is the dimensionless coefficient of the cosmological constant term in the thermal effective action, $a$ is the Euler anomaly coefficient, and $F$ is the sphere free energy. Spherical Rényi entropy relates the four-dimensional bound to the conformal collider bounds. We formulate a stronger conjectural inequality involving the stress-tensor three-point function, saturated by every free theory, and establish it in controlled regimes of weakly coupled gauge theories, large-$N$ vector models, and holographic CFTs. Finite-$N$ numerical results provide additional tests. The bounds constrain the Cardy growth of the density of states at high energy.

Authors

Publication Details

Journal
arXiv (Cornell University)
Published
2026-10-27
DOI
https://doi.org/10.48550/arxiv.2610.37449
Primary Topic
Black Holes and Theoretical Physics
Type
preprint
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preprint

Entanglement Bounds on Cardy Growth in Higher Dimensions

Yuya Kusuki, Yin Tang
arXiv (Cornell University)
Black Holes and Theoretical Physics
preprint

Entanglement Bounds on Cardy Growth in Higher Dimensions

Yuya Kusuki, Yin Tang
preprint en

Abstract

We propose bounds relating thermal entropy to entanglement in unitary conformal field theories: $f\le4π^2a$ in four dimensions and $f\le2.99830949\ldots\,F$ in three dimensions. Here $f$ is the dimensionless coefficient of the cosmological constant term in the thermal effective action, $a$ is the Euler anomaly coefficient, and $F$ is the sphere free energy. Spherical Rényi entropy relates the four-dimensional bound to the conformal collider bounds. We formulate a stronger conjectural inequality involving the stress-tensor three-point function, saturated by every free theory, and establish it in controlled regimes of weakly coupled gauge theories, large-$N$ vector models, and holographic CFTs. Finite-$N$ numerical results provide additional tests. The bounds constrain the Cardy growth of the density of states at high energy.

arXiv (Cornell University)
Black Holes and Theoretical Physics
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