CO2 LASER-DRIVEN REACTIONS IN PURE ACETYLENE FLOW
Журнал: SCIENCE EVOLUTION
Том 2 № 2
, 2017
Рубрики: PHYSICAL SCIENCES
Авторы:
1.
National CRI Center for Nano Particle Control, Institute of Advanced, Machinery and Design, School of Mechanical and Aerospace Engineering, Seoul National University
Россия
Россия
2.
National CRI Center for Nano Particle Control, Institute of Advanced, Machinery and Design, School of Mechanical and Aerospace Engineering, Seoul National University
Россия
Россия
3.
National CRI Center for Nano Particle Control, Institute of Advanced, Machinery and Design, School of Mechanical and Aerospace Engineering, Seoul National University
Россия
Россия
Тип:
Статья
Страницы:
с 96
по 101
Статус:
Опубликован
Получено:
30.12.2017
Одобрено:
30.12.2017
Опубликовано:
30.12.2017
Классификаторы:
ГРНТИ 29.01 Общие вопросы физики
ГРНТИ 27.01 Общие вопросы математики
ГРНТИ 31.01 Общие вопросы химии
ГРНТИ 34.01 Общие вопросы биологии
ГРНТИ 27.01 Общие вопросы математики
ГРНТИ 31.01 Общие вопросы химии
ГРНТИ 34.01 Общие вопросы биологии
Язык материала:
английский
Ключевые слова:
Laser-driven reactions, acetylene decomposition
Аннотация (русский):
We show that multiple-photon absorption of radiation from a 10.56 μm cw CO2 laser by intermediates (ethylene, vinylidene) generated in pure acetylene flow makes them decompose to carbon dimers and excited hydrogen. The latter associates with downstream acetylene to feedback those laser absorbing intermediates thus making the reactions self-sustained in the absence of oxygen. This process is different from acetylene self-decomposition that may occur at higher temperature and pressure. The results of our work may be useful for understanding the generation of various carbon allotropes and interstellar dust from acetylene.
We show that multiple-photon absorption of radiation from a 10.56 μm cw CO2 laser by intermediates (ethylene, vinylidene) generated in pure acetylene flow makes them decompose to carbon dimers and excited hydrogen. The latter associates with downstream acetylene to feedback those laser absorbing intermediates thus making the reactions self-sustained in the absence of oxygen. This process is different from acetylene self-decomposition that may occur at higher temperature and pressure. The results of our work may be useful for understanding the generation of various carbon allotropes and interstellar dust from acetylene.
Ключевые слова:
Laser-driven reactions, acetylene decomposition
Laser-driven reactions, acetylene decomposition
INTRODUCTION Currently there is a growing interest in generation of allotropic carbon solids, polycyclic aromatic hydrocarbons (PAH) and aliphatic hydrocarbons which are found in interstellar space [1-3] along with fullerenes discovered in a planetary nebula [4]. Recently it was found [5] that a light absorption feature in acetylene plasma may coincide with one broad diffuse interstellar band which induces one to take a close look to possible reactions in pure acetylene gas. It was reported earlier [6] that pure acetylene flow inside a diffusion O2/H2 flame generated carbon shell- shaped nanoparticles when irradiated with a 10.56 μm cw CO2 laser in spite of the fact that acetylene practically does not absorb the laser frequency [7]. The generation phenomenon was ascribed in Ref. [6] to the pre-heating of acetylene by O2/H2 flame, the initial pyrolysis and the incipient nanoparticles due to the heating, and then to the surface reactions sped up by additional heating of the incipient nanoparticles by the laser radiation. However, our later experiments [8] demonstrated that the process of nanoparticle generation successfully occurs (after initialisation) in the absence of O2/H2 flame in pure acetylene flow shielded from air and diluted by inert gases (Ar, N2, He) and H2; moreover, many carbon allotropes were found among the nanoparticles, including nanodiamonds [8] (Fig. 1) that could not stand the high temperature in O2/H2 flame and thus were not observed in Ref. [6]. The laser power needed for the generation of shell-shaped nanoparticles turned out to be several times less than found in Ref. [6]. Additionally, PAH are produced and detected in ultraviolet (UV) absorption spectra from extra situ material [3]. The generation of nanoparticles is followed by blazing light from the reaction zone with a clearly non-Planckian broad spectrum in near UV region that tells us about non- thermal way of the reaction. It is useful to mention the review [9] describing allothermal effects that usually lead to diverse carbon structures. In Ref. [8] it was preliminary concluded that the intermediates (e.g. excited ethylene and vinylidene) that absorb the laser radiation [10-12] can keep the reaction going in laser-driven chain reactions aside from the soot-generating reactions; the latter can make acetylene be capable of sustaining a thermal self- decomposition flame only at high pressures and temperatures above 12000C. Here we report on a theoretical description of the laser-driven reactions and compare the results with our experiment where a 10.56 μm cw CO2 laser beam irradiates pure (or diluted with inert gases) acetylene flow shielded from air completely by nitrogen or argon (Fig. 2). The experimental set-up was the same as described in Ref. [6] with the exception that no O2/H2 flame was used (see Fig. 2a for the experimental setup). We additionally experiment with the gas flow rate and the dilution of acetylene. The relevant parameters are the laser power W, the acetylene flow velocity V and the acetylene concentration n=xn0, where x is the dilution ratio (x=1 for pure acetylene) and n0 is the concentration of pure acetylene. We calculate the threshold values of the parameters at which the reaction terminates. Possible thermal acetylene decomposition and surface reactions are ignored in our approach as far as our thermocouple measurements of the gas flow temperature as close as only 2 mm above/below the reaction zone indicated the temperature not exceeding 5000C. This fact excludes the thermal decomposition effects in acetylene at least for not too high laser power. Please cite this article in press as: Pikhitsa P.V., Kim D., and Choi M. CO2 laser-driven reactions in pure acetylene flow. Science Evolution, 2017, vol. 2, no. 2, pp. 96-101. DOI: 10.21603/2500-1418-2017-2-2-96-101. Copyright © 2017, Pikhitsa et al. This is an open access article distributed under the terms of the Creative Commons Attribution 4.0 International License (http:// creativecommons.org/licenses/by/4.0/), allowing third parties to copy and redistribute the material in any medium or format and to remix, transform, and build upon the material for any purpose, even commercially, provided the original work is properly cited and states its license. This article is published with open access at http:// science- evolution.ru/. (a) (b) (c) (d) Fig. 1. Transmission electron microscopy images of (a) shell-shaped carbon nanoparticle [6, 8], (b) single-walled nanohorns (see [20]) collected from the carbon stream, (c) graphene sheets, and (d) nanodiamonds [8]. The inset shows the selected area diffraction pattern for nanodiamonds. B eam stoppe z x Thermo phoretic local y sampling device (TEM) filter (powder collecting) R otary pump Exhaust CW C02 Air shield MFC MFC C2H2 N2 Carbon Lase Z Acetylene Fig. 2. (Color online) The interaction of the acetylene flow with the laser beam. (a) Experimental set-up, (b) The evolution of the reaction zone at different flow rates. The diameter of the inner nozzle is 3 mm. Z is the position of the reaction depending on the gas velocity in the centre (Z=2.5 mm in the photo). Bottom and right panels show successive evolution of the reaction zone with the increasing flow rate from right to left and from top to bottom, respectively. The right panel corresponds to x=0.4 (see Fig. 4a). THEORETICAL Boundary conditions are: The most general and most simplified reaction scheme at z , na n , ne 0 , nh 0 ; for generation laser-absorbing intermediates may be the following: at z , na 0 , ne h 0 , n n . 2 C2H2 + H * 4 C2H *. (1) the concentrations are continuous at z 0 . If we neglect losses ( = 0), neglect diffusion of This general addition reaction (and its variations with acetylene and ethylene (by setting Da 0 and De 0 as participation of charged reagents, of atomic hydrogen etc [13-16]) occurs with the addition reaction rate constant α. far as hydrogen diffusion coefficient h D 1 cm2/s is at 4 The asterisk denotes excited species. Then C2H * decomposes under the CO2 laser irradiation into CH2=C: +H2 and further, vinylidene decomposes into C2 * least 10 times larger) and make substitutions na n exp( ) and nh (V / n)n then Eqs. (5)-(7) can be combined in one equation: and H2 * as was described in Refs. [9-12]. Thus the parent D ( D v) exp( ) v H2 molecule produces two molecules in the branching: * * C2H4 + hv C2 + 2H2 . (2) [1 exp( )] 0 , (9) The system of differential equations that follows from (1) and (2) predicts the critical behaviour with the where D Dh /( n) , v V /( n) , w / V ; then critical gas velocity Vc for given acetylene concentration ne nD v 1 e / 2 . Note that these parameters that can terminate the reaction even at arbitrary high laser power. The exact solution of the corresponding equations have dimensions: [D]=cm2, [ν]=cm, and [ω]=1/cm. By direct substitution one can make sure that when gives the relative position z-z0 of the reaction zone to be v 1 / 2 and v D / 2 (therefore D v 0) compared with the experimental one (Fig. 2b). From the solution we obtained for z an approximation formula suitable for high laser power: Z = z0 + (4Dh / Vc)(1 - V/Vc)-1/2, (3) Eq. (9) has the exact solution: 0 2ln1exp(z z )/ 2D, (10) where Dh is the hydrogen diffusion coefficient; Then for the concentrations one obtains: 2 n n z z0 ; n ; z z 0 Vc 2 nDh 2 n0 Dh x V1 x . (4) a 4 1 tanh 2 2D nh 2 1 tanh 2 2D Let us derive Eqs. (3), (4). The reactions in Eqs. (1) n n cosh2 z z0 . (11) (2), can be described by the following one dimensional steady-state differential equations (prime denotes differentiation on z): e 4 2 2D V na na nh na Da na , (5) The presence of z0 means that there is an arbitrary position of the soliton solutions in Eq. (11). Thus the reaction zone can be “blown up” arbitrarily high and V n e na nh ne w ( z ) ne De n e , (6) parameters v 1 / 2 and v D / 2 are therefore V nh na nh nh 2w( z) ne Dh nh , (7) critical for the reaction. Returning to dimensional where parameters one gets wthr w0 n / 2 . Vthr nDh / 2 and w w(z) 0 z 0 z 0 . (8) Let us show that the parameter values obtained above are on the critical curve which separates reaction/no reaction regions in the parameter domain. The curve can Here w (an increasing function of the laser power be found from Eqs. (5)-(7) after their linearization at W [10, 12]) is the rate of laser induced decomposition of the infrared-absorbing intermediate (with concentration (n na ), ne , nh n with the solution in form of ne and diffusion coefficient De) which we will conventionally call “ethylene” though, as we said above, vinyl radical and vinylidene can participate as well; na , exp( z z0 ) , 0 , that corresponds to the asymptotic solution of the soliton type when the soliton is far on the right side from z=0, therefore for Eq. (11) z0 z 1 and 0 e n nexp(z z ) 2D from Eq. (11). Da and nh , Dh - concentrations and diffusion coefficients 2 2D of acetylene and hydrogen, respectively; V is the gas Thus, thr 1 2D n (2Dh ) is found from the velocity in the direction of the vertical coordinate z ; prime denotes the derivative with respect to z ; describes losses in the real system. Eq (8) describes the asymptotic of the exact solution of Eq. (11). One finds from linearized Eq. (6), (7) half-infinite laser beam which simplification allows (V 2 De )(V n 2 Dh ) analytical results. Pressure effects are not taken into account here, as far as the C2 vapor quickly condenses into carbon nanoparticles in the reaction zone and thus the number of gas molecules can be considered nearly w h V n D 2 h (V )(V n D 2 ) 2 (12) constant. V n Dh as far as we neglected and De for simplification. One observed in our experiment (see Fig. 2). There is no reaction can make sure that for 0 not any positive values of w are possible. At a given V the value of w which is a marginal value separating existing and non-existing solutions is given by the equation: w 0 . (13) Eq. (13) can be rewritten as: 2 in the centre of the reaction zone when the velocity there is above Vc. The laser power was 900 W and the beam diameter was around 2 mm thus the power density of 7162 W/cm2 can be considered as a high power density [12]. Note the blue- violet light [19] from the lower part of the reaction zone which may indicate acetylene/hydrogen plasma emission. Also there is the low power threshold for the laser power [12] as far as multi-photon processes are involved. For the precise determination of the critical velocity one has to calculate the position of the reaction zone and to follow its change with the gas velocity or dilution. From V n / Dh 2n n / Dh . (13a) computing Eqs. (5)-(8) for two different rates w/w0=1 (exact Both of Eqs. (12), (13a) define the critical diagram shown in Fig. 3a. The direct substitution of the solution) and w/w0=100 we found the position of the reaction zone at velocities V approaching the threshold velocities Vthr (Fig. 3b,c). Using the boundary conditions at z=0 one can parameter values (thr n (2Dh ), Vthr nDh / 2, show that for the location of the reaction zone maximum z -1 -1/2 and wthr n / 2) found above for the exact solution of Eq. there is an asymptotic z = z0 +A βc (1-V/Vthr) . into Eqs. (12), (13a) satisfies them. Therefore, the soliton solution is indeed a threshold solution. As one can derive from Eqs. (12), (13), the critical diagram in Fig. 3a has Dimensionless A, which is difficult to calculate analytically in a general case, may slightly vary with w. One can make a good approximation in Fig. 3d for two superposed dependencies calculated at very different w with A 2 the critical velocity of Eq. (4) Vc 2 nDh 2 n0 Dh x -1/2 (then c n / Dh and wc ). z=z0 + (4Dh / Vc)(1 - V/Vthr) (14) If the gas velocity overcomes the critical velocity, no laser power can support the reaction. This phenomenon is which leads to Eq. (3) for high power as far as Vthr=Vc. The shift z0 was adjusted to superpose data on one curve. Reaction w/wO ne/n w = wthr = 100wO soliton v/vC z∗f3C (b) ne/n z∗f3C w = wthr = wO 2∗(1 - V/Vthr )-1/2 + canst z∗f3C (1 - V/VthrC)-1/2 (c) (d) Fig. 3. (Color online) The laser-driven reaction in acetylene: (a) The critical diagram for the reaction from Eqs. (12), (13). The area under the critical curve corresponds to no reaction. Arrows indicate the approach to the threshold velocities at two different values of the power; (b), (c) computer solutions of Eq. (5)-(8) for the concentration of intermediates at approaching the threshold velocity at the power of the exact soliton solution and at the power 100 times more, correspondingly; (d) the approximation of the “universal” position dependency. COMPARISON WITH EXPERIMENT AND DISCUSSION Let us compare Eq. (3) with the experimental data shown in Fig. 4 a, b. The transformation coefficient from flow rate to gas velocity is 0.25 cm s-1 (ccm/min)-1 that is the critical flow of 338 ccm/min in Fig. 4b corresponds to Vc = 84.5 cm/s at this dilution of x=0.6. Fitting the experimental dependency of the position z of the reaction zone against the gas velocity at dilution x=0.6 (x=0.4) gives values of Dh = 2.5 cm2/s (Dh =2.87 cm2/s) and an0 = 1000 s-1 (an0 = 1150 s-1) and therefore from Eq. (4) V1 = 101cm/s (V1 = 115cm/s). Additionally, Eq. (4) was used for fitting the velocities when the reaction zone starts breaking into halves (eye observation) at various dilutions which gives V1 = 96.2 cm/s (see Fig. 4c). The calculated value βc=2 mm-1 gives additional opportunity to check our theory by measuring the light intensity spatial distribution near the edge of the reaction zone by using a digital camera. We took images of the reaction zone at different shutter speeds thus controlling the position of the apparent reaction edge seen by the digital camera (Fig. 5). The plot of the shutter speed against the edge position determined from the images gives the distribution of the intensity of the reaction (Fig. 5) with the characteristic spatial decay parameter β=2.5 mm-1. A reasonable agreement between theoretical values and the experimental ones supports the mechanism for the acetylene conversion to carbon through laser absorbing gaseous intermediates. Their decomposition and the following condensation of resulting carbon dimers at low-temperature conditions leads to the metastable carbon [8] including nanodiamonds. The metastable carbon rapidly transforms into continuous layer shell-shaped carbon nanoparticles or nanohorns [20] (Fig. 1) under the laser beam similar to [17] where crystallization in 50 milliseconds of a carbon nanotube from an amorphous nanotube was reported. Note that the case of pure ethylene is different. First, no splitting of the reaction zone is observed as far as ethylene fuel is absorbing the laser power [8] and also the feedback scheme described by Eq. (1) does not work for pure ethylene. Second, it is seen that the reaction is supported by too extensive heating of the reaction zone with twice more hydrogen and the products which are mostly soot-like carbon [18] and PAH. Yet, acetylene might also be created in this process [11, 19] and then additionally participate in the reaction according to the mechanism described above. However the reaction intensity should be lower than for pure acetylene as we indeed observe in our experiment. Position (mm) Position (mm) Total flow (ccm/min) dilution x=0.4 dilution x=0.6 Total flow (ccm/min) Total flow (ccm/min) Dilution x (a) (b) (c) Fig. 4. Experimental data on the reaction zone evolution with the change in the gas velocity. (a) The position of the reaction zone against the acetylene velocity at dilution ratio x=0.4 and (b) x=0.6. Squares are experimental; the line is the fitting by Eq. (3). (c) The critical flow for the interruption of the reaction zone vs. dilution (squares). The line is the fit with Eq. (4). Shutter speed, s-1 Distance, mm Fig. 5. (Color online) The reaction intensity profile measured indirectly by the position of the luminous reaction edge (lower part of the reaction zone) seen by the digital camera at different shutter speeds. Five data points (filled circles) correspond to five images on the left. The red line is the exponential fit which gives β=2.5 mm-1 to be compared with βc=2 mm-1 that is calculated with Dh =2.5 cm2/s and an0 = 1000 s-1. CONCLUSIONS In conclusions, grounding on the theoretical description of our experiment we suggested steady state laser-driven reactions in pure acetylene flow that may be interesting for further investigation of number of processes in hydrocarbons: from tailored synthesis of carbon allotropes to photochemistry of hydrocarbons and the understanding of interstellar grains. ACKNOWLEDGEMENTS Financial support from the Acceleration Research Program supported by the Korean Ministry of Science and Technology is gratefully acknowledged. Support from the BK21 program and WCU (World Class University) multiscale mechanical design program through the Korea Research Foundation is also gratefully acknowledged. P.V.P. thanks Fyodor Sirotkin for taking photos of the reaction zone.
1. Jager C., Mutschke H., Henning Th., and Huisken F. Spectral Properties of Gas-phase Condensed Fullerene-like Carbon Nanoparticles from Far-ultraviolet to Infrared Wavelengths. The Astrophysical Journal, 2008, vol. 689, no. 1, pp. 249-259.
2. Biennier L., Georges R., Chandrasekaran V., et al. Characterization of circumstellar carbonaceous dust analogues produced by pyrolysis of acetylene in a porous graphite reactor. Carbon, 2009, vol. 47, no. 14, pp. 3295-3305. DOI:https://doi.org/10.1016/j.carbon.2009.07.050.
3. Pikhitsa P.V., Kim Y.J., Kim M.W., Yang S., Noh T.W., and Choi M. Optical manifestations of the condensation of topological defects in continuous layer multishell carbon nanoparticles. Physical Review B, 2005, vol. 71, no. 7, p. 073402. DOI:https://doi.org/10.1103/PhysRevB.71.073402.
4. Cami J., Bernard-Salas J., Peeters E., and Malek S.E. Detection of C60 and C70 in a Young Planetary Nebula. Science, 2010, vol. 329, no. 5996, pp. 1180-1182. DOI:https://doi.org/10.1126/science.1192035.
5. Linnartz H., Wehres N., Van Winckel H., et al. A coincidence between a hydrocarbon plasma absorption spectrum and the λ5450 DIB. Astronomy and Astrophysics, 2010, vol. 511, L3. DOI: https://doi.org/10.1051/0004-6361/201014019.
6. Choi M., Altman I.S., Kim Y.J., Pikhitsa P.V., et al. Formation of Shell-Shaped Carbon Nanoparticles Above a Critical Laser Power in Irradiated Acetylene. Advanced Material, 2004, vol. 16, no. 19, pp, 1721-1725. DOI:https://doi.org/10.1002/adma.200400179.
7. Förster J., Hagen Th., von Hoesslin M., and Uhlenbusch J. Journal of Applied Physics, 1996, vol. 62, 263.
8. Pikhitsa P.V., Kim Y.J., and Choi M. Proc. of 4th Asian Aerosol Conference. Mumbai, 2005, pp. 18-19.
9. Gonzalez-Aguilar J., Moreno M., and Fulcheri L. Carbon nanostructures production by gas-phase plasma processes at atmospheric pressure. Journal of Physics D: Applied Physics, 2007, vol. 40, no. 8, p. 2361.
10. Chekalin N.V., Letokhov V.S., Lokhman V.N., and Shibanov A.N. Primary products of multiphoton dissociation of the C2H4 molecule in an intense IR field. Chemical Physics, 1979, vol. 36, no. 415-421. DOI:https://doi.org/10.1016/0301-0104(79)85025-9.
11. Gordienko V.M., Danilov E.O., Platonenko V.T., and Slobodyanyuk V.A. Multiphoton excitation and dissociation of ethylene by intense 10 μm picosecond pulses. Journal of Molecular Structure, 1995, vol. 349, pp. 219-221. DOI:https://doi.org/10.1016/0022-2860(95)08748-K.
12. Letokhov V.S. Nonlinear laser chemistry: Multiple-photon excitation. Springer Series in Chemical Physics, vol 22. New York, 1983.
13. Payne W.A. and Stief L.J. Journal of Chemical Physics, 1976, vol. 64, pp. 1150.
14. Maluendes S.A., McLean A.D., and Herbst E. New calculations on the ion-molecule processes C2H+2 + H2 → C2H+3 + H and C2H+2 + H2 → C2H+4. Chemical Physics Letters, 1994, vol. 217, pp. 571-576. DOI:https://doi.org/10.1016/0009-2614(93)E1427-I.
15. Toyoda H., Childs M.A., Menningen K.L., Anderson L.W., and Lawler J.E. Ultraviolet spectroscopy of gaseous species in a hot filament diamond deposition system when C2H2 and H2 are the input gases. Journal of Applied Physics, 1994, vol. 75, no. 6, pp. 3142. DOI: https://doi.org/10.1063/1.356169.
16. Smith J.A., Cameron E., Ashfold M.N.R., Mankelevich Y.A., and Suetin N.V. In the mechanism of CH3 radical formation in hot filament activated CH4/H2 and C2H2/H2 gas mixtures. Diamond and Related Materials, 2001, vol. 10, no. 3-7, pp. 358-363. DOI:https://doi.org/10.1016/S0925-9635(00)00443-X.
17. Huang J.Y., Chen S., Ren Z.F., Chen G., and Dresselhaus M.S. Real-Time Observation of Tubule Formation from Amorphous Carbon Nanowires under High-Bias Joule Heating. Nano Letters, 2006, vol. 6, no. 8, pp. 1699-1705. DOI:https://doi.org/10.1021/nl0609910.
18. Morjan I., Voicu I., Dumitrache F., et al. Carbon nanopowders from the continuous-wave CO2 laser-induced pyrolysis of ethylene. Carbon, 2003, vol. 41, no. 15, pp. 2913-2921. DOI:https://doi.org/10.1016/S0008-6223(03)00381-6.
19. Kozlov G.I. Some laws governing laser beam ignition of an ethylene stream in air.Technical Physics Letters, 1997, vol. 23, no. 12, pp. 964-965. DOI: https://doi.org/10.1134/1.1261751.
20. Azami T., Kasuya D., Yoshitake T., et al. Production of small single-wall carbon nanohorns by CO2 laser ablation of graphite in Ne-gas atmosphere. Carbon, vol. 45, no. 6, pp. 1364-1367. DOI:https://doi.org/10.1016/j.carbon.2007.02.031.
