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Direct evidence of non-acoustic collective modes in dynamics of molten Carbon
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  • Published: 01 April 2026

Direct evidence of non-acoustic collective modes in dynamics of molten Carbon

  • Taras Bryk  ORCID: orcid.org/0000-0002-4360-06341,2,
  • Giancarlo Ruocco  ORCID: orcid.org/0000-0002-2762-95333,4,
  • Jean-François Wax5 &
  • …
  • Noël Jakse6 

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

  • Characterization and analytical techniques
  • Chemical physics
  • Computational science
  • Structure of solids and liquids

Abstract

Understanding the structure and dynamics of molten Carbon extends beyond the study of carbon-rich planetary interiors, with perspective applications in nuclear fusion, material science and industrial processes. While the recent X-ray observation of liquid C rekindled the interest in its microscopic structure, it also reminds of the challenges in rationalising the complex dynamics extending beyond the hydrodynamic regime. Primary among them is the theoretical description of non-hydrodynamic processes in one-component liquids. Here, we report collective longitudinal and transverse propagating modes in molten Carbon at T = 5500 K and pressure range 10-40 GPa from ab initio simulations and machine learned molecular dynamics. We observe an unusual two-peak shape of the longitudinal current spectral functions pointing at a branch of non-acoustic propagating modes in the wave number range k > 1 Å−1. By applying a generalized collective modes framework to recover the time dependence of time correlations in the system, we identify the peak at lower energy as a non-hydrodynamic mode, and ascribe it to out-of-phase motion of particles encapsulated in cages of their nearest neighbors.

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Data availability

Numerical data sets are available from the corresponding author upon a request.

Code availability

VASP26,27,28,29 and LAMMPS37 are the standard packages for computer simulations. Computer codes for numerical calculation of time correlation functions and spectral functions are available from the corresponding author upon a request.

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Acknowledgements

T.B. was supported by the National Research Foundation of Ukraine under Project 2023.05/0019. N.J. acknowledges the CINES, TGCC and IDRIS under Project No. INP2227/72914/gen5054, as well as CIMENT/GRICAD for computational resources. This work has been partially supported by MIAI Cluster AI (ANR-19-P3IA-0003). Discussions within the French collaborative network in artificial intelligence in materials science GDR CNRS 2123 (IAMAT) are also acknowledged. The calculations have been performed using the ab initio total-energy and molecular dynamics program VASP (Vienna ab initio simulation program) developed at the Institute für Materialphysik of the Universität Wien26,27,28,29.

Author information

Authors and Affiliations

  1. Yukhnovskii Institute for Condensed Matter Physics, National Academy of Sciences of Ukraine, Lviv, Ukraine

    Taras Bryk

  2. Institute of Applied Mathematics and Fundamental Sciences, Lviv National Polytechnic University, Lviv, Ukraine

    Taras Bryk

  3. Center for Life Nano- & Neuro-Science, Istituto Italiano di Tecnologia, Roma, Italy

    Giancarlo Ruocco

  4. Dipartimento di Fisica, Universita’ di Roma “La Sapienza”, Roma, Italy

    Giancarlo Ruocco

  5. Laboratoire de Chimie et de Physique A2MC, Université de Lorraine - Metz, Metz, France

    Jean-François Wax

  6. Université Grenoble Alpes, CNRS, Grenoble INP, SIMaP, Grenoble, France

    Noël Jakse

Authors
  1. Taras Bryk
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  2. Giancarlo Ruocco
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  3. Jean-François Wax
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  4. Noël Jakse
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Contributions

T.B. and N.J. designed the research. T.B, N.J. and J.-F.W. performed and analyzed the analytical and numerical calculations. T.B., N.J. and G.R. discussed the results and wrote the paper.

Corresponding author

Correspondence to Taras Bryk.

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The authors declare no competing interests.

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Bryk, T., Ruocco, G., Wax, JF. et al. Direct evidence of non-acoustic collective modes in dynamics of molten Carbon. Commun Phys (2026). https://doi.org/10.1038/s42005-026-02602-x

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  • Received: 07 August 2025

  • Accepted: 13 March 2026

  • Published: 01 April 2026

  • DOI: https://doi.org/10.1038/s42005-026-02602-x

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