2015
DOI: 10.1088/0963-0252/24/4/044009
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Electron heating via self-excited plasma series resonance in geometrically symmetric multi-frequency capacitive plasmas

Abstract: The self-excitation of Plasma Series Resonance (PSR) oscillations plays an important role in the electron heating dynamics in Capacitively Coupled Radio Frequency (CCRF) plasmas. In a combined approach of PIC/MCC simulations and a theoretical model based on an equivalent circuit, we investigate the self-excitation of PSR oscillations and their effect on the electron heating in geometrically symmetric CCRF plasmas driven by multiple consecutive harmonics. The discharge symmetry is controlled via the Electrical … Show more

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Cited by 42 publications
(33 citation statements)
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References 112 publications
(228 reference statements)
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“…At the higher pressure of 50 mTorr the EEPF still curves outward for the highest quenching coefficients (as there is DA-heating present) but it transitions to curve inward (bi-Maxwellian) for the lowest quenching coefficients. The bi-Maxwellian shape of the EEPF in CCPs is commonly associated with predominant sheath 10 heating (α-mode). The low energy electron population represents electrons confined in the bulk plasma by an ambipolar potential, which are only weakly heated by the rf field, while the high energy population participates in the sheath heating.…”
Section: Resultsmentioning
confidence: 99%
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“…At the higher pressure of 50 mTorr the EEPF still curves outward for the highest quenching coefficients (as there is DA-heating present) but it transitions to curve inward (bi-Maxwellian) for the lowest quenching coefficients. The bi-Maxwellian shape of the EEPF in CCPs is commonly associated with predominant sheath 10 heating (α-mode). The low energy electron population represents electrons confined in the bulk plasma by an ambipolar potential, which are only weakly heated by the rf field, while the high energy population participates in the sheath heating.…”
Section: Resultsmentioning
confidence: 99%
“…This electron heating process is referred to as * tumi@hi.is electron bounce resonance heating (BRH) and can occur for certain combinations of driving frequency and electrode gap [3][4][5][6][7]. The sheath motion and thus the stochastic heating can also be enhanced by self-excited non-linear plasma series resonance (PSR) oscillations [8][9][10][11]. Collisionless electron heating via sheath oscillations is commonly referred to as the α-mode [12].…”
Section: Introductionmentioning
confidence: 99%
“…This effect is referred to as electron bounce resonance heating (BRH) [3]. The sheath motion and thus the stochastic heating can also be enhanced by selfexcited non-linear plasma series resonance (PSR) oscil- * tumi@hi.is lations [4][5][6][7][8]. At higher pressures some of the power is deposited by ohmic heating in the bulk plasma due to collisional momentum transfer between the oscillating electrons and the neutrals.…”
Section: Introductionmentioning
confidence: 99%
“…The evolution in T e is interesting because it was well known that T e will either remain constant or slightly decrease with n e in the single-step or multi-step ionization global model. 1, 16 One possible explanation for this trend in T e may be the dramatic evolution of the EEPF through the electron heating effect 11,21,[30][31][32][33][34][35][36][37] or electronelectron collisions. 17,26,38,39 However, our experiment was conducted in plasmas having nearly Maxwellian EEPFs.…”
mentioning
confidence: 99%