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This article investigates the propagation of squeezed graviton states from astrophysical sources, concluding that local detectors cannot observe their quantum signatures due to kinematic conflicts that suppress coherence. The study demonstrates a fundamental limitation where macroscopic squeezing does not guarantee observable effects at far-field locations, causing these states to appear classically thermal to single observers.
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Astrophysical Graviton Squeezing Can Be Hidden in the Far-Field

arXiv2 min read

arXiv:2608.17015v1 Announce Type: cross Abstract: While localized astrophysical sources can generate macroscopic graviton squeezing, their observable quantum signatures at far-field detectors remain unresolved. In this work, we investigate the propagation dynamics of the squeezed states using spatial quantum optics methods to evaluate correlation functions accessible to a local observer. Crucially, we reveal a severe kinematic conflict in same-cone measurements, which highly suppresses local quantum coherence. Consequently, these macroscopically squeezed states appear classically thermal to a single detector. Our results demonstrate that global squeezing does not guarantee local observability, and the measurable quantum signatures may be significantly weaker than what would be expected from the overall squeezing parameter of the state.

Abstract:While localized astrophysical sources can generate macroscopic graviton squeezing, their observable quantum signatures at far-field detectors remain unresolved. In this work, we investigate the propagation dynamics of the squeezed states using spatial quantum optics methods to evaluate correlation functions accessible to a local observer. Crucially, we reveal a severe kinematic conflict in same-cone measurements, which highly suppresses local quantum coherence. Consequently, these macroscopically squeezed states appear classically thermal to a single detector. Our results demonstrate that global squeezing does not guarantee local observability, and the measurable quantum signatures may be significantly weaker than what would be expected from the overall squeezing parameter of the state.

arXiv:2608.17015 [gr-qc]

(or arXiv:2608.17015v1 [gr-qc] for this version)

https://doi.org/10.48550/arXiv.2608.17015 Focus to learn more arXiv-issued DOI via DataCite (pending registration)

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Full text under the publisher's open licence · 196 words

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