Abstract
In the current research, we use the hydrodynamic model of electron-ion plasmas with a very general Fermi–Dirac equation of state for electrons in order to investigate the modulational behaviour of ion acoustic (IA) excitation in environments relevant to a wide range of parameters from laboratory to astrophysical phenomena. The reductive perturbation method is used to reduce the model equations into the nonlinear Schrödinger equation from which the dispersion of modulated IA excitations is evaluated and the stability criterion for nonlinear envelope excitations is obtained in terms of normalized electron temperature and chemical potential, applicable to a wide range of parametric space from solid state and inertial-confined fusion plasmas up to the compact stellar objects like white dwarf stars. It is shown that both kinds of bright and dark envelop solitons can exist in warm dense matter, and their stability depends strongly on electron fluid parameters.
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Data Availability Statement
This manuscript has no associated data or the data will not be deposited. [Authors’ comment: The data that support the findings of this study are available from the corresponding author upon reasonable request.]
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MAM conceived of the presented idea. MM developed the theoretical formalism, performed the analytic calculations and performed the numerical simulations. MAM and MM verified the analytical methods. MAM encouraged MM to investigate a specific aspect and supervised the findings of this work. All authors discussed the results and contributed to the final manuscript.
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Mohammadnejad, M., Akbari-Moghanjughi, M. Formation of ion acoustic rogue waves in warm dense matter. Eur. Phys. J. D 75, 307 (2021). https://doi.org/10.1140/epjd/s10053-021-00313-2
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DOI: https://doi.org/10.1140/epjd/s10053-021-00313-2