Abstract:The dispersion relation for symmetrical TM electromagnetic surface waves propagating in a plasma waveguide with a strongly magnetized plasma column and a dielectric rod is investigated. The growth rate for excitation of these waves is obtained and its dependence on the radius of the annular beam, current intensity and accelerating voltage are investigated.
“…Probably this second case took place in numerically solving the dispersion relation in Jazi & Mehdian (2004). It is a pity that the mistakes in deriving the expressions for the components of the extraordinarily polarized ASW fields in Shokri & Jazi (2003), Jazi & Mehdian (2004), Jazi & Shokri (2005), Jazi et al. (2006), Daryanoosh & Mehdian (2007) require these authors to revise the results obtained therein.…”
Section: Discussionmentioning
confidence: 99%
“…The second part was devoted to studying the dispersion properties of extraordinarily polarized ASWs with the components E r , E ϕ , B z -this part is wrong because of mistakes in the algebra when deriving the expressions for E r and E ϕ from the set of Maxwell equations. The same mistakes are present in the papers by Shokri & Jazi (2003), Jazi & Shokri (2005), Jazi, Shokri & Arbab (2006) and Daryanoosh & Mehdian (2007) and make these papers meaningless. The paper by Shokri & Jazi (2003) presented the limiting case of the paper by Jazi & Mehdian (2004), the space r < R 4 was occupied there by a vacuum.…”
Section: Introductionmentioning
confidence: 89%
“…The expressions (2.4) were derived for the first time by Wait (1966). The wrong expressions for E r and E ϕ in Shokri & Jazi (2003), Jazi & Mehdian (2004), Jazi & Shokri (2005), Jazi et al (2006), Daryanoosh & Mehdian (2007) invalidate the conclusions therein.…”
Section: Derivation Of the Dispersion Relation And Its Analytical Studymentioning
Azimuthal surface waves are eigenmodes of cylindrical plasma–dielectric–metal structures both in the presence of and without an axial static magnetic field. They are actively studied due to possible applications in plasma electronics, nanotechnologies and biomedical diagnostics. Higher radial modes are known to propagate at higher frequencies and shorter wavelengths compared to those of the zeroth mode, a feature which is of interest for practical applications. To gain the advantage of the excitation of higher radial modes of azimuthal surface waves one has first to know their dispersion properties. This paper generalizes the results of earlier papers by including a static axial magnetic field and considering the higher radial modes. The presence of the constant axial magnetic field removes the degeneracy in the wave spectrum with respect to the sign of the azimuthal wavenumber.
“…Probably this second case took place in numerically solving the dispersion relation in Jazi & Mehdian (2004). It is a pity that the mistakes in deriving the expressions for the components of the extraordinarily polarized ASW fields in Shokri & Jazi (2003), Jazi & Mehdian (2004), Jazi & Shokri (2005), Jazi et al. (2006), Daryanoosh & Mehdian (2007) require these authors to revise the results obtained therein.…”
Section: Discussionmentioning
confidence: 99%
“…The second part was devoted to studying the dispersion properties of extraordinarily polarized ASWs with the components E r , E ϕ , B z -this part is wrong because of mistakes in the algebra when deriving the expressions for E r and E ϕ from the set of Maxwell equations. The same mistakes are present in the papers by Shokri & Jazi (2003), Jazi & Shokri (2005), Jazi, Shokri & Arbab (2006) and Daryanoosh & Mehdian (2007) and make these papers meaningless. The paper by Shokri & Jazi (2003) presented the limiting case of the paper by Jazi & Mehdian (2004), the space r < R 4 was occupied there by a vacuum.…”
Section: Introductionmentioning
confidence: 89%
“…The expressions (2.4) were derived for the first time by Wait (1966). The wrong expressions for E r and E ϕ in Shokri & Jazi (2003), Jazi & Mehdian (2004), Jazi & Shokri (2005), Jazi et al (2006), Daryanoosh & Mehdian (2007) invalidate the conclusions therein.…”
Section: Derivation Of the Dispersion Relation And Its Analytical Studymentioning
Azimuthal surface waves are eigenmodes of cylindrical plasma–dielectric–metal structures both in the presence of and without an axial static magnetic field. They are actively studied due to possible applications in plasma electronics, nanotechnologies and biomedical diagnostics. Higher radial modes are known to propagate at higher frequencies and shorter wavelengths compared to those of the zeroth mode, a feature which is of interest for practical applications. To gain the advantage of the excitation of higher radial modes of azimuthal surface waves one has first to know their dispersion properties. This paper generalizes the results of earlier papers by including a static axial magnetic field and considering the higher radial modes. The presence of the constant axial magnetic field removes the degeneracy in the wave spectrum with respect to the sign of the azimuthal wavenumber.
“…The development of sources of radiation in the microwave portion of the electromagnetic spectrum, which extends from approximately 300 MHz to 300 GHz, began many years ago. However, an impressive increase in the power and operating frequency of these sources has taken place in the last few decades, due to progress in a new branch of physics that can be called relativistic high-frequency electronics [8][9][10][11]. The term relativistic refers first to the use of high-voltage electron beams with velocities close to the speed of light, which can have very high current densities, and second to the appearance of new microwave sources based on specific relativistic effects [9][10][11].…”
The dispersion relation of azimuthal electromagnetic surface waves in a rod dielectric magnetized plasma waveguide is obtained. It is investigated that these waves in E-type can be excited by a thin annular relativistic rotating electron beam (TARREB). The effects of the rotating velocity of beam, radius TARREB, on the frequency spectra and growth-rate coefficient are presented.
“…6 Due to their special properties, the surface waves have already been the subject of many theoretical, experimental, and numerical researches. [7][8][9][10][11][12][13][14][15] These waves can be excited on a sufficiently dense plasma and essentially depend on the plasma properties. The surface waves propagation characteristics in dense plasmas are also affected by quantum effects.…”
The propagation of surface waves on a semi-bounded quantum plasma is investigated taking into account the collisional effects. The quantum hydrodynamic model includes Bohm's quantum force, Fermi-Dirac statistical, and collisional corrections are used to derive the dispersion relation of these waves. It is shown that the collisions play a significant role on the decay of surface wave amplitude. Furthermore, the surface waves can be unstable in the presence of collisional effects. It is also indicated that the growth rate of the surface wave instability increases with the increase of collisional and quantum effects, especially in the high wavenumber region. V C 2012 American Institute of Physics. [http://dx.
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