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Laser-driven annular shock waves as laboratory analogues of wCDM cosmologies and cosmological gravitational waves
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  • Published: 04 March 2026

Laser-driven annular shock waves as laboratory analogues of wCDM cosmologies and cosmological gravitational waves

  • Felipe A. Asenjo  ORCID: orcid.org/0000-0002-7085-658X1,
  • Felipe Veloso  ORCID: orcid.org/0000-0002-6703-54492 &
  • Julio C. Valenzuela  ORCID: orcid.org/0000-0001-8499-45992 

Communications Physics , Article number:  (2026) Cite this article

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We are providing an unedited version of this manuscript to give early access to its findings. Before final publication, the manuscript will undergo further editing. Please note there may be errors present which affect the content, and all legal disclaimers apply.

Subjects

  • Cosmology
  • Laser-produced plasmas

Abstract

Cosmology faces major observational challenges arising from the spatial and temporal scales involved. Analogue experiments that recreate cosmological scenarios in the laboratory offer a valuable means to probe and better understand the current tensions in cosmological models. Here we demonstrate that the experimental evolution of an annular, laser-driven plasma shock wave, expanding over time and undergoing self-interaction gives rise to multiple shock structures that evolve analogously to a multicomponent cosmological universe. Different propagation trajectories along the shock surface correspond to various forms of wCDM cosmologies, enabling the study of scenarios ranging from simple radiation- or matter-dominated universes to those including dark energy. We further show that the dynamics of the Mach stems approximately follows a Hubble-like law. Additionally, perturbations in the shock fronts serve as experimental analogues of cosmological gravitational perturbations in a matter-dominated universe. This work opens experimental pathway using plasmas for classically simulating complex cosmological models, gravitational waves and the evolution of dark energy at macroscopic scales in laboratory.

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Data availability

The data that support the findings of this study are available from the corresponding authors upon request.

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Acknowledgements

F.A.A. thanks to FONDECYT grant No. 1230094. F.V. thanks to FONDECYT grant No. 1231286 that supported this work. J.C.V. thanks to FONDECYT grant No. 1220533 that supported this work.

Author information

Authors and Affiliations

  1. Facultad de Ingeniería y Ciencias, Universidad Adolfo Ibáñez, Santiago, Chile

    Felipe A. Asenjo

  2. Instituto de Física, Pontificia Universidad Católica de Chile, Santiago, Chile

    Felipe Veloso & Julio C. Valenzuela

Authors
  1. Felipe A. Asenjo
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  2. Felipe Veloso
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  3. Julio C. Valenzuela
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Contributions

F.A.A. contributed with theoretical calculations and analysis of experimental data. F.V. contributed with the development of the experiment setup and analysis of experimental data. J.C.V. contributed with the development of the experiment setup and analysis of experimental data.

Corresponding authors

Correspondence to Felipe A. Asenjo, Felipe Veloso or Julio C. Valenzuela.

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The authors declare no competing interests.

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Asenjo, F.A., Veloso, F. & Valenzuela, J.C. Laser-driven annular shock waves as laboratory analogues of wCDM cosmologies and cosmological gravitational waves. Commun Phys (2026). https://doi.org/10.1038/s42005-026-02570-2

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  • Received: 08 September 2025

  • Accepted: 19 February 2026

  • Published: 04 March 2026

  • DOI: https://doi.org/10.1038/s42005-026-02570-2

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