Abstract:Planar microwave discharges using a multi-slotted planar antenna are investigated. The enhancement of the microwave fields near the plasma resonance is observed in accordance with the theory of the resonant absorption. By operating the antenna with the azimuthally rotating fields, highly uniform overdense plasmas can be produced without being affected by eigenmode structures of surface waves. As a result, the radial distribution of the ion saturation current can be controlled by tailoring the power radiation p… Show more
“…[8][9][10][11][12] show that manipulating the position of the plasma generation in the bulk radially is most important for plasma profile controllability. Axial magnetic fields of varying magnitude combined with slots placed at larger radii make this effect possible.…”
Section: Resultsmentioning
confidence: 99%
“…Above a critical density ($3 Â 10 17 m À3 ), surface wave modes are produced with the plasma density generally peaking at the location of peak electric field. A series of papers by Sugai et al [4][5][6] describe the properties of the generation region while a series of papers by Yasaka et al 7,8 illustrate the impact of the antenna structure on the form of the coupled microwave field and consequent plasma. The radial line slot antenna plasma source is characterized as having low electron temperature and high plasma density near the wafer, which translates to low damage and high process (e.g., etch) rates.…”
The radial line slot antenna plasma source is used in semiconductor device fabrication. As is the case for all plasma sources, ever more strict uniformity control requirements are driven by the precision demands of new device technologies. Large volume diffusion plasmas, of which the radial line slot antenna source is one type, must overcome transport effects or diffusion modes that tend to “center peak” the plasma density near the wafer being processed. One way to resolve problematic transport effects is the insertion of magnetic fields into the plasma region. In this paper, the impact of the magnetic field on plasma properties is parameterized as a function of slot configuration. The magnetic field orientation and the magnitude of magnetic field are varied in a computational study in which the source is modeled as a two-dimensional axisymmetric quasineutral plasma. This work employs a finite element model simulation. The magnitude of magnetic fields considered is 50 Gauss maximum with a microwave power of 3000 W at a pressure of 20 mTorr. 20 mTorr is chosen as this is a condition where diffusion effects are challenging to counteract. The study showed that there are specific conditions for slot configuration and magnetic field that improve the plasma controllability and some that do not. Plasma property modulation is most effective when the plasma source region is placed at large radius with axial magnetic fields. There are synergistic effects between the slot location and magnetic field that are important and placing large magnetic fields at the chamber edge alone does not result in improved uniformity. Electron cyclotron resonance (ECR) heating and the impact of pulsing the magnetic fields are presented. ECR heating is not important for the conditions relevant to this paper and pulsing is shown to have benefit.
“…[8][9][10][11][12] show that manipulating the position of the plasma generation in the bulk radially is most important for plasma profile controllability. Axial magnetic fields of varying magnitude combined with slots placed at larger radii make this effect possible.…”
Section: Resultsmentioning
confidence: 99%
“…Above a critical density ($3 Â 10 17 m À3 ), surface wave modes are produced with the plasma density generally peaking at the location of peak electric field. A series of papers by Sugai et al [4][5][6] describe the properties of the generation region while a series of papers by Yasaka et al 7,8 illustrate the impact of the antenna structure on the form of the coupled microwave field and consequent plasma. The radial line slot antenna plasma source is characterized as having low electron temperature and high plasma density near the wafer, which translates to low damage and high process (e.g., etch) rates.…”
The radial line slot antenna plasma source is used in semiconductor device fabrication. As is the case for all plasma sources, ever more strict uniformity control requirements are driven by the precision demands of new device technologies. Large volume diffusion plasmas, of which the radial line slot antenna source is one type, must overcome transport effects or diffusion modes that tend to “center peak” the plasma density near the wafer being processed. One way to resolve problematic transport effects is the insertion of magnetic fields into the plasma region. In this paper, the impact of the magnetic field on plasma properties is parameterized as a function of slot configuration. The magnetic field orientation and the magnitude of magnetic field are varied in a computational study in which the source is modeled as a two-dimensional axisymmetric quasineutral plasma. This work employs a finite element model simulation. The magnitude of magnetic fields considered is 50 Gauss maximum with a microwave power of 3000 W at a pressure of 20 mTorr. 20 mTorr is chosen as this is a condition where diffusion effects are challenging to counteract. The study showed that there are specific conditions for slot configuration and magnetic field that improve the plasma controllability and some that do not. Plasma property modulation is most effective when the plasma source region is placed at large radius with axial magnetic fields. There are synergistic effects between the slot location and magnetic field that are important and placing large magnetic fields at the chamber edge alone does not result in improved uniformity. Electron cyclotron resonance (ECR) heating and the impact of pulsing the magnetic fields are presented. ECR heating is not important for the conditions relevant to this paper and pulsing is shown to have benefit.
“…Therefore, SWP have been exhaustively investigated both theoretically and experimentally [1][2][3][4][5][6]. For example, M. Nagatsu et al [2] have yielded large-area surface-wave plasmas with an internally mounted planar cylindrical launcher, Y. Yasaka et al [7][8][9] have produced large-diameter uniformity plasma using multislotted planar antenna, and C. Tian et al [10] have studied characteristics of large-diameter plasma using a radial-line slot antenna. But most of the structure of chamber reported in the literature is circular cylinder; a rectangular cavity [11][12][13] is adopted in this article.…”
The theory of surface-wave discharge is introduced. A novel structure of the slot antenna array is designed in this paper, and its excitation is numerical analyzed using dipole-antenna array model and FDTD method, respectively. A microwave discharge experiment is operated with this slot-antenna array, and a numerical simulation is also done with FDTD code using the parameter of plasma from experimental measurement. It is found that the designed slot antenna array can excite effectively the microwave coupling into the cavity, and produce the stable large-area high-density plasma.
“…Due to their peculiar phase rotation, these beams have recently received a great interest at radiofrequencies and microwaves. Indeed, OAM can be potentially capable, among other applications, of an increased capacity of communication channels [3], enhanced remote sensing [4], and plasma control [5], [6].…”
International audienceIn this communication, it is shown that a nondiffracting vortex beam (i.e., a higher order Bessel beam with azimuthal phase variation) can be generated in the near field by synthesizing an inward cylindrical traveling-wave distribution over a finite aperture antenna. A radial line slot array (RLSA) is then designed to prove the concept. The collimated vortex beam is excited in the proximity of the RLSA, within a region properly defined by the nondiffracting range of the generated beam. The radial dependence of the longitudinal electric field of the vortex-beam magnitude follows a first-order Bessel function, and its phase presents a linear azimuthal variation. Full-wave results validate the generation of the nondiffractive higher order Bessel beam within the radiative near field of the launcher
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