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This research establishes fundamental theoretical limits on detecting quantum signatures in weakly coupled fields like axion dark matter and gravitational waves. The study proves that realistic detector constraints and coupling suppression make observing nonclassical effects practically impossible with current technology, effectively ruling out proposals to verify gravity's quantization via these methods. While highly squeezed states could theoretically overcome this barrier, the required parameters remain far beyond experimental reach today.
Sources coveringarXiv, Quantum Zeitgeist
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Suppressed Quantum Effects of Weakly Coupled Waves

arXiv2 min read

arXiv:2607.27313v1 Announce Type: cross Abstract: Precision experiments increasingly target weakly coupled waves, including axion dark matter and gravitational radiation. Such waves are commonly described as classical fields, yet they could exist in quantum states with no classical counterpart. We exhibit two severe obstructions to detecting nonclassical effects, both independent of the mode occupancy. First, realistic detectors cannot resolve the fundamental modes of a field; instead they couple to coarse-grained "effective" modes, which often washes out nonclassical effects. Second, all nonclassical effects are suppressed by extra powers of the weak coupling, making them much harder to detect than the waves themselves. We prove this in general, and explicitly show how the suppression arises for quadrature and number statistics, entanglement, and decoherence. The suppression can in principle be overcome given suitable quantum resources, such as highly squeezed detector states, but the required parameters are far beyond current experimental capabilities. We use the axion cavity haloscope as an explicit example, although our conclusions apply to many ultralight dark matter searches, and rule out proposals to establish the quantization of gravity from observations of gravitational waves.

Abstract:Precision experiments increasingly target weakly coupled waves, including axion dark matter and gravitational radiation. Such waves are commonly described as classical fields, yet they could exist in quantum states with no classical counterpart. We exhibit two severe obstructions to detecting nonclassical effects, both independent of the mode occupancy. First, realistic detectors cannot resolve the fundamental modes of a field; instead they couple to coarse-grained "effective" modes, which often washes out nonclassical effects. Second, all nonclassical effects are suppressed by extra powers of the weak coupling, making them much harder to detect than the waves themselves. We prove this in general, and explicitly show how the suppression arises for quadrature and number statistics, entanglement, and decoherence. The suppression can in principle be overcome given suitable quantum resources, such as highly squeezed detector states, but the required parameters are far beyond current experimental capabilities. We use the axion cavity haloscope as an explicit example, although our conclusions apply to many ultralight dark matter searches, and rule out proposals to establish the quantization of gravity from observations of gravitational waves.

arXiv:2607.27313 [hep-ph]

(or arXiv:2607.27313v1 [hep-ph] for this version)

https://doi.org/10.48550/arXiv.2607.27313 arXiv-issued DOI via DataCite (pending registration)

Full text under the publisher's open licence · 192 words

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