22nd International Symposium on Plasma Chemistry July 5-10, 2015; Antwerp, Belgium Laser-induced photodetachment in a magnetically confined low-pressure argon-acetylene plasma destined for nanoparticles formation G. Al Makdessi1, A. Hamdan1, J. Margot1 and R. Clergereaux2 1 Groupe de physique des plasmas, Université de Montréal, C.P. 6128, succ. centre-ville, Montréal, Québec, H3C 3J7, Canada 2 Université de Toulouse-LAPLACE-CNRS, 118 Route de Narbonne, Bât. 3R3, 31062 Toulouse Cedex, France Abstract: We present the investigation of negative ions in magnetically confined Ar-C 2 H 2 plasmas, using the laser photodetachment technique. The negative ion density n - is observed to increase with B and to slightly decrease with the C 2 H 2 percentage. In addition, n - decreases with increasing gas pressure. The photodetachment cross section is deduced from the laser photodetachment signal as a function of laser energy. It is shown to be significantly higher than the cross-section expected from C 2 H - ion only. This is attributed to the negatively charged nanoparticles synthesized and confined in the plasma. Keywords: laser photodetachment, acetylene, negative ions, magnetic field, nanoparticles 2. Experimental setup The experimental setup is schematically shown in Fig. 1. The reactor is composed of a cylindrical stainless steel chamber (20 cm of diameter and 96 cm of length) connected to a 15 cm-diameter quartz tube. The plasma was generated by a surface wave whose power was injected by a Ro-box [5]. The frequency of the surface wave is 200 MHz and the absorbed power was fixed at 350 W. The stainless steel chamber was exposed to a magnetic field created by four coils connected in series and spatially distributed to form a magnetic mirror with a P-II-7-17 magnetic mirror ratio of 1.9. L2 M1 Baratron gauge Coils Coaxial stub Ionization gauge Grid Quartz tube L3 Quartz windows Platinum tip Langmuir probe Alumina M2 Ro-box Faraday cage Valve Turbomolecular pump Mechanical pump 100 Ω Mass flow controller Photodiode L1 VDC Oscilloscope C2H2 XeCl laser 308 nm Ar 1. Introduction Dusty plasmas are plasmas containing charged nanoand micro-sized particles. Beside their dominant presence in the universe, dust particles are also observed in laboratory plasmas especially those used in material processing [1] and nuclear fusion [2, 3]. When reactive gases (silane, acetylene, etc.) are introduced in the plasma, dusty particles can spontaneously form in the reactor chamber independently of the power coupling mode provided the residence time of the precursors is large enough for allowing volume interactions dominate over surface interactions. In RF discharges at pressures below than 150 mTorr, anions are considered to be the species being the most likely to form dust particles [4]. This has been linked to their largest residence time (confinement in the ambipolar electric field) among all species present in the plasma. For this reason, the characterization of negative species remains an important issue for further understanding of dusty plasmas kinetics. In this work, we are interested in the determination of the negative ion density in magnetized dusty plasmas operated at very low pressure. This density is measured using a laser photodetachment technique in plasmas generated in argon-acetylene mixture. The influence of the operating plasma parameters is investigated. Trigger signal Fig. 1. Schematic of the experimental setup. Photodetachment was achieved by using a pulsed XeCl excimer laser at 308 nm. The laser frequency was fixed at 10 Hz and its temporal pulse width is ~10 ns. The laser beam was focused in the plasma using a lens of 5 cm in diameter and 2 m in focal length. A few centimeters ahead of the focal region, the beam was crossed by an electrostatic planar probe formed of a platinum disk (3 mm of diameter). The disk is connected to a tungsten wire (0.5 mm of diameter) and both are surrounded by an alumina tube except the disk surface. The probe was positioned at the chamber center by ensuring that its surface was completely immersed in the laser beam and that it was not ablated. A DC voltage of 55 V was applied to the probe in order to attract all the electrons present in the plasma around the probe. This voltage value was selected based on Langmuir probe measurements ensuring that we operate in the electron saturation region. The value of the current (before and after each laser pulse) was deduced by measuring the potential drop across a calibrated resistor of 100 Ω connected in series with the voltage source (batteries). The electrical signal was 1 visualized and saved using a Tektronix oscilloscope (TDS 2014C, 100 MHz-2GS/s). digital 3. Laser induced photodetachment When the energy of an incident photon is greater than the electron affinity of a negative ion, the photon can detach the electron in excess from this ion. This phenomenon leads to a time-dependent increase of the electron density. Quantitatively, the fraction ρ of negative ions lost through photodetachment in the laser beam volume is given by [6]: 1 − exp(− ρ= EL σ p (e L ) ) SL e L (1) For large enough laser fluence (E L /S L ), ρ tends to 1, which means that all the negative ions present in the plasma-laser interaction volume are photodetached. In such a case, the negative ions density n ‒ can be linked to the electron density n e through the equation: n− ∆ne = ne ne 0 (2) Δn e represents the instantaneous increase of n e due to the photodetached electrons and n e0 is the initial electron density (i.e., without laser perturbation). Considering that the probe electron saturation current is proportional to the electron density, equation 2 can be expressed as follows: ∆I e n− = I e 0 ne 1.52 probe-lens distance 0.12 ∆Ie/Ie0 133 cm 98 cm 0.10 0.08 0.06 6 9 12 15 18 EL/SL (mJ/cm2) 21 24 Fig. 3. ΔI e /I e as function of E L /S L for two probe-lens distances for 55 V, 2 mTorr, 20% C 2 H 2 and 350 W. 1.48 ∆Ie Ie (mA) 0.14 0.04 3 1.56 1.40 1.36 -1 Ie0 0 1 2 3 4 Time (ms) 5 6 7 Fig. 2. Example of photodetachment signal. Pressure = 2 mTorr, power = 350 W, the percentage of C2H2 = 80% and the probe-lens distance = 98 cm. 2 4. Results and discussion In order to optimize the laser parameters (fluence, focal point position, etc.) and make sure that all the negative ions are detached in the interaction region, we have performed first the following study. The fluence of the laser at the probe position was varied by changing the laser energy E L and the focal point position (which changes the beam section S L at the probe position). This was achieved by moving the lens with respect to the entrance of the vacuum chamber. The ratio ΔI e /I e0 was then determined and plotted in Fig. 3 as a function of the fluence E L /S L for two lens positions (the distance lensprobe being equal to 98 cm and 133 cm). (3) where I e0 corresponds to the electron density of the undisturbed plasma and ΔI e to the disturbed electron current increment. In Fig. 2, we present a typical photodetachment signal observed in Ar-C 2 H 2 (80-20%) mixture. 1.44 After each laser pulse, the current undergoes an increase due to the photodetached electrons. This first peak is followed by a series of secondary peaks. These oscillations are explained by the formation of a dynamic sheath at the probe surface due to the fast motion of electrons as compared to ions. As we can see, these oscillations are rapidly damped and they disappear after several microseconds as the plasma relaxes to its equilibrium state. In this study, attention is exclusively focused on the ratio ΔI e /I e0 . We note that when E L /S L is lower than ~18 mJ cm-2, the ratio ΔIe /I e0 increases with the fluence independently of the lens-probe distance. Then it saturates when the fluence reaches ~14 to 18 mJ cm-2 as expected from theory. In addition, for a laser fluence higher than ~18 mJ cm-2, ΔIe /I e0 starts to increase again. This second increase could be related to phenomena other than photodetachment such as multiphoton ionization. In the following, E L /S L has been fixed at ~15 mJ cm-2 by setting the laser energy at 100 mJ and the lens-probe distance at 98 cm. In these conditions, Eq. 3 can be used to directly calculate the ratio of the negative species density to the electron density (n ‒ /n e ). P-II-7-17 Moreover, fitting the data of Fig. 3 by Eq. 1 and Eq. 3 enables to determine the photodetachment cross section σ. It is found to be ~1.4×10ˉ16cm2. The dominant negative species in acetylene discharges have been found to be C 2 Hˉ, C 4 Hˉ and C 6 Hˉ [7] and their corresponding photodetachment cross-sections, for a photon energy of ~4 eV, are 5.05×10-18, 7.72×10-18 and 1.04×10-18 cm2, respectively. The discrepancy between these values and that obtained in our case (two orders of magnitude higher) suggests that the observed photodetachment signal cannot be related only to the negative ions but to other species. These species could be carbon nanoparticles that are known to be negatively charged in acetylene plasmas [8, 9]. If the electron affinity of these nanoparticles is relatively low and their photodetachment cross section is relatively high, they could significantly contribute to the photodetachment signal. 3.1. Effect of the magnetic field and Ar-C 2 H 2 mixture The variation of the ratio n ‒ /n e as a function of the magnetic field intensity is shown in Fig. 4 for two acetylene percentages; 20% and 50%. 0.12 20% C2H2 50% C2H2 n-/ne 0.10 The variation of the n - /n + ratio with the magnetic field and the acetylene percentage is very similar to n ‒ /n e . Their dependence on B can be attributed to an increase in the confinement of positive ions in the center of the plasma as the intensity of the magnetic field augments. This can also be related to the confinement of electrons by the magnetic field. Indeed, the ionization rate increases in the plasma leading thus to the formation of more electrons and positive ions without denying an enhancement in the electron dissociative attachment process which creates negative ions. Moreover, another reason can explain the decrease in the ratio n ‒ /n + . Note that the positive ions can be created from argon as well as from hydrocarbon radicals. As a consequence, their creation rate increases more rapidly with B than the creation rate of the negative ions. Indeed negative ions are only created from hydrocarbon negative ions and from nanoparticles. 3.2. Effect of gas pressure The effect of gas pressure on the n ‒ /n + ratio is presented in Fig. 5 for 20% of C 2 H 2 . It shows a decrease when the pressure increases from 2 to 10 mTorr. Clearly, the decrease rate depends on the magnetic field intensity. For instance, without magnetic field (B = 0) n ‒ /n + decreases from ~0.1 at 2 mTorr to ~0.06 at 10 mTorr, while at 140 G the decease is only ~0.01 (four times lower). 0.12 0.08 0G 140 G 0.10 n-/n+ 0.06 0.04 0 20 40 60 80 100 120 140 Magnetic field (Gauss) Fig. 4. n - /n e as function of B for two C 2 H 2 percentages for 2 mTorr and 350 W. First of all, let us note that the negative species density does not exceed 10% of the electron density. For instance, n ‒ /n e is about 0.1 without magnetic field (B = 0) and it decreases with the magnetic field to reach ~ 0.04 at 140 G. This indicates that the electronegativity of the plasma is rather weak. The decrease rate does not depend much on the acetylene percentage and, for 20% of C 2 H 2 , n ‒ /n e is slightly higher than that obtained for 50% of C2H2. Using the plasma quasi-neutrality condition (i.e., n + = n e + n ‒ ), the negative-to-positive ion density ratio can be deduced from the n - /n e ratio as: n− 1 = n+ 1 + ( n− ) −1 ne P-II-7-17 (4) 0.08 0.06 0.04 0.02 2 4 6 8 Pressure (mTorr) 10 Fig. 5. n - /n + as function of pressure for two values of B for 20% C 2 H 2 and 350 W. Without magnetic field and at low gas pressure, one can assume that the charged species, electrons and positive ions diffuse easily outside the plasma axis due to the ambipolar diffusion to the walls. At high gas pressure, they can no longer spread so easily and they remain confined in the central plasma which results in a decrease of the n ‒ /n + ratio. When applying a magnetic field (140 G) at low pressure (2m Torr), the charged species are already confined and prevented from diffusing outside the plasma center which decreases the effect of the pressure observed without B, as we notice in Fig. 5. 3.3. Absolute density of negative species 3 The absolute value of the negative ion density can be deduced from the n ‒ /n + ratios taking the positive ion density determined from probe measurements. The variation of n ‒ as a function of the magnetic field intensity is shown in Fig. 6 for three C 2 H 2 percentages. 3,0 20% C2H2 50% C2H2 80% C2H2 n- (109cm-3) 2,5 2,0 1,5 1,0 0,5 0,0 0 20 40 60 80 100 120 140 Magnetic field (Gauss) Fig. 6. Variation of n - with B for three percentages of acetylene for 2 mTorr and 350 W. First, n ‒ shows a drop off from ~ 1.5×10 cmˉ at 0G to ~1×109 cmˉ3 at 35 G in the case of 20% of C 2 H 2 . When augmenting further the intensity of the magnetic field, n ‒ increases from ~ 1×109 cmˉ3 reaching a value of ~ 3×109 cm-3 at 140 G. In the other hand, the dependence of n - on the C 2 H 2 percentage is less important except at high magnetic field intensity. For instance, at 140 G n ‒ is higher when the C 2 H 2 percentage is lower. The variation of n ‒ , for 20% C 2 H 2, as a function of the gas pressure is presented in Fig. 7. In general, n ‒ decreases with the gas pressure with a rate depending on the magnetic field intensity. When the gas pressure increases from 2 to 10 mTorr and without a magnetic field, the decrease is ~ 22% while it is ~ 45% when applying a magnetic field (140 G). 9 3 3,0 0G 140 G 2,7 n- (109cm-3) 2,4 2,1 1,8 1,5 1,2 2 4 6 8 Pressure (mTorr) 10 Fig. 7. Variation of n - with pressure for two values of B for 2 mTorr, 20% of C 2 H 2 and 350 W. 4 In acetylene discharges, the nucleation of carbon nanoparticles process strongly depends on the concentration of C 2 H- ions that are expected to be efficiently generated in Ar/C 2 H 2 plasmas [10]. Increasing the magnetic field intensity will induce two important phenomena: i) increase in the dissociative attachment rate of C 2 H 2 molecules leading to the formation of more nanoparticles through chain reactions and ii) increase of the negative species residence time in the plasma, by compensating the gravitational force, leading to an increase in their density. On the other hand, when increasing the percentage of argon in the plasma, the absolute value of the negative species increases signifying that the presence of argon enhances the formation of carbon nanoparticles, through the enhancement of the dissociative attachment over other processes such as for example ionization. As pressure increases, the collision frequency between plasma species increases and therefore the probability of ion-ion recombination rises. This induces a global decrease in the negative species in the plasma. 5. Conclusion In this work, laser photodetachment was used to measure the density of negative species n ‒ in Ar/C 2 H 2 magnetized dusty plasma. The negative ion density n varies non monotonously with B, while it decreases with increasing acetylene percentage and pressure. In addition, the photodetachment cross section is likely to be related to the negatively charged carbon nanoparticles synthesized in the plasma volume. 6. References [1] G.S. Selwyn, J. Singh and R.S. Bennett. J. Vacuum Sci. Technol. A, 7, 2758 (1989) [2] J. Winter. Plasma Phys. Control. Fusion, 40, 1201-1210 (1998) [3] M. Rubel, M. Cecconello, J.A. Malmberg, G. Sergienko, W. Biel, J.R. Drake, A. Hedqvist, A. Huber and V. Philipps. Nuclear Fusion, 41, no 8 (2001) [4] K. De Bleecker, A. Bogaerts and W. Goedheer. Phys. Rev. E, 73, 026405 (2006) [5] M. Moisan and Z. Zakrzewski. J. Phys. D: Appl. Phys., 24, 1025-1048 (1991) [6] M. Bacal, G.W. Hamilton, A.M. Bruneteau and H. J. Doucet. Rev. Sci. Instrum., 50, 719 (1979) [7] T. Best, R. Otto, S. Trippel, P. Hlavenka, A. von Zastrow, S. Eisenbach, S. Jézouin, R.Wester, E. Vigren, M. Hamberg and W.D. Geppert. Astrophys. J., 742 , 63 (2011) [8] J. Benedikt. J. Phys. D: Appl. Phys., 43, 043001 (2010) [9] J. Berndt, E. Kovacevic, I. Stefanovic, O. Stepanovic, S.H. Hong, L. Boufendi and J. Winter. Contrib. Plasma Phys., 49, 107-133 (2009) P-II-7-17 [10] S.H. Hong, J. Berndt and J. Winter. Sources Sci. Tech., 12, 46 (2003) P-II-7-17 Plasma 5
© Copyright 2026 Paperzz