A strong diffusive ion mode in dense ionized matter predicted by Langevin dynamics.
A strong diffusive ion mode in dense ionized matter predicted by Langevin dynamics.
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DOI:
10.1038/ncomms14125
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发表时间:
2017-01-30
影响因子:
16.6
通讯作者:
Gregori G
中科院分区:
文献类型:
--
作者:
Mabey P;Richardson S;White TG;Fletcher LB;Glenzer SH;Hartley NJ;Vorberger J;Gericke DO;Gregori G
The state and evolution of planets, brown dwarfs and neutron star crusts is determined by the properties of dense and compressed matter. Due to the inherent difficulties in modelling strongly coupled plasmas, however, current predictions of transport coefficients differ by orders of magnitude. Collective modes are a prominent feature, whose spectra may serve as an important tool to validate theoretical predictions for dense matter. With recent advances in free electron laser technology, X-rays with small enough bandwidth have become available, allowing the investigation of the low-frequency ion modes in dense matter. Here, we present numerical predictions for these ion modes and demonstrate significant changes to their strength and dispersion if dissipative processes are included by Langevin dynamics. Notably, a strong diffusive mode around zero frequency arises, which is not present, or much weaker, in standard simulations. Our results have profound consequences in the interpretation of transport coefficients in dense plasmas. Studying the properties of dense plasmas is challenging due to strong interactions between electrons and ions, and numerical methods overcome this difficulty using a static thermostat. Here the authors predict a strong diffusive ion mode at low energy by including dissipative processes in the model.