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Reply to: Experiments implementing small commuting models lack gravitational features

The Original Article was published on 23 July 2025

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Fig. 1: Thermalization and operator growth.
Fig. 2: Size winding of individual fermions.
Fig. 3: Behaviour of a perturbed Hamiltonian.

References

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Acknowledgements

This work is supported by the Department of Energy, Office of High Energy Physics through QuantISED programme grant SC0019219 on Quantum Communication Channels for Fundamental Physics. This manuscript has been authored by the Fermi Research Alliance, under contract no. DE-AC02-07CH11359 with the US Department of Energy, Office of Science, Office of High Energy Physics. S.I.D. is partially supported by the Brinson Foundation.

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Contributions

J.D.L. worked on the theoretical calculations, computational aspects and simulations. D.J. worked on all theoretical aspects and the validation of the wormhole dynamics. Graduate student D.K.K. worked on theoretical aspects and calculations of the chord diagrams. Graduate student S.I.D. worked on the computations and simulation. Graduate student A.Z. worked on all theory and computational aspects, the learning methods and the validation results. H.N. reviewed all the validation results. M.S. is the lead principal investigator of the QCCFP Consortium Project and worked on all aspects of the research and the manuscript together with all authors. N. Lauk has taken a position at Photonic and did not work on this Reply.

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Correspondence to Maria Spiropulu.

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Jafferis, D., Zlokapa, A., Lykken, J.D. et al. Reply to: Experiments implementing small commuting models lack gravitational features. Nature 643, E20–E23 (2025). https://doi.org/10.1038/s41586-025-08995-z

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