| Authors | Seyed mohammadd Khorashadizadeh |
| Journal | Physics of Plasmas |
| Page number | 521071-5210710 |
| Serial number | 5 |
| Volume number | 31 |
| IF | 2.142 |
| Paper Type | Full Paper |
| Published At | 2024 |
| Journal Grade | ISI |
| Journal Type | Typographic |
| Journal Country | Iran, Islamic Republic Of |
| Journal Index | ISI،JCR،Scopus |
| Keywords | relativistic beam, ultra, relativistic hot plasmas, astrophysical plasma, longitudinal wave instabillity, the growth rate of instability |
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Abstract
The investigation of waves and instabilities in ultra-relativistic charged particle beam-plasma systems is
considerable for a wide class of astrophysical environments. Hence in this study, using relativistic kinetic
plasma theory and Lorentz transformations, we study the interaction of a relativistic electron beam with
an ultra-relativistic hot plasma. First, we obtain the dispersion relation of fast and slow longitudinal waves
and consequently the growth rate of the slow wave (negative-energy wave) instability. Then, we plot the
instability growth rate in terms of different physical parameters such as the Lorentz factor, the electron beam
density, the thermal velocity of electrons, and the temperature of the beam particles, and discuss them further.
Our results in the ultra-relativistic regime show that the growth rate of instability decreases by increasing
the Lorentz factor and thermal velocity of particles, while the beam density enhances the growth rate of
instability. Moreover, a comparison with the results obtained from previous studies shows that the growth
rate of instability in the cold electron beam-cold plasma interaction is higher than the instability growth rate
in the case of the relativistic electron beam and ultra-relativistic hot plasma.