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arXiv:2511.11203

Relative entropy for locally squeezed states

Daniela Cadamuro, Markus B. Fröb, Dimitrios Katsinis, Jan Mandrysch

quant-phhep-thmath-phSubmitted Nov 14, 2025• Announced Nov 17, 2025• 0 citations• Revised Nov 28, 2025 (v2)
v1 · Nov 14, 2025v2 · Nov 28, 2025v3 · Sep 16, 2026
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Abstract

Relative entropy serves as a fundamental measure of state distinguishability in both quantum information theory and relativistic quantum field theory. Despite its conceptual importance, however, explicit computations of relative entropy remain notoriously difficult. Thus far, results in closed form have only been obtained for ground states, coherent states, and, more recently, single-mode squeezed states. In this work, we extend the analysis to multi-mode squeezed states, imposing that the squeezing generators be local either in space or in spacetime, which results in a continuum of squeezed modes. We provide a detailed and self-contained analysis of such states for a free scalar quantum field on Minkowski spacetime, connecting also with older results on the essential self-adjointness of the Wick square, and showing that they lie in the folium of the Minkowski vacuum representation. Although the local squeezing is natural from a foundational standpoint, we uncover a severe incompatibility between locality and squeezing: the relative entropy between a locally squeezed state and the vacuum generally diverges, however small the squeezing is. This shows that while locally squeezed states are well-defined elements of the state space of a free quantum field, they are infinitely different from the vacuum, in contrast to coherent states whose relative entropy with respect to the vacuum is finite.

Comments
34 pages, references added, typos, minor correction (end of Sec.3)

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Relative entropy serves as a fundamental measure of state distinguishability in both quantum information theory and relativistic quantum field theory. Despite its conceptual importance, however, explicit computations of relative entropy remain notoriously difficult. Thus far, results in closed form have only been obtained for ground states, coherent states, and, more recently, single-mode squeezed states. In this work, we extend the analysis to multi-mode squeezed states, imposing that the squeezing generators be local either in space or in spacetime, which results in a continuum of squeezed modes. We provide a detailed and self-contained analysis of such states for a free scalar quantum field on Minkowski spacetime, connecting also with older results on the essential self-adjointness of the Wick square, and showing that they lie in the folium of the Minkowski vacuum representation. Although the local squeezing is natural from a foundational standpoint, we uncover a severe incompatibility between locality and squeezing: the relative entropy between a locally squeezed state and the vacuum generally diverges, however small the squeezing is. This shows that while locally squeezed states are well-defined elements of the state space of a free quantum field, they are infinitely different from the vacuum, in contrast to coherent states whose relative entropy with respect to the vacuum is finite.
Abstract Utilizing the Tomita–Takesaki modular theory, we derive a closed-form analytic expression for the Araki–Uhlmann relative entropy between a single-mode squeezed state and the vacuum state in a free relativistic massive scalar Quantum Field Theory within wedge regions of Minkowski spacetime. Similarly to the case of coherent states, this relative entropy is proportional to the smeared Pauli–Jordan distribution. Consequently, the Araki–Uhlmann entropy between a single-mode squeezed state and the vacuum satisfies all expected properties: it remains positive, increases with the size of the Minkowski region under consideration, and decreases as the mass parameter grows.
We numerically investigate the Araki-Uhlmann relative entropy in Quantum Field Theory, focusing on a free massive scalar field in 1+1-dimensional Minkowski spacetime. Using Tomita-Takesaki modular theory, we analyze the relative entropy between a coherent state and the vacuum state, with several types of test functions localized in the right Rindler wedge. Our results confirm that relative entropy decreases with increasing mass and grows with the size of the spacetime region, aligning with theoretical expectations.
We numerically investigate the Araki-Uhlmann relative entropy in Quantum Field Theory, focusing on a free massive scalar field in 1 + 1 -dimensional Minkowski spacetime. Using Tomita-Takesaki modular theory, we analyze the relative entropy between a coherent state and the vacuum state, with several types of test functions localized in the right Rindler wedge. Our results confirm that relative entropy decreases with increasing mass and grows with the size of the spacetime region, aligning with theoretical expectations.
A spacetime description of squeezed states in quantum fields is presented, revealing the connection between squeezing and nonequilibrium dynamics. Squeezings in configuration space, occupation number space, and phase space are distinguished; generating transformations and criteria for their physical realization are discussed. The results have an immediate applicability to atoms and ions in traps, as well as to quantum optics in relativistic and nonequilibrium systems. Squeezing, sub-Poissonian statistics, and antibunching are all shown to be a direct consequence of spacetime inhomogeneities in the quantum field. The finite speed of communication between separate regions of the field (finite speed of light) places a lower limit on the attainable spectral width of squeezed states. The squeezing parameter for field quadratures has the appearance of a chemical potential in an inhomogeneous field, and through a renormalization may be generated by a Chern-Simons-like term.
Positive Wigner functions can have less Shannon entropy than the vacuum, even arbitrarily close to the vacuum state. We construct physical counterexamples and identify the competition that controls their entropy: the relative entropy to the vacuum phase-space density can exceed twice the mean photon number. A two-level family exhibits a finite window in which coherence lowers entropy while preserving global Wigner positivity. A complementary construction repairs a remote negative tail with an exponentially small thermal admixture; an explicit mixing weight of 2×10−212\times10^{-21}2×10−21 preserves a rigorously established entropy decrease. Optimisation over all one-mode Wigner-nonnegative states gives the sharp low-energy scale Eγ/[ln⁡(1/E)]βE^γ/[\ln(1/E)]^βEγ/[ln(1/E)]β, with γ≃0.7412γ\simeq0.7412γ≃0.7412 and β≃0.5861β\simeq0.5861β≃0.5861. Because γ<1γ<1γ<1, tensor products can have vanishing total energy and trace distance from vacuum while their entropy deficit diverges. We derive the exact half-transmission threshold for universal Shannon-entropy recovery and connect it to companion results showing residual non-Gaussian structure. The counterexamples reveal distinct controls on entropy: coherence sets the local descent, mode number amplifies it, and loss restores the vacuum bound.