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Prediction of a roton-type feature in warm dense hydrogen

Paul Hamann, Linda Kordts, Alexey Filinov, Michael Bonitz, Tobias Dornheim, and Jan Vorberger
Phys. Rev. Research 5, 033039 – Published 21 July 2023

Abstract

In a recent Letter [T. Dornheim et al., Phys. Rev. Lett. 121, 255001 (2018)], it was predicted on the basis of ab initio quantum Monte Carlo simulations that, in a uniform electron gas, the peak ω0 of the dynamic structure factor S(q,ω) exhibits an unusual nonmonotonic wave number dependence, where dω0/dq<0, at intermediate q, under strong coupling conditions. This effect was subsequently explained by the pair alignment of electrons [T. Dornheim et al., Commun. Phys. 5, 304 (2022)]. Here we predict that this nonmonotonic dispersion resembling the roton-type behavior known from superfluids should be observable in a dense, partially ionized hydrogen plasma. Based on a combination of path integral Monte Carlo simulations and linear response results for the density response function, we present the approximate range of densities, temperatures and wave numbers and make predictions for possible experimental observations.

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  • Received 21 April 2023
  • Accepted 9 June 2023

DOI:https://doi.org/10.1103/PhysRevResearch.5.033039

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Plasma Physics

Authors & Affiliations

Paul Hamann1, Linda Kordts1, Alexey Filinov1, Michael Bonitz1, Tobias Dornheim2,3, and Jan Vorberger3,*

  • 1Institut für Theoretische Physik und Astrophysik, Christian-Albrechts-Universität zu Kiel, D-24098 Kiel, Germany
  • 2Center for Advanced Systems Understanding (CASUS), D-02826 Görlitz, Germany
  • 3Helmholtz-Zentrum Dresden-Rossendorf (HZDR), D-01328 Dresden, Germany

  • *j.vorberger@hzdr.de

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Vol. 5, Iss. 3 — July - September 2023

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