4.2 Article

Electromagnetic solitons and their stability in relativistic degenerate dense plasmas with two electron species

Journal

Publisher

FRONTIERS MEDIA SA
DOI: 10.3389/fspas.2022.1007584

Keywords

electromagnetic soliton; electron-acoustic wave; degenerate plasma; two-temperature electrons; nonlinear schrodinger equation; stability of solitons; ponderomotive force

Funding

  1. Science and Engineering Research Board (SERB, Government of India)
  2. [CRG/2018/004475]
  3. [DSC-07033608101PRD]

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The evolution of electromagnetic solitons in relativistic degenerate dense astrophysical plasmas is studied, and the conditions for the existence and stability of moving solitons are analyzed. The results show that the stability regions shift due to relativistic degeneracy, the fraction of classical to degenerate electrons, and the EM wave frequency. The stability of moving solitons depends on the degree of electron degeneracy, the soliton eigenfrequency, and the soliton velocity.
The evolution of electromagnetic (EM) solitons due to nonlinear coupling of circularly polarized intense laser pulses with low-frequency electron-acoustic perturbations is studied in relativistic degenerate dense astrophysical plasmas with two groups of electrons: a sparse population of classical relativistic electrons and a dense population of relativistic degenerate electron gas. Different forms of localized stationary solutions are obtained and their properties are analyzed. Using the Vakhitov-Kolokolov stability criterion, the conditions for the existence and stability of a moving EM soliton are also studied. It is noted that the stable and unstable regions shift around the plane of soliton eigenfrequency and the soliton velocity due to the effects of relativistic degeneracy, the fraction of classical to degenerate electrons and the EM wave frequency. Furthermore, while the standing solitons exhibit stable profiles for a longer time, the moving solitons, however, can be stable or unstable depending on the degree of electron degeneracy, the soliton eigenfrequency and the soliton velocity. The latter with an enhanced value can eventually lead to a soliton collapse. The results should be useful for understanding the formation of solitons in the coupling of highly intense laser pulses with slow response of degenerate dense plasmas in the next generation laser-plasma interaction experiments as well as the novel features of x-ray and gamma-ray pulses that originate from compact astrophysical objects.

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