<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">APM</journal-id><journal-title-group><journal-title>Advances in Pure Mathematics</journal-title></journal-title-group><issn pub-type="epub">2160-0368</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/apm.2013.33049</article-id><article-id pub-id-type="publisher-id">APM-31234</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Derivation of Moment Equations for the Theoretical Description of Electrons in Nonthermal Plasmas
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>arkus</surname><given-names>M. Becker</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Detlef</surname><given-names>Loffhagen</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Leibniz Institute for Plasma Science and Technology, Greifswald, Germany</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>markus.becker@inp-greifswald.de(AMB)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>08</day><month>05</month><year>2013</year></pub-date><volume>03</volume><issue>03</issue><fpage>343</fpage><lpage>352</lpage><history><date date-type="received"><day>December</day>	<month>11,</month>	<year>2012</year></date><date date-type="rev-recd"><day>February</day>	<month>17,</month>	<year>2013</year>	</date><date date-type="accepted"><day>March</day>	<month>19,</month>	<year>2013</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
   The derivation of moment equations for the theoretical description of electrons is of interest for modelling of gas discharge plasmas and semiconductor devices. Usually, certain artificial closure assumptions are applied in order to derive a closed system of moment equations from the electron Boltzmann equation. Here, a novel four-moment model for the description of electrons in nonthermal plasmas is derived by an expansion of the electron velocity distribution function in Legendre polynomials. The proposed system of partial differential equations is consistently closed by definition of transport coefficients that are determined by solving the electron Boltzmann equation and are then used in the fluid calculations as function of the mean electron energy. It is shown that the four-moment model can be simplified to a new drift-diffusion approximation for electrons without loss of accuracy, if the characteristic frequency of the electric field alteration in the discharge is small in comparison with the momentum dissipation frequency of the electrons. Results obtained by the proposed fluid models are compared to those of a conventional drift-diffusion approximation as well as to kinetic results using the example of low pressure argon plasmas. It is shown that the results provided by the new approaches are in good agreement with kinetic results and strongly improve the accuracy of fluid descriptions of gas discharges. 
 
</p></abstract><kwd-group><kwd>Moment Equations; Plasma Modelling; Electron Transport</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Nonthermal plasmas are widely used in many technical applications including plasma display panels, energy saving lamps, devices for microbial decontamination and ozonizers [1-4]. They are characterized by low gas temperatures <img src="6-5300411\529b18dd-2772-4408-8dc1-5a894f264640.jpg" /> in the range from 300 to 1000 K and comparatively high mean electron energies <img src="6-5300411\653586fc-3fe2-4dd0-a130-71d068bf2052.jpg" /> between 1 and 10 eV, where 1 eV corresponds to temperature of 11605 K. Computer simulations of electric gas discharges producing nonthermal plasmas are used since many years to get a deeper understanding of fundamental processes and to improve technical devices [5-10]. In order to describe all phenomena taking place in the discharge mechanism, in principle, a mathematical model comprising the kinetic Boltzmann equation [<xref ref-type="bibr" rid="scirp.31234-ref11">11</xref>]</p><disp-formula id="scirp.31234-formula123336"><label>(1)</label><graphic position="anchor" xlink:href="6-5300411\98a4d6d5-3ca2-4dcf-8866-5d04911ea965.jpg"  xlink:type="simple"/></disp-formula><p>for the distribution function <img src="6-5300411\faa4b1f9-31ed-4630-bda7-d832d63b8278.jpg" /> of each gas species “s” with charge <img src="6-5300411\9dabb4ad-24d0-4249-b594-a1100fca35c3.jpg" /> and mass <img src="6-5300411\f00b87bc-2af7-4a0d-b086-94825dbfd089.jpg" /> in seven-dimensional space of<img src="6-5300411\70bf8582-e722-4a13-907f-0d1839ee347c.jpg" />, velocity</p><p><img src="6-5300411\217e1bef-b904-465e-b34e-977264b5a2e2.jpg" />and time <img src="6-5300411\e785175e-7c05-46d2-a527-13c2d932a3c7.jpg" /> has to be solved in combination with Maxwell’s equations for the electric field <img src="6-5300411\5d4157d7-d643-4808-99d9-cbc9107499ab.jpg" /> and the magnetic field<img src="6-5300411\f7ea225f-59a2-481c-9d36-a05d224c444d.jpg" />. The right-hand side in (1) accounts symbolically for the change in the distribution function due to collision processes. However, such system is not solvable in reasonable computing time and several simplifying assumptions have to be taken into account. For the nonthermal plasmas under consideration, magnetic fields are negligible, and, instead of the hole system of Maxwell’s equations, the Poisson equation</p><disp-formula id="scirp.31234-formula123337"><label>(2)</label><graphic position="anchor" xlink:href="6-5300411\89e5cdbb-a4c8-4f3c-a14f-c41f29a08c93.jpg"  xlink:type="simple"/></disp-formula><p>for the electric potential <img src="6-5300411\4d12d07e-94a3-4dd3-b5d6-93fad7d0db29.jpg" /> is solved for determination of the electric field<img src="6-5300411\3deed7e9-b8ba-4db7-a979-95c1ae1922d6.jpg" />, where <img src="6-5300411\0315f302-9a5d-450f-a757-39439dd40fc1.jpg" /> is the number of gas species with densities <img src="6-5300411\12bbbdae-f2d4-45a1-9ec3-dc1ceade50b2.jpg" /> and <img src="6-5300411\d39bdbc6-dd7a-4181-bcd2-697e3515dbe5.jpg" /> denotes the permittivity of free-space. Furthermore, heavy particles are frequently assumed to be in thermodynamic equilibrium and macroscopic fluid equations with constant temperature <img src="6-5300411\da7d4059-ca77-42a8-bc27-047e0cf82e09.jpg" /> are taken into account for tracing the spatiotemporal behaviour of ions and neutral particles [12-15]. In contrast, the non-local kinetics of electrons plays an important role in the discharge mechanisms and the application range of fluid models which do not describe electrons adequately is very limited [16-18]. Therefore, hybrid models are frequently used in which fluid equations are solved for heavy particles and electrons are treated kinetically [19-21]. However, it has been pointed out recently that fluid models are able to capture electron kinetic effects, if the electron energy flux is adequately described [22,23].</p><p>In the present paper, a high order fluid model comprising moment equations for particle density, particle flux, energy density and energy flux of the electron component is consistently derived from the electron Boltzmann equation. In addition a novel drift-diffusion approximation for electrons is proposed. Results are compared to those of a conventional drift-diffusion model frequently used [24,25] and to kinetically obtained results at the example of argon gas discharge plasmas.</p></sec><sec id="s2"><title>2. Kinetic Description of Electrons</title><p>In spite of the increasing speed of computers, the solution of the electron Boltzmann equation in seven dimensions is computationally not feasible. A conventional approach for reducing computing time is to decrease dimensionality by decomposition of the electron velocity distribution function (evdf) <img src="6-5300411\a7f5823b-0634-4151-b8df-50678f8d9656.jpg" />in terms of spherical harmonics in velocity space [26,27]. In the planar system considered in the present studies and depicted in <xref ref-type="fig" rid="fig1">Figure 1</xref>, where all gradients and the electric field are assumed to be normal to the electrodes, the general spherical harmonics expansion reduces to the Legendre polynomial expansion [27,28]</p><disp-formula id="scirp.31234-formula123338"><label>(3)</label><graphic position="anchor" xlink:href="6-5300411\8152542a-2490-4b76-97cf-2d64f111ed01.jpg"  xlink:type="simple"/></disp-formula><p>In this case the velocity distribution function becomes symmetric around the electric field and depends on the space coordinate<img src="6-5300411\a8ee3a09-1506-4c19-899d-26f34d1abebf.jpg" />, the velocity magnitude<img src="6-5300411\5387ef34-ede1-4f32-961c-f5eb37d352a0.jpg" />, the direction cosine <img src="6-5300411\db431884-a4a8-46cf-b3fb-fda724fd2064.jpg" /> and time. The substitution of the expansion (3) into the electron Boltzmann equation</p><disp-formula id="scirp.31234-formula123339"><label>(4)</label><graphic position="anchor" xlink:href="6-5300411\ad96ff0b-dbe0-4ea5-aed0-66f4cc74ce79.jpg"  xlink:type="simple"/></disp-formula><p>with elementary charge <img src="6-5300411\81d028a6-f764-4207-859f-2db3e4160f86.jpg" /> and the transformation of the expansion coefficients into the space of kinetic energy <img src="6-5300411\e2daf374-8fc9-4f95-bdce-230496cd1720.jpg" /> according to</p><disp-formula id="scirp.31234-formula123340"><label>(5)</label><graphic position="anchor" xlink:href="6-5300411\0362fc8d-ad9b-44b0-960b-6759b20af5c3.jpg"  xlink:type="simple"/></disp-formula><p>finally yields the infinite system of partial differential equations [<xref ref-type="bibr" rid="scirp.31234-ref16">16</xref>]</p><disp-formula id="scirp.31234-formula123341"><label>(6a)</label><graphic position="anchor" xlink:href="6-5300411\835fb78c-37fa-4702-aa87-4db6f85b4cca.jpg"  xlink:type="simple"/></disp-formula><p><img src="6-5300411\29517be8-dd51-4950-ad16-94fdd71702b1.jpg" /></p><p>(6b)</p><p>for the expansion coefficients<img src="6-5300411\060870ff-2bfc-4a37-a61f-d3024de50ca3.jpg" />. Here, <img src="6-5300411\7af449ae-9bb2-403d-a01d-c61fe6662ee0.jpg" />and <img src="6-5300411\19c7558d-d953-4804-9ce0-ddfbaa8d9672.jpg" /> are the cross sections of elastic and inelastic collisions of electrons with heavy particles with density <img src="6-5300411\eff6865a-71ae-4afd-b3ac-535efa9cf23f.jpg" /> and mass <img src="6-5300411\17b13746-a649-4518-a597-88d769576fc1.jpg" /> and <img src="6-5300411\9f32b632-ae96-416a-9795-460f1f8ad29f.jpg" /> and <img src="6-5300411\712d87af-80e4-4d8b-8a63-f6b261edeee7.jpg" /> denote the number of heavy particle species and reactions, respectively. The kinetic energy that is lost in the corresponding inelastic electron collision is denoted by <img src="6-5300411\22154e1b-1729-4953-9749-d098a25dc278.jpg" /> and the parameter <img src="6-5300411\3855cafd-9f1c-4222-9814-b0281eee0be0.jpg" /> depends on the different kinds of inelastic electron collision processes. It is zero for dissociative attachment of electrons and one for excitation, dissociation and deexcitation processes. Using the assumption that the binding energy is equally shared between the two released electrons <img src="6-5300411\55f9746a-8698-4222-9662-174628df814f.jpg" /> equals two for an ionization event [<xref ref-type="bibr" rid="scirp.31234-ref16">16</xref>].</p><p>In order to solve system (1), it has to be truncated after a reasonable finite number of equations. Within the common framework of the two-term expansion [29-31], only the first two equations for <img src="6-5300411\efeaea27-a52a-47b5-bfb6-45140350d4d0.jpg" /> and <img src="6-5300411\1b985946-ae01-4e49-8798-c6ab43462a7c.jpg" /> are taken into account and <img src="6-5300411\7d29687c-72df-4712-9f79-be65fae542aa.jpg" /> is set to zero for<img src="6-5300411\91847c26-efa1-4e0c-bbe2-f001e8448c00.jpg" />. Usually, the rapidity of the temporal change of the anisotropic distribution f<sub>1</sub> is by some orders of magnitude greater than that of the isotropic distribution f<sub>0</sub> as long as the characteristic frequency for the field alteration is small compared to the power dissipation in elastic and inelastic collisions [<xref ref-type="bibr" rid="scirp.31234-ref30">30</xref>]. In this case, the time derivative term <img src="6-5300411\c608ebe7-f54d-4140-9592-10d955472343.jpg" /> in (7) for<img src="6-5300411\a2556fc9-aac0-430f-bdb4-9c9cd8912e90.jpg" />, which describes the establishment of <img src="6-5300411\1cc6f58a-3024-4b7d-8526-e4416c310a50.jpg" /> into the quasi-stationary state</p><p><img src="6-5300411\06014053-43e0-4c42-bc24-24c29240ae2a.jpg" /></p><p>(7)</p><p>can be neglected. If in this case <img src="6-5300411\b6c9ac2c-2707-4025-b88c-fe7b78680a06.jpg" /> is set to zero for<img src="6-5300411\f4754fa3-a051-406a-8fc8-b88413e27e51.jpg" />, the system (6) reduces to the single parabolic differential Equation (6a) using the expression (7) with <img src="6-5300411\9eed4d74-761e-4e37-9d6d-3f469bdfcda5.jpg" /> for the anisotropic contribution <img src="6-5300411\9dae2804-4e97-4fb1-9ad8-46832f813432.jpg" /> to the evdf [<xref ref-type="bibr" rid="scirp.31234-ref30">30</xref>].</p><p>In the past, the system (6) has been solved in two-term approximation [29,30] using the expression (7) with <img src="6-5300411\2d338ae6-2e2b-409e-911b-69c69de50dfb.jpg" /> as well as in multiterm approximation considering higher order contributions to the evdf anisotropy [32-35] to study the behaviour of electrons in prescribed time-dependent as well as stationary electric fields. But the coupled solution (stationary or time-dependent) of the kinetic Equations (6) for electrons, fluid equations for heavy particles and Poisson’s equation for the electric field is still an ambitious task and has been achieved for a few discharge situations, only [21,36-38]. In the following a macroscopic system of moment equations is consistently derived from the system (6), which strongly simplifies the description of electron transport.</p></sec><sec id="s3"><title>3. Macroscopic Transport Equations for Electrons</title><sec id="s3_1"><title>3.1. Four-Moment Model</title><p>The derivation of a system of moment equations for the description of electrons in nonthermal plasmas starts from the kinetic system (6). Multiplication of Equation</p><p>(6a) by factors <img src="6-5300411\040ba683-10f1-4bc1-bd3f-03d647f52f30.jpg" /> and<img src="6-5300411\37728fef-06df-44ed-95ad-68cf7c887aea.jpg" />, respectively, and subsequent integration over kinetic energy U directly provides the two moment equations</p><disp-formula id="scirp.31234-formula123342"><label>(8a)</label><graphic position="anchor" xlink:href="6-5300411\52da2914-72fe-4535-9aff-5dfc89c62c9a.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.31234-formula123343"><label>(8b)</label><graphic position="anchor" xlink:href="6-5300411\8c905a3e-d0bf-494a-8322-e792c0d71b65.jpg"  xlink:type="simple"/></disp-formula><p>with macroscopic quantities</p><disp-formula id="scirp.31234-formula123344"><label>(9)</label><graphic position="anchor" xlink:href="6-5300411\47a95fed-0c97-4c5f-b4ce-07679834f26f.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.31234-formula123345"><label>(10)</label><graphic position="anchor" xlink:href="6-5300411\0e0655ca-eee0-4d61-9e09-0beced1d8ec7.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.31234-formula123346"><label>(11)</label><graphic position="anchor" xlink:href="6-5300411\dcaf4332-56e5-4ac9-86ed-e29588f1d6b3.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.31234-formula123347"><label>(12)</label><graphic position="anchor" xlink:href="6-5300411\363da4a4-6605-48d8-9c1d-7956078efbed.jpg"  xlink:type="simple"/></disp-formula><p>The source terms <img src="6-5300411\47536a0f-ed85-49a1-ad4a-2c0c4824a393.jpg" /> and <img src="6-5300411\aeea8c03-e927-4948-adde-6deebefbcc6f.jpg" /> in Equations (8a) and (8b) describe the gain and loss of particles and energy due to collision processes. For a specific gas, they are given as the sum of rates of all relevant processes with rate coefficients depending on the mean electron energy<img src="6-5300411\24a2cb84-3747-4093-b07e-c3fb20c9ce78.jpg" />, see, e.g., [15,16] for more details.</p><p>In order to consistently derive partial differential equations for the determination of the particle flux (11) and the energy flux (12), Equation (6b) for <img src="6-5300411\f76bd120-0b9b-4eb9-9e1d-8bbf8aa6a1dc.jpg" /> is multiplied by factors <img src="6-5300411\5c0e2dac-92d4-4b45-b584-f420b5e6fdd9.jpg" /> and<img src="6-5300411\77b6d761-ec37-48ed-9a3a-60fce394182a.jpg" />, respectively. As before, subsequent integration over kinetic energy <img src="6-5300411\ad1513e1-f9a7-4424-a819-4b32db819087.jpg" /> yields the two moment equations</p><p><img src="6-5300411\7deff47e-d119-4eb0-882f-f7289741421c.jpg" /></p><p>(13a)</p><p><img src="6-5300411\6449648e-d5f9-4ae3-8acd-da3fed26817d.jpg" /></p><p>(13b)</p><p>with the mean free path of electrons</p><disp-formula id="scirp.31234-formula123348"><label>(14)</label><graphic position="anchor" xlink:href="6-5300411\a962d8b5-55db-4164-85f8-55b17ffe4b3a.jpg"  xlink:type="simple"/></disp-formula><p>The definition of the set of transport coefficients</p><disp-formula id="scirp.31234-formula123349"><label>(15a)</label><graphic position="anchor" xlink:href="6-5300411\009fa0fe-0904-4508-81e1-4be9fb60f873.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.31234-formula123350"><label>(15b)</label><graphic position="anchor" xlink:href="6-5300411\df862df5-dedb-49e3-8e80-3119db66e1b0.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.31234-formula123351"><label>(15c)</label><graphic position="anchor" xlink:href="6-5300411\a316a7e8-cb95-4df5-b211-52f34b6b495f.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.31234-formula123352"><label>(15d)</label><graphic position="anchor" xlink:href="6-5300411\9af38315-ffd1-418d-980d-af6caf76c62a.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.31234-formula123353"><label>(15e)</label><graphic position="anchor" xlink:href="6-5300411\336744ae-f82d-49bf-a6d9-25cefee79180.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.31234-formula123354"><label>(15f)</label><graphic position="anchor" xlink:href="6-5300411\5c38e098-280a-46ca-af70-85ee982c1499.jpg"  xlink:type="simple"/></disp-formula><p>with the mean velocity of electrons <img src="6-5300411\b2b8d0bf-7701-4275-be98-a999a326fe75.jpg" /> allows to write the four-moment model (4MM) for electrons in the form</p><disp-formula id="scirp.31234-formula123355"><label>(16a)</label><graphic position="anchor" xlink:href="6-5300411\705d647d-6c57-448c-8318-cf40efecdfb8.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.31234-formula123356"><label>(16b)</label><graphic position="anchor" xlink:href="6-5300411\89f98e56-742d-4fcb-acce-72ca7f802b97.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.31234-formula123357"><label>(16c)</label><graphic position="anchor" xlink:href="6-5300411\07e3f71a-1164-4225-a00f-cef11e3799e7.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.31234-formula123358"><label>(16d)</label><graphic position="anchor" xlink:href="6-5300411\a2180f4b-34cb-4fbc-8415-f31be50389b3.jpg"  xlink:type="simple"/></disp-formula><p>Electron transport coefficients used in fluid calculations are commonly obtained by solving the kinetic system (6) in multiterm approximation [<xref ref-type="bibr" rid="scirp.31234-ref16">16</xref>] or in twoterm approximation [<xref ref-type="bibr" rid="scirp.31234-ref39">39</xref>] for given values of the electric field, neglecting spatial and temporal derivatives. The resulting coefficients are then put into lookup tables as functions of the mean electron energy for the usage in fluid calculations. The same procedure, known as localmean-energy approximation [16,40], is used for the determination of the new transport coefficients (15).</p></sec><sec id="s3_2"><title>3.2. Drift-Diffusion Approximation</title><p>As mentioned in Section 2, the rapidity of the temporal change of the anisotropic distribution <img src="6-5300411\66bb91d8-acab-4189-8f9c-1985f58dec54.jpg" /> is by some orders of magnitude greater than that of the isotropic distribution <img src="6-5300411\b3ec29b9-ceac-46d9-8bc5-20b17fab4176.jpg" /> and the time derivative in Equation (6b) for <img src="6-5300411\04ae324d-4ed2-4fbe-b685-d51c1c6603ff.jpg" /> can be neglected in many discharge situations. With this assumption and definition of the coefficient</p><disp-formula id="scirp.31234-formula123359"><label>(17)</label><graphic position="anchor" xlink:href="6-5300411\8c867f47-cc55-4458-88a6-30acd33e58a0.jpg"  xlink:type="simple"/></disp-formula><p>the new drift-diffusion approximation (DDAn)</p><disp-formula id="scirp.31234-formula123360"><label>(18a)</label><graphic position="anchor" xlink:href="6-5300411\d59885aa-36b3-43ec-b6b2-b1d08953d83a.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.31234-formula123361"><label>(18b)</label><graphic position="anchor" xlink:href="6-5300411\052e6b27-7de4-496f-a127-170b7149881c.jpg"  xlink:type="simple"/></disp-formula><p>is obtained for the particle flux <img src="6-5300411\b72458b1-e0bf-4f55-9644-62b39f11edc8.jpg" /> and energy flux <img src="6-5300411\a72fd388-faf0-4182-b2ba-7e348405855c.jpg" /> of the electrons. Substitution of (18a) and (18b) into Equations (16a) and (16c), respectively, reduces the fourmoment model to a system of two parabolic differential equations for the particle density <img src="6-5300411\27506ed7-8b41-4b52-9f68-56155ce7c4ff.jpg" /> and the energy density <img src="6-5300411\5e5813fd-2d74-4551-aebe-ac7446d1d56a.jpg" /> of electrons. The coefficient (17) is determined in the same way as the coefficients (15).</p><p>As an example, the transport coefficients (15) used in the four-moment model (16) and the drift-diffusion approximation (18) are shown in <xref ref-type="fig" rid="fig2">Figure 2</xref> for argon gas, where the underlying cross sections are detailed in reference [<xref ref-type="bibr" rid="scirp.31234-ref15">15</xref>]. It becomes obvious that for mean electron energies <img src="6-5300411\c174163e-8820-4a8f-bf61-45fae0944499.jpg" /> the distribution anisotropy <img src="6-5300411\cfe60c56-930c-4ac7-9df1-51829636f8f9.jpg" /> becomes important and should not be neglected by using the conventional two-term approximation.</p><p>The derived drift-diffusion approximation (18) can be used for description of electron transport instead of the conventional drift-diffusion approximation DDAc</p><disp-formula id="scirp.31234-formula123362"><label>(19a)</label><graphic position="anchor" xlink:href="6-5300411\baa978e9-f0ee-4e12-9413-6e6820a3608c.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.31234-formula123363"><label>(19b)</label><graphic position="anchor" xlink:href="6-5300411\7dafb9bc-21fd-4cdd-bd29-ad7faf51c33e.jpg"  xlink:type="simple"/></disp-formula><p>which is deduced from Equation (7) with [<xref ref-type="bibr" rid="scirp.31234-ref16">16</xref>] and without [8,40,41] consideration of the higher order contribution <img src="6-5300411\f7d6239a-2034-4999-b0e2-e6158be982bf.jpg" /> to the distribution anisotropy. The electron diffusion coefficients of particle <img src="6-5300411\bb6472bc-1317-4c42-86b3-9d0cc2c136af.jpg" /> and energy <img src="6-5300411\acc01835-d4d1-4016-949b-6412933d9f1b.jpg" /> transport as well as the electron mobilities of particles <img src="6-5300411\6b6bca7c-d92a-48f5-b143-2dea3a350782.jpg" /> and energy <img src="6-5300411\9cff8819-3442-4e21-b199-f57ec7323e7b.jpg" /> are determined in the same way as the coefficients of the four-moment model (15) and (17) as functions of the mean electron energy [<xref ref-type="bibr" rid="scirp.31234-ref16">16</xref>].</p></sec><sec id="s3_3"><title>3.3. Conventional Three-Moment Model</title><p>The derivation of the four-moment model 4MM and the</p><p>drift-diffusion model DDAn is consistent in the sense that beside the truncation of the expansion (3) no additional assumptions are needed in order to close the system of macroscopic moment equations. This is not the case if moment equations are derived directly from the electron Boltzmann Equation (4) and not from the kinetic system (6), see, e.g., [13,42,43]. The multiplication of Equation (4) by factors 1, <img src="6-5300411\e816b8ee-c059-4fe9-b16c-3eeed33af643.jpg" />and<img src="6-5300411\b07e62ae-e35f-482d-8070-7d2acff7ec4d.jpg" />, respectively, and subsequent integration over velocity space yields the system of three moment equations [<xref ref-type="bibr" rid="scirp.31234-ref44">44</xref>]</p><disp-formula id="scirp.31234-formula123364"><label>(20a)</label><graphic position="anchor" xlink:href="6-5300411\799caef3-05b0-43f6-8f9f-3508bf2fc7aa.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.31234-formula123365"><label>(20b)</label><graphic position="anchor" xlink:href="6-5300411\01a7b8bd-2e5d-4a53-aaa9-b50023c74e74.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.31234-formula123366"><label>(20c)</label><graphic position="anchor" xlink:href="6-5300411\b2a9c8d9-e4a7-41f2-803e-b932fdd3565c.jpg"  xlink:type="simple"/></disp-formula><p>for the particle density<img src="6-5300411\46369f6d-d9a6-4cf7-91a9-842aa297dc3e.jpg" />, the particle flux <img src="6-5300411\ab4a5f51-0784-43e1-84df-3b01296962fb.jpg" /> and the energy density <img src="6-5300411\4a633b34-4fff-4758-9a82-218603a06b01.jpg" /> of electrons. In order to solve system (20) it has to be closed by certain expressions for the electron pressure tensor</p><disp-formula id="scirp.31234-formula123367"><label>(21)</label><graphic position="anchor" xlink:href="6-5300411\71105dbf-5c63-4c87-bd72-47d23fa27ca7.jpg"  xlink:type="simple"/></disp-formula><p>with <img src="6-5300411\11d37853-dc90-4247-8e14-bf72672177c1.jpg" /> and the random electron velocity <img src="6-5300411\b1a7c63f-365b-47aa-bdd5-5f246c704e76.jpg" /> as well as for the electron energy flux</p><disp-formula id="scirp.31234-formula123368"><label>(22)</label><graphic position="anchor" xlink:href="6-5300411\47fc5809-e775-4efb-a22e-5aef4b29e5b0.jpg"  xlink:type="simple"/></disp-formula><p>For light particles such as electrons, the pressure tensor <img src="6-5300411\1057864d-931b-4c8a-85b3-3a0d1902e9bd.jpg" /> can be simplified to the scalar electron pressure [45,46]</p><disp-formula id="scirp.31234-formula123369"><label>(23)</label><graphic position="anchor" xlink:href="6-5300411\8f9ecaf8-fa22-4ddf-9ad2-4e7a48e454d7.jpg"  xlink:type="simple"/></disp-formula><p>and is therefore determined in terms of the macroscopic quantities<img src="6-5300411\ea4b214a-dfbf-4ff3-84ba-196cb543f252.jpg" />, <img src="6-5300411\06c97f14-5ab0-4a7f-9247-0fe5550eeab0.jpg" />and<img src="6-5300411\f25d678a-8786-4a86-9f2c-6ebe17b495bb.jpg" />. The derivation of an adequate expression for the third order moment <img src="6-5300411\7a2ca97e-a60c-481b-9b74-7867c426a664.jpg" /> in terms of lower order moments is a much more difficult task. Most often, the electron energy flux is rewritten as [<xref ref-type="bibr" rid="scirp.31234-ref44">44</xref>]</p><disp-formula id="scirp.31234-formula123370"><label>(24)</label><graphic position="anchor" xlink:href="6-5300411\2bfd7948-653f-49d9-b957-8c77d162183f.jpg"  xlink:type="simple"/></disp-formula><p>with the exact electron heat flux</p><disp-formula id="scirp.31234-formula123371"><label>(25)</label><graphic position="anchor" xlink:href="6-5300411\911f9dd4-38a4-458a-b8c0-ca2b382857b6.jpg"  xlink:type="simple"/></disp-formula><p>and then the heat flux is approximated by Fourier heat conduction according to [12,13]</p><disp-formula id="scirp.31234-formula123372"><label>(26)</label><graphic position="anchor" xlink:href="6-5300411\4915dbc3-6b61-486f-a7bf-73a2d308f64a.jpg"  xlink:type="simple"/></disp-formula><p>However, this approximation is known to be inaccurate in most discharge situations [22,43].</p><p>A more sophisticated heat flux ansatz has been derived by Robson et al. [<xref ref-type="bibr" rid="scirp.31234-ref22">22</xref>]. Unfortunately, their heat flux expression depends on parameters which are not known for real gases and is therefore not applicable without further benchmark calculations [<xref ref-type="bibr" rid="scirp.31234-ref23">23</xref>].</p></sec></sec><sec id="s4"><title>4. Comparison of Macroscopic and Kinetic Models</title><p>In order to show that the derived systems of partial differential equations 4MM and DDAn improve the accuracy of fluid models for the description of electrons, numerical calculations for two different discharge situations in argon were performed. First, the electron transport equations were solved for prescribed pulse-like electric field (benchmark model). Secondly, an abnormal glow discharge in low pressure argon was described selfconsistently in the sense that the electron transport equations were solved together with transport equations for heavy particles and Poisson’s equation for determination of the electric field. The finite-difference methods used to discretize the system of differential equations in space and time are detailed in reference [<xref ref-type="bibr" rid="scirp.31234-ref15">15</xref>].</p><sec id="s4_1"><title>4.1. Argon Benchmark Model</title><p>Probe measurements in plasmas cause an abrupt change of the local electric field. This situation is considered here, and the four-moment model 4MM (16) as well as the drift-diffusion model DDAn using the new flux representation (18) and the drift-diffusion model DDAc using the conventional flux representation (19) were solved for argon gas at a pressure of 133 Pa and a gas temperature of 300 K using the prescribed electric field profile shown in <xref ref-type="fig" rid="fig3">Figure 3</xref>(a). In order to rate the results of 4MM, DDAn and DDAc, the space-dependent electron Boltzmann equation was solved kinetically according to Sigeneger et al. [<xref ref-type="bibr" rid="scirp.31234-ref41">41</xref>] for the same electric field, taking into account elastic and inelastic electron collision processes. Figures 3(b) and 3(c) exhibit the results obtained for the mean velocity and the mean energy of the electrons by means of the different models.</p><p>Because the applied field is time-independent and therefore the temporal derivatives of all quantities are zero, results of 4MM and DDAn are almost the same. The spatial profile predicted by the models 4MM and DDAn for the mean velocity and the mean energy are in qualitative agreement with the kinetic results. In contrast,</p><p>the results of DDAc strongly differ from those of the kinetic solution. The results show impressively that the accuracy of fluid models for the theoretical description of electrons is strongly increased by the proposed methods.</p></sec><sec id="s4_2"><title>4.2. Abnormal Glow Discharge in Argon</title><p>To demonstrate the practical applicability of the derived moment equations, the ignition of an abnormal glow discharge in argon at a gas pressure of 133 Pa and a gas temperature of 300 K was theoretically described using the discharge geometry depicted in <xref ref-type="fig" rid="fig1">Figure 1</xref>. At the powered electrode at <img src="6-5300411\82abb6ff-ebdf-4501-bcf7-167d81a7bd98.jpg" /> (cathode) a voltage of –250 W was applied and the electrode at x = 1 cm (anode) was grounded. The general procedure for solving the coupled system of transport equations for the species and Poisson’s equation has been described in [<xref ref-type="bibr" rid="scirp.31234-ref15">15</xref>] and the data used for the electron-atom collisions are the same as those reported in this paper.</p><p>The results obtained by the models 4MM, DDAn and DDAc for the mean electron velocity, the mean electron energy and the self-consistently determined electric field are shown in <xref ref-type="fig" rid="fig4">Figure 4</xref> at three different instants of time. Obviously, all fluid models under consideration predict qualitatively the same dynamic behaviour. Shortly after switching on the discharge, at t = 1 μs, a quasi-stationary Townsend phase is reached which is characterized by an almost constant electric field and small spatial variations in the mean velocity and mean energy of electrons.</p><p>Charge carriers are produced mainly in front of the grounded electrode by ionization of argon atoms in collisions with electrons and by secondary electron emission at the powered electrode due to ion bombardment. At <img src="6-5300411\4ecbdc6a-7ce2-4da8-a06c-87ef94ab7a6c.jpg" /> enough charge carriers are produced to distinctly perturb the homogeneous electric field. Due to the increase of the electric field in the cathode region strong charge carrier multiplication takes place and finally the discharge ignites. The discharge becomes stationary after approximately 100 μs. Electrons emitted at the cathode gain energy in the strong electric field and are then slowed down in electron collisions. The discharge is brightest in the negative glow region at approximately<img src="6-5300411\84bbbda5-3881-4896-8286-82fb2cb1c811.jpg" />.</p><p>Because the characteristic frequency for the field alteration is small in the discharge situation considered here, the results of the four-moment model 4MM and the new drift-diffusion model DDAn are almost the same. Small differences occur in front of the boundaries due to the fact that different types of boundary conditions have to be applied for the system of first-order differential equations 4MM and the parabolic system DDAn. Again, the results of DDAc differ markedly. Particularly in the transition from the cathode region to the negative glow at <img src="6-5300411\0a7ac5f5-136f-487f-9bec-62019b289797.jpg" /> strong deviations in the results for the mean energy occur at steady state. The mean energy minimum is strongly overestimated by DDAc and it has been found that this issue causes the occurrence of a singular point in the temporal evolution of the discharge ignition if gas pressure, discharge chemistry or applied voltage are slightly changed.</p></sec></sec><sec id="s5"><title>5. Conclusions</title><p>A new system of moment equations for the description of electrons in nonthermal plasmas was derived by an expansion of the electron velocity distribution function in Legendre polynomials and the definition of transport coefficients that are determined by means of the localmean-energy approximation. The new model 4MM is consistent in the sense that no additional assumptions are necessary to close the system of moment equations. It has been shown that the additional requirement of a small characteristic frequency for the field alteration allows to reduce the system of four first-order partial differential equations for particle density, particle flux, energy density and energy flux of electrons to a parabolic driftdiffusion model comprising two second-order partial differential equations for the particle density and energy density of electrons. If this requirement is fulfilled, the results provided by the new drift-diffusion model DDAn are in good agreement with those of the high order fluid model 4MM.</p><p>The comparison of results obtained by the models 4MM and DDAn with results of the conventional driftdiffusion model DDAc as well as kinetically obtained results has pointed out that the new approach strongly increases the accuracy of fluid models for the description of electron transport in nonthermal plasmas. Since similar partial differential equations for electrons arise in the theoretical description of semiconductors [47-49], it potentially improves the theoretical description of electrons in semiconductor devices, too.</p></sec><sec id="s6"><title>6. Acknowledgments</title><p>This work was supported by the German Research Foundation within the Collaborative Research Centre Transregio 24.</p></sec><sec id="s7"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.31234-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">B. Eliasson, M. Hirth and U. Kogelschatz, “Ozone Synthesis from Oxygen in Dielectric Barrier Discharges,” Journal of Physics D: Applied Physics, Vol. 20, No. 11, 1987, pp. 1421-1437. doi:10.1088/0022-3727/20/11/010</mixed-citation></ref><ref id="scirp.31234-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">U. 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