<?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">JMP</journal-id><journal-title-group><journal-title>Journal of Modern Physics</journal-title></journal-title-group><issn pub-type="epub">2153-1196</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jmp.2016.714167</article-id><article-id pub-id-type="publisher-id">JMP-71312</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>
 
 
  Linear and Nonlinear Electron Beam Heating of Magnetized, Motional, and Dusty Plasma
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sherif</surname><given-names>Mohamed Khalil</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Badriah</surname><given-names>Mesfer AL Alotaibi</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Physics Department, Faculty of Science, Princess Nora Bint Abdurrahman University, Riyadh, KSA</addr-line></aff><aff id="aff1"><addr-line>Plasma Physics &amp;amp; Nuclear Fusion Department, N.R.C., Atomic Energy Authority, Cairo, Egypt</addr-line></aff><pub-date pub-type="epub"><day>17</day><month>10</month><year>2016</year></pub-date><volume>07</volume><issue>14</issue><fpage>1889</fpage><lpage>1900</lpage><history><date date-type="received"><day>September</day>	<month>1,</month>	<year>2016</year></date><date date-type="rev-recd"><day>Accepted:</day>	<month>October</month>	<year>15,</year>	</date><date date-type="accepted"><day>October</day>	<month>19,</month>	<year>2016</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><html>
 <head></head>
 
  Recent theoretical work on electron beam heating of magneto-active motional Plasma is presented. Power transfer from beam (plasma heating) and generated electric fields for different physical situations of linear and nonlinear beam-plasma interaction, are studied. Based on previous works [1] [2], we shall study the effects of dusts and plasma motion (
  <img src="Edit_48772777-4799-4ae1-8466-134a26237eff.bmp" alt="" />) on plasma heating. Besides, the case of an inhomogeneity of beam velocity (
  <img src="Edit_48e58362-f86d-47c8-8262-7f4282942317.bmp" alt="" />) is also considered. Taking into consideration nonlinear process, dust, plasma motion, and beam velocity inhomogeneity, are found to play a crucial role via power absorbed by the beam and the generated electric field in the system.
 
</html></p></abstract><kwd-group><kwd>Beam-Plasma Interaction</kwd><kwd> Motional Plasma</kwd><kwd> Dusty Plasmas</kwd><kwd> Plasma Heating</kwd><kwd>  Electric Field Generation</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Electron beam-plasma interaction presents a great interest for many applications in areas like development of new methods in amplification and generation of electromagnetic waves, acceleration of charged particles in plasma (Plasma Accelerator). Besides, the electron beam-plasma system showed great importance via plasma generation, design of microwave tubes waveguides, explanation of natural phenomena that occur in space and solar plasmas, material studies, compact torus formation, generation of x-ray and microwave, and others.</p><p>The recent development in the electron beam technology has shown the capability of generating powerful electron energy sources, making the electron beam very useful to controlled thermonuclear fusion research or in general, to plasma heating. Besides, the electron beam provides a free energy source for a rich variety of nonlinear process to evolve in a plasma. Accordingly, It is not surprising to find up till now a long list of studies and research on beam-plasma interaction and applications, which was also reviewed by many authors, (e.g., see [<xref ref-type="bibr" rid="scirp.71312-ref1">1</xref>] - [<xref ref-type="bibr" rid="scirp.71312-ref8">8</xref>] and references therein).</p><p>Multiple harmonic generation by laser/beam-plasma interaction has been widely investigated [<xref ref-type="bibr" rid="scirp.71312-ref9">9</xref>] - [<xref ref-type="bibr" rid="scirp.71312-ref13">13</xref>] . The generation of harmonics through a nonlinear mechanism driven by bunching at the fundamental has sparked interest as a path toward enhancing and extending the usefulness of an x-ray free-electron laser (FEL) facility. Besides, the sensitivity of nonlinear harmonic generation to electron beam quality is found to play a crucial role via FEL [<xref ref-type="bibr" rid="scirp.71312-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.71312-ref15">15</xref>] .</p><p>Currently, high-order harmonic generation (HHG) is considered as one of the more efficient technique for producing coherent short-wavelength radiation in a broad spectral range [<xref ref-type="bibr" rid="scirp.71312-ref16">16</xref>] . Also, the nonlinear cold plasma-bunched beam interaction represents an interesting application for plasma wakefield accelerator [<xref ref-type="bibr" rid="scirp.71312-ref17">17</xref>] .</p><p>From the point of view of beam-plasma interaction, the impact of dust on plasma is an important explosed field of research. It is increasingly being studied these days due to their applications in a wide range of fields. The presence of relatively highly charged and massive dust grains in a plasma can modify or influence the collective phenomena of the plasma. The possible dust modes may explain the extremely low-frequency fluctuations, new channels for the parametric coupling of other waves, generation of wakefields, etc., in dusty plasma. The impurities coming off from the walls of fusion device can create a dusty plasma at the edge of the discharge. These particles can enhance power loss due to radiation and dilution of fuel as well as can cool down the hot ion by charge-exchange process [<xref ref-type="bibr" rid="scirp.71312-ref18">18</xref>] - [<xref ref-type="bibr" rid="scirp.71312-ref23">23</xref>] .</p><p>The subject of this paper is to study and investigate the electron beam heating of magneto-active motional dusty plasma under discuss different effects or parameters.</p><p>Section 2 explores the interaction of electron beam with a homogeneous magnetized non-motional plasma and plasma heating. Section 3 studies linear, non-motional (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x4.png" xlink:type="simple"/></inline-formula>) and clean plasma in static magnetic field, while Section 4 is devoted to study the effects of the dust on the nonlinear beam interaction with non-motional plasma. Dusty plasma is characterized as a low-temperature ionized gas whose constituents are electrons, ions, and micron-sized dust particulates. The latter is usually negatively charged due to the attachment of the background plasma electrons on the surface of dust grains via collisions. The physical processes in dusty plasmas are interesting because of their importance for a number of applications in space plasmas and the earth s environment, as well as in the laboratory, and in several technologies. The dust grains have a strong effect on energy absorbed in the plasma. In Section 5, we study and investigates the effects of motional plasma (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x5.png" xlink:type="simple"/></inline-formula>) on the heating processes due to beam-plasma interaction. Finally, in Section 6, we investigate the effects due to the inhomogeneity of beam velocity on both power absorption and generated electric field.</p><p>The electron beam is considered to be injected into plasma under the effect of static magnetic field<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x6.png" xlink:type="simple"/></inline-formula>. We use the well known expression for the amount of energy absorbed by the plasma per unit time S as:</p><disp-formula id="scirp.71312-formula117"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x7.png"  xlink:type="simple"/></disp-formula><p>where E is the electric field generated in the system.</p></sec><sec id="s2"><title>2. Linear, Non-Motional and Clean Plasma in Static Magnetic Field</title><p>The equations of motion, and the continuity equation for electron beam, which travels along the magnetic field are:</p><disp-formula id="scirp.71312-formula118"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x8.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71312-formula119"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x9.png"  xlink:type="simple"/></disp-formula><p>while the equation of motion, and the continuity equation for cold inhomogeneous plasma electrons in the static magnetic field are given by:</p><disp-formula id="scirp.71312-formula120"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x10.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71312-formula121"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x11.png"  xlink:type="simple"/></disp-formula><p>where, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x12.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x13.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x14.png" xlink:type="simple"/></inline-formula>.</p><p>For non motional plasma<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x15.png" xlink:type="simple"/></inline-formula>. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x16.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x17.png" xlink:type="simple"/></inline-formula> are the unperturbed velocity and density of the beam and plasma respectively.</p><p>Solving the above system of equations we can derive the following expressions for the perturbed densities:</p><disp-formula id="scirp.71312-formula122"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x18.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71312-formula123"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x19.png"  xlink:type="simple"/></disp-formula><p>where, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x20.png" xlink:type="simple"/></inline-formula>, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x21.png" xlink:type="simple"/></inline-formula> is the cyclotron frequency.</p><p>Using relations (6) and (7) in Poisson’s equation</p><disp-formula id="scirp.71312-formula124"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x22.png"  xlink:type="simple"/></disp-formula><p>we obtain the following wave equation for the electric field:</p><disp-formula id="scirp.71312-formula125"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x23.png"  xlink:type="simple"/></disp-formula><p>where, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x24.png" xlink:type="simple"/></inline-formula></p><p>Introducing the electric field form:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x25.png" xlink:type="simple"/></inline-formula>, Equation (9) reduces to:</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x26.png" xlink:type="simple"/></inline-formula>, where,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x27.png" xlink:type="simple"/></inline-formula> (10)</p><p>Then we can write the final solution of (9) in the simple form:</p><disp-formula id="scirp.71312-formula126"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x28.png"  xlink:type="simple"/></disp-formula><p>Set (11) into (1), the energy absorbed absorbed by the beam reads:</p><disp-formula id="scirp.71312-formula127"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x29.png"  xlink:type="simple"/></disp-formula><p>Relation (12) is investigated for different cases of magnetic field: zero, weak and strong magnetic fields.</p></sec><sec id="s3"><title>3. Linear Dusty Plasma Heating</title><p>For dusty plasma, we use the system of Equations (2)-(5) with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x30.png" xlink:type="simple"/></inline-formula>, then we obtain the following equation of motion, and the continuity equation as:</p><disp-formula id="scirp.71312-formula128"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x31.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71312-formula129"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x32.png"  xlink:type="simple"/></disp-formula><p>Solving the above system of equations we can derive the following expressions for the dust perturbed density:</p><disp-formula id="scirp.71312-formula130"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x33.png"  xlink:type="simple"/></disp-formula><p>where, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x34.png" xlink:type="simple"/></inline-formula>Charge of dust.</p><p>Using relations (7) and (8), (15) in Poisson’s equation:</p><disp-formula id="scirp.71312-formula131"><label>(16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x35.png"  xlink:type="simple"/></disp-formula><p>we obtain the following wave equation for the perturbed electric field:</p><disp-formula id="scirp.71312-formula132"><label>(17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x36.png"  xlink:type="simple"/></disp-formula><p>where, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x37.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x38.png" xlink:type="simple"/></inline-formula>.</p><p>The energy absorbed in this case reads:</p><p><img data-original="http://html.scirp.org/file/4-7502904x39.png" />,<img data-original="http://html.scirp.org/file/4-7502904x40.png" /> (18)</p><p>In linear regime, if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x41.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x42.png" xlink:type="simple"/></inline-formula> are the energy absorbed by the beam in clean and in dusty plasma, respectively, then:</p><disp-formula id="scirp.71312-formula133"><graphic  xlink:href="http://html.scirp.org/file/4-7502904x43.png"  xlink:type="simple"/></disp-formula><p>It is clear that, existence of dust leads to less energy absorption by the plasma.</p><p>The generated electric field under the effect of dusty and clean plasma is shown in <xref ref-type="fig" rid="fig3">Figure 3</xref>.</p></sec><sec id="s4"><title>4. Nonlinear Dusty Plasma Heating</title><p>In nonlinear regime, the equation of motion, and the continuity equation for electron beam, which travels along the magnetic field are:</p><disp-formula id="scirp.71312-formula134"><label>(19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x44.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71312-formula135"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x45.png"  xlink:type="simple"/></disp-formula><p>The equation of motion, and the continuity equation for homogeneous plasma electrons in a static magnetic field perpendicular to the plasma are given by:</p><disp-formula id="scirp.71312-formula136"><label>(21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x46.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71312-formula137"><label>(22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x47.png"  xlink:type="simple"/></disp-formula><p>The dusty nonlinear equations of motion, and continuity are:</p><disp-formula id="scirp.71312-formula138"><label>(23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x48.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71312-formula139"><label>(24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x49.png"  xlink:type="simple"/></disp-formula><p>Solving the above system of equations we can derive the following expressions for the nonlinear perturbed densities:</p><disp-formula id="scirp.71312-formula140"><label>(25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x50.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71312-formula141"><label>(26)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x51.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71312-formula142"><label>(27)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x52.png"  xlink:type="simple"/></disp-formula><p>where, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x53.png" xlink:type="simple"/></inline-formula>(second harmonic generation), and</p><disp-formula id="scirp.71312-formula143"><graphic  xlink:href="http://html.scirp.org/file/4-7502904x54.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71312-formula144"><graphic  xlink:href="http://html.scirp.org/file/4-7502904x55.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71312-formula145"><graphic  xlink:href="http://html.scirp.org/file/4-7502904x56.png"  xlink:type="simple"/></disp-formula><p>Using relations (25)-(27), and considering the nonlinear form of Poisson’s Equation (16), we obtain the following wave equation for the nonlinear generated electric field:</p><disp-formula id="scirp.71312-formula146"><label>(28)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x57.png"  xlink:type="simple"/></disp-formula><p>where, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x58.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x58.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x59.png" xlink:type="simple"/></inline-formula>.</p><p>Accordingly, we obtain the energy absorption from the beam as:</p><p><img data-original="http://html.scirp.org/file/4-7502904x60.png" />,<img data-original="http://html.scirp.org/file/4-7502904x61.png" /> (29)</p><p>From (18) and (29) we conclude that:</p><disp-formula id="scirp.71312-formula147"><label>(30)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x62.png"  xlink:type="simple"/></disp-formula><p>Ratio (30) shows that, for nonlinear interaction the existence of dust leads to less energy absorption by the plasma as in the linear regime.</p><p><xref ref-type="fig" rid="fig4">Figure 4</xref> shows the generated electric field under the effect of dusty and clean nonlinear plasma. In this regime amplification of electric field in dusty plasma is clear compared to clean plasma.</p><p>Generally speaking, nonlinearity plays a crucial role in the amplification of the electric field generated due to beam-plasma interaction, for different situations, compared to linear case.</p></sec><sec id="s5"><title>5. Motional Plasma</title><p>For motional plasma, for the electron beam, we use the above system of Equations (2), (3 and (6). On the other hand, the equation of motion, and the continuity equation for homogeneous plasma electrons in a static magnetic field perpendicular to the plasma are given by:</p><disp-formula id="scirp.71312-formula148"><label>(31)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x63.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71312-formula149"><label>(32)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x64.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71312-formula150"><label>(33)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x65.png"  xlink:type="simple"/></disp-formula><p>Accordingly, we obtain the following expressions for the perturbed plasma density</p><disp-formula id="scirp.71312-formula151"><label>(34)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x66.png"  xlink:type="simple"/></disp-formula><p>Using relations (6) and (34) in Poisson’s Equation (8), we obtain the following wave equation for the electric field in motional plasma</p><disp-formula id="scirp.71312-formula152"><label>(35)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x67.png"  xlink:type="simple"/></disp-formula><p>where,</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x68.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x68.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x69.png" xlink:type="simple"/></inline-formula>,</p><p>In this case the energy absorbed is:</p><disp-formula id="scirp.71312-formula153"><label>(36)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x70.png"  xlink:type="simple"/></disp-formula><p>From this relation and non-motional relation (12) we conclude that:</p><disp-formula id="scirp.71312-formula154"><label>(37)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x71.png"  xlink:type="simple"/></disp-formula><p>Ratio (37) shows that, the existence of plasma motion leads to less energy absorption from the beam, as indicated in <xref ref-type="fig" rid="fig6">Figure 6</xref>.</p><p><xref ref-type="fig" rid="fig7">Figure 7</xref> shows the reduction of the generated electric field under the effect of motional plasma compared to non-motional plasma.</p></sec><sec id="s6"><title>6. Inhomogeneity of Beam Velocity Effects</title><p>Let us consider the case of an electron beam moves with inhomogeneous velocity, i.e.,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x72.png" xlink:type="simple"/></inline-formula>. In this case we have to include the term <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x73.png" xlink:type="simple"/></inline-formula> in both the equations of</p><p>motion (2) and continuity. Accordingly, we obtain the perturbed beam velocity and density as:</p><disp-formula id="scirp.71312-formula155"><label>(38)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x74.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71312-formula156"><label>(39)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x75.png"  xlink:type="simple"/></disp-formula><p>where, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x76.png" xlink:type="simple"/></inline-formula>, and the equation controlling the perturbed electric field is given by:</p><p><img data-original="http://html.scirp.org/file/4-7502904x77.png" />,<img data-original="http://html.scirp.org/file/4-7502904x78.png" /> (40)</p><p>Using mathematical tools used in previous sections, we obtain, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x79.png" xlink:type="simple"/></inline-formula>, hence the energy absorbed in this case:</p><disp-formula id="scirp.71312-formula157"><label>(41)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7502904x80.png"  xlink:type="simple"/></disp-formula><p><xref ref-type="fig" rid="fig8">Figure 8</xref> shows that the sharp increase in the generated electric field due to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x81.png" xlink:type="simple"/></inline-formula>―after a critical distance in the plasma―compared to the case<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x82.png" xlink:type="simple"/></inline-formula>. This positively affects the plasma heating, and creates a type of plasma acceleration.</p></sec><sec id="s7"><title>7. Conclusions and Final Remarks</title><p>The Electron Beam Heating of Magneto-Active Motional Dusty Plasma is investigated.</p><p>Generally speaking, nonlinear process, dust, plasma motion, and beam velocity inhomogeneity, are found to play a crucial role via power absorbed by the beam and the generated electric field in the system.</p><p>It is shown that strong magnetic field generates an intense electric field compared to zero, and weak magnetic fields (<xref ref-type="fig" rid="fig1">Figure 1</xref>). In turn, an applied external static magnetic field leads to enhanced power absorption from the electron beam, and accordingly to plasma heating in beam-plasma system.</p><p>The energy absorbed from the beam in clean (S) and dusty (S<sub>d</sub>) plasma (<xref ref-type="fig" rid="fig2">Figure 2</xref>), shows that dust causes a loss in the power energy absorbed in the plasma.</p><p>Considering nonlinear interaction, ratio (30) shows that dust leads to less energy absorption by the plasma as in the linear regime.</p><p><xref ref-type="fig" rid="fig3">Figure 3</xref> and <xref ref-type="fig" rid="fig4">Figure 4</xref>, shows the generated electric field under the effect of dusty and non-dusty plasmas in linear and nonlinear stages. In this regime amplification of electric field in dusty plasma is less compared to clean plasma. However, in clean plasms, the nonlinear effects associated with the generation of second harmonics, plays an important role in the process of energy transfer from the beam to the plasma as</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Generated electric field under the effect of zero, weak and strong magnetic fields</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-7502904x83.png"/></fig><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Energy absorbed from the beam in clean (S) and dusty (S<sub>d</sub>) plasmas</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-7502904x84.png"/></fig><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Generated electric field under the effect of dusty and clean linear plasma</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-7502904x85.png"/></fig><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Generated electric field under the effect of dusty and clean nonlinear plasma</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-7502904x86.png"/></fig><p>compared with linear stage. This is due to the fact that the electric field intensity at double harmonics is stronger than that of the basic frequency (<xref ref-type="fig" rid="fig5">Figure 5</xref> shows electric field amplification in nonlinear regime).</p><p>As application, the generation of second harmonics through a nonlinear mechanism driven by bunching at the fundamental has sparked interest as a path toward enhancing and extending the usefulness of an x-ray free-electron laser (FEL) facility [<xref ref-type="bibr" rid="scirp.71312-ref14">14</xref>] . Currently, high-order harmonic generation (HHG) is considered as one of the more efficient technique for producing coherent short-wavelength radiation in a broad spectral range [<xref ref-type="bibr" rid="scirp.71312-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.71312-ref24">24</xref>] [<xref ref-type="bibr" rid="scirp.71312-ref25">25</xref>] .</p><p>In the motional plasma, the interaction between the electron beam and plasma will occur and induce electrons to exchange energy with plasma waves. The self-magnetic field of the motional electrons is a key parameter of this interaction.</p><p>Ratio (37) shows that, the existence of plasma motion leads to less energy absorption of the beam, as indicated in <xref ref-type="fig" rid="fig6">Figure 6</xref>. The reduction of the generated electric field under the effect of motional plasma compared to non-motional plasma, is shown in <xref ref-type="fig" rid="fig7">Figure 7</xref>.</p><p>An interesting result is shown in <xref ref-type="fig" rid="fig8">Figure 8</xref>, the sharp increase in the generated electric field due to beam velocity inhomogeneity<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x87.png" xlink:type="simple"/></inline-formula>―after a critical distance in the plasm compared to the case<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7502904x88.png" xlink:type="simple"/></inline-formula>. This enhanced power absorption of the electron</p><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> Electric field amplification in the nonlinear regime</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-7502904x89.png"/></fig><fig id="fig6"  position="float"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title> Energy absorbed from the beam in non-motional (S) and motional (S<sub>mot.</sub>) plasmas</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-7502904x90.png"/></fig><fig id="fig7"  position="float"><label><xref ref-type="fig" rid="fig7">Figure 7</xref></label><caption><title> Generated electric field under the effect of motional and nonmotional plasma</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-7502904x91.png"/></fig><fig id="fig8"  position="float"><label><xref ref-type="fig" rid="fig8">Figure 8</xref></label><caption><title> Generated electric field under the effect of inhomogeneous and homogeneous beam velocity</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-7502904x92.png"/></fig><p>beam, and positively affects the plasma heating, and may create a type of plasma acceleration.</p><p>In due course, we are going to investigate the effects of an inhomogeneous relativistic electron beam (REB) interaction with dusty, motional inhomogeneous plasma placed in an oscillating magnetic field.</p></sec><sec id="s8"><title>Cite this paper</title><p>Khalil, Sh.M. and AL Alotaibi, B.M. (2016) Linear and Nonlinear Electron Beam Heating of Magnetized, Motional, and Dusty Plasma. Journal of Mo- dern Physics, 7, 1889-1900. http://dx.doi.org/10.4236/jmp.2016.714167</p></sec></body><back><ref-list><title>References</title><ref id="scirp.71312-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Khalil, Sh.M. and Al-Enazi, M.M. (2009) Advanced Studies in Theoretical Physics, 3, 369. http://www.m-hikari.com/astp/astp2009/astp9-12-2009/index.html</mixed-citation></ref><ref id="scirp.71312-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Khalil, Sh.M. and Al-Enazi, M.M. (2010) Journal of Modern Physics, 2, 79. http://dx.doi.org/10.4236/jmp.2011.22013</mixed-citation></ref><ref id="scirp.71312-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Karlicky, M. 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