<?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.2013.42033</article-id><article-id pub-id-type="publisher-id">JMP-28324</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>
 
 
  The Propagation of Circularly Polarized Waves in Quantum Plasma
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>ahaa</surname><given-names>F. Mohamed</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>Rehab</surname><given-names>Albrulosy</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Plasma Physics Department, N.R.C., Atomic Energy Authority, Cairo, Egypt</addr-line></aff><aff id="aff2"><addr-line>Physics Department, Faculty of Science, Banha University, Banha, Egypt</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>mohamedbahf@yahoo.co.uk(AFM)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>05</day><month>02</month><year>2013</year></pub-date><volume>04</volume><issue>02</issue><fpage>236</fpage><lpage>239</lpage><history><date date-type="received"><day>September</day>	<month>2,</month>	<year>2012</year></date><date date-type="rev-recd"><day>November</day>	<month>1,</month>	<year>2012</year>	</date><date date-type="accepted"><day>November</day>	<month>28,</month>	<year>2012</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 quantum effects on the propagation circularly polarized waves have been investigated in electron magnetized quantum plasmas. We obtain the dispersion equations of the propagation of circularly polarized laser beam through cold plasma. The results show that the laser can be propagated due to the quantum effects which enhance the propagation phase velocity. For this purpose, the quantum hydrodynamic (QHD) equations with magnetic field and Maxwell’s equations system is used to derive these dispersion relations. The perturbed electron density and current due to the interaction of laser beam with quantum plasma have been investigated. It is shown that the external magnetic field which is parallel to the propagation waves has strong effect on the dispersion relation for the laser propagation in quantum model than the classical regime. 
 
</p></abstract><kwd-group><kwd>Dense Quantum Plasma; Laser Plasma Interaction; Quantum Effects</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The classical plasmas, in general, are characterized by high temperature and low density regimes where quantum effects are negligible. However, there are examples in nature where both plasma and quantum effect can coexist. In such situations, quantum effects are expected to play a significant role on the dynamics of plasma particles.</p><p>The quantum plasma has received much attention in recent years due to its important applications in ultrasmall electronics devices [<xref ref-type="bibr" rid="scirp.28324-ref1">1</xref>], quantum dots and quantum wire [<xref ref-type="bibr" rid="scirp.28324-ref2">2</xref>], in dense astrophysical plasma system [3,4] as well as in laser-produced plasma [<xref ref-type="bibr" rid="scirp.28324-ref5">5</xref>] and nonlinear optics [<xref ref-type="bibr" rid="scirp.28324-ref6">6</xref>].</p><p>Two well-known models are used to study quantum plasmas systems. The first one is the Wigner model which describes the statistical behavior of plasmas based on the Wigner-Poisson system. The other is Hartree model which describes the hydrodynamic behavior of plasmas based on the Schrodinger-Poisson system [7,8]. The quantum hydrodynamic (QHD) model describes the transport of charge, momentum and energy in charged particle system interacting though a self-consistent electrostatic potential.</p><p>The quantum plasma effects become important in dense plasmas, when the de Broglie wavelength of the charge carriers becomes comparable to the spatial scale of plasma system. So, the new dispersion relationship with quantum effects corrections for some types of linear waves in a uniform cold quantum plasma with nonzero external magnetic field are calculated by Ren et al. [<xref ref-type="bibr" rid="scirp.28324-ref9">9</xref>]. Also, the dispersion relation for the propagation of linearly polarized laser beam through cold quantum plasma has been obtained by Kumar et al. [<xref ref-type="bibr" rid="scirp.28324-ref10">10</xref>] using perturbation techniques.</p><p>In addition, the surface plasma waves propagating along the plasma-vacuum interface has attracted much attention since the frequency spectra have wide applications in many areas such as laser physics, Plasma spectroscopy and plasma technology [<xref ref-type="bibr" rid="scirp.28324-ref11">11</xref>]. Lazer et al. [<xref ref-type="bibr" rid="scirp.28324-ref12">12</xref>] has presented the dispersion relation for surface plasmons that can exist on a dense quantum plasma halfspace. Also, the dispersion relations of one-, two-stream and beam-plasma instabilities in uniform quantum magnetized plasmas are investigated through the new dielectric tensor [<xref ref-type="bibr" rid="scirp.28324-ref13">13</xref>].</p><p>In the present paper, the quantum effects on the propagation circularly polarized waves have been investigated in electron quantum plasmas. We study the dispersion equations of its propagation through cold plasma under an external magnetic field based on the (QHD) model.</p></sec><sec id="s2"><title>2. Governing Equations</title><p>Considering a circularly polarized laser beam represented by the electric field</p><p><img src="13-7500970\1b01c9e7-3f20-4641-ae61-525415312cd4.jpg" /></p><p>and the magnetic field</p><p><img src="13-7500970\1d65598f-facd-4884-b0c8-f2565c24a7fc.jpg" /></p><p>propagates through the quantum electron plasma electrons.</p><p>We assume that the plasma is immersed in an ambient static magnetic field<img src="13-7500970\62387701-1a6e-4444-8d5d-9c74b099304c.jpg" />. From QHD model, the dynamics of the electrons are governed by the following continuity equation and the momentum equation:</p><disp-formula id="scirp.28324-formula33933"><label>(1)</label><graphic position="anchor" xlink:href="13-7500970\a78dcd64-389f-46fa-9766-440fe6cf2c26.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28324-formula33934"><label>(2)</label><graphic position="anchor" xlink:href="13-7500970\b5abadaa-04fd-4bd5-9e2a-7723f1984ede.jpg"  xlink:type="simple"/></disp-formula><p>Here n, u and m are the number density, the velocity and the mass of electron respectively and <img src="13-7500970\1f245ca8-9f0a-45a4-8a8c-51bfad3cb4b3.jpg" /> is the Plank’s constant divided by<img src="13-7500970\b57294b2-037e-49f0-a3b7-9b7a7d274a2a.jpg" />. The electrons obey the following pressure law which represents the equation of state in one-dimensional zero-temperature Fermi gas:</p><p><img src="13-7500970\ea76d189-adfc-4e98-8428-a90ec3843ba6.jpg" /></p><p>where <img src="13-7500970\40f28df3-b655-4e95-8710-1a6b569f47ad.jpg" /> is the Fermi thermal speed, <img src="13-7500970\eb9487f9-f079-42ed-9b6a-7caa2484e461.jpg" /></p><p>is the particle Fermi temperature, K<sub>B</sub> is the Boltzmann’s constant and <img src="13-7500970\640644f7-46ec-4c06-8d83-f52bc9a20eb5.jpg" /> is the equilibrium particle number density. We have included both the quantum statistical effects through Fermi temperature and the quantum diffraction in the <img src="13-7500970\28f16cdb-13eb-42ef-b2f8-381c6f9cc689.jpg" />-dependent. If we set <img src="13-7500970\0a49b762-55e3-43ca-90bc-6d9d66fe8053.jpg" /> equal to zero and <img src="13-7500970\3516b00f-cfe1-40cf-984b-a051f30674f5.jpg" /> equal the temperature of electrons, we obtain the classical hydrodynamic equation.</p><p>Using the perturbation technique, we assume any physical quantity <img src="13-7500970\c7145e47-872f-4b93-8726-343a73a95796.jpg" /> representing has the following form <img src="13-7500970\f97519b2-3293-41ca-af49-5386414cc7ed.jpg" /> where <img src="13-7500970\daaab8bf-9a97-4769-8ba4-6aae7f79799f.jpg" /> is the unperturbed value and <img src="13-7500970\51c67ca1-31a8-4f11-869e-44c1f7973b95.jpg" /> is a small perturbation<img src="13-7500970\ab7b0a8b-49c9-4587-a834-dd6c8add9111.jpg" />, we get:</p><disp-formula id="scirp.28324-formula33935"><label>(3)</label><graphic position="anchor" xlink:href="13-7500970\f6251aa4-192a-4870-a8d2-36caf37f7696.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28324-formula33936"><label>(4)</label><graphic position="anchor" xlink:href="13-7500970\8bce3ec5-1abf-41f1-9911-acbc41bfde6d.jpg"  xlink:type="simple"/></disp-formula><p>The last term in the Equation (4), which representing the Bohm potential, has been perturbatively expanded using [<xref ref-type="bibr" rid="scirp.28324-ref10">10</xref>]. The basic set of linearized equation in homogeneous quantum magnetized cold plasma is:</p><disp-formula id="scirp.28324-formula33937"><label>(5)</label><graphic position="anchor" xlink:href="13-7500970\2eda9288-e275-458f-a1ef-904fe246ccde.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28324-formula33938"><label>(6)</label><graphic position="anchor" xlink:href="13-7500970\2f1b4b5e-24cc-476f-9511-09d1591ec173.jpg"  xlink:type="simple"/></disp-formula><p>where,</p><p><img src="13-7500970\373e50ea-c681-47c3-a91b-43fca1882526.jpg" /></p><p>Taking into account Equation (6) and the expression of k, the following equation is derived:</p><disp-formula id="scirp.28324-formula33939"><label>(7)</label><graphic position="anchor" xlink:href="13-7500970\a13f9ca8-8fe5-4e10-8040-1759549c4bae.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="13-7500970\8bdc20ca-635b-4de7-b065-85f84b38881d.jpg" />, <img src="13-7500970\651018ba-b301-42a5-be39-0c136a6048b7.jpg" />When we have</p><p><img src="13-7500970\d818b6cd-2df7-4add-81d4-6279728ec910.jpg" />, <img src="13-7500970\a65b007c-d2aa-45ea-8142-a516ee59fea5.jpg" />then the current density <img src="13-7500970\49b357b1-4dbd-401d-a0c5-51dfbff55b3d.jpg" /> components of the plasma electrons in the plane of circularized polarized laser beam can be written as:</p><disp-formula id="scirp.28324-formula33940"><label>(8)</label><graphic position="anchor" xlink:href="13-7500970\7d32005f-48f8-41b2-a565-03cdc0775083.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28324-formula33941"><label>(9)</label><graphic position="anchor" xlink:href="13-7500970\69a58c5a-8a83-4750-b708-3ade8cceb4bc.jpg"  xlink:type="simple"/></disp-formula><p>where,</p><p><img src="13-7500970\aa3b6f61-5b31-4416-ad17-b855b34c15e4.jpg" /></p><p>and <img src="13-7500970\4d60fc1f-ca81-4ddc-97a5-c2e26acca11d.jpg" /> is the electron Larmor frequency. But at the same time the current density and the dielectric tensor <img src="13-7500970\90e27409-46dc-453f-bdab-eeba27a78b65.jpg" /> are given by:</p><disp-formula id="scirp.28324-formula33942"><label>(10)</label><graphic position="anchor" xlink:href="13-7500970\ecb87e7a-1a2e-4c5b-b801-48db2f3a8d0f.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28324-formula33943"><label>(11)</label><graphic position="anchor" xlink:href="13-7500970\a5f12a7a-fc0c-4f5f-ba20-92a2b07d51f4.jpg"  xlink:type="simple"/></disp-formula><p>Then, according to Equations (8), (9) and (11) we obtain:</p><disp-formula id="scirp.28324-formula33944"><label>(12)</label><graphic position="anchor" xlink:href="13-7500970\e9d33454-9d3c-4232-85cc-189e36d13dd9.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="13-7500970\655d5877-f2f1-4167-8748-84cc4c05681c.jpg" /> is the unit tensor and <img src="13-7500970\64942c1d-337a-48ab-b6cb-11ce6aeb7fb2.jpg" /> is the electron plasma frequency. Therefore, the dispersion relation can be written as</p><disp-formula id="scirp.28324-formula33945"><label>(13)</label><graphic position="anchor" xlink:href="13-7500970\e1ad79ee-10df-4d00-a047-8ade12d2cb6a.jpg"  xlink:type="simple"/></disp-formula><p>where, <img src="13-7500970\cf375b89-9826-459a-b59e-9d9410f4e5d1.jpg" />, <img src="13-7500970\23d835f6-3351-4b36-a500-f6c8557558ba.jpg" />, <img src="13-7500970\84c5a904-d8ab-4613-b106-63ca72f9f04a.jpg" />Also,</p><p><img src="13-7500970\167427ea-748e-4f50-9a46-f4992d949a11.jpg" />, <img src="13-7500970\6b7901e2-e242-4fdf-bfe2-f66e29449224.jpg" />and <img src="13-7500970\97a24bd0-173b-4630-a005-da09b8c6e292.jpg" /></p></sec><sec id="s3"><title>3. Discussions</title><p>In this section, we focus our attention to investigate the dispersion relationship (13) analytically and numerically in some cases for <img src="13-7500970\0cf6329d-f333-48b9-89b8-393a9d5f04ef.jpg" /> (i.e.,<img src="13-7500970\ee31b9ec-1096-4e64-809c-08d914c871f1.jpg" />). First, in the absence of the external magnetic field<img src="13-7500970\66b2d5e4-bc1c-4cf0-ba76-b7b4558ce3ec.jpg" />, it is reduced to the following equation:</p><disp-formula id="scirp.28324-formula33946"><label>(14)</label><graphic position="anchor" xlink:href="13-7500970\6986517a-1892-4fd6-b0b7-f156d3e1b09a.jpg"  xlink:type="simple"/></disp-formula><p>which gives two dispersion relations describe the propagation of laser beam in unmagnetized plasma. In this case</p><disp-formula id="scirp.28324-formula33947"><label>(15)</label><graphic position="anchor" xlink:href="13-7500970\5e587a2f-1873-4619-9eae-b5f870afc9ec.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.28324-formula33948"><label>(16)</label><graphic position="anchor" xlink:href="13-7500970\f744f5d8-6b42-46fb-98d2-2d936c407f1b.jpg"  xlink:type="simple"/></disp-formula><p>It is noticed that Equation (15) is the well known linear dispersion relation of the laser beam propagating in classical plasma <img src="13-7500970\b5a40405-6b79-4253-a21e-6638798025a0.jpg" /> and Equation (16) agrees with Equation (8), in reference [<xref ref-type="bibr" rid="scirp.28324-ref10">10</xref>], which describes the propagation of the linearly polarized laser beam in unmagnetized quantum plasma.</p><p>Second, in the case of magnetized plasma and ignoring the quantum effects caused by the Bohm potential and the quantum statistical effects through Fermi temperature<img src="13-7500970\ebd2adc1-7e46-42f1-a6b1-48a92feff252.jpg" />, Equation (13) becomes:</p><disp-formula id="scirp.28324-formula33949"><label>(17)</label><graphic position="anchor" xlink:href="13-7500970\429c9de8-6b5e-46d8-b812-3134b7b2f665.jpg"  xlink:type="simple"/></disp-formula><p>It is the dispersion relation of beam laser propagating in classical magnetized plasma which is as the earlier result [<xref ref-type="bibr" rid="scirp.28324-ref14">14</xref>].</p><p>Introducing the normalized quantities<img src="13-7500970\7f84c55f-f262-49a1-b831-5597c809ab40.jpg" />, <img src="13-7500970\1d38b3b1-1638-43ce-bc7d-1f12a4e74101.jpg" />, <img src="13-7500970\b6c3f4ba-43d4-4694-b9d9-20376268dd6b.jpg" />, <img src="13-7500970\bc5eacb3-6bb2-4ed8-9e7c-054b883a130b.jpg" />and the plasmonic coupling <img src="13-7500970\a165a601-bba4-4223-b154-7d7cac7244cb.jpg" />which describes the ratio of plasmonic energy density to the electron Fermi energy density, we rewrite the dispersion relation (16) as:</p><disp-formula id="scirp.28324-formula33950"><label>(18)</label><graphic position="anchor" xlink:href="13-7500970\e13e5d14-1bdd-455c-9443-67cb38f57249.jpg"  xlink:type="simple"/></disp-formula><p>For typical parameters of the gold metallic plasma at room temperature [<xref ref-type="bibr" rid="scirp.28324-ref12">12</xref>], n<sub>0</sub> = 5.9 &#215; 10<sup>22</sup> cm<sup>−3</sup>, ω<sub>p</sub> = 1.37 &#215; 10<sup>16</sup> s<sup>−3</sup>, V<sub>Fe</sub> = 1.4 &#215; 10<sup>8</sup> cm/s, Equation (18) is plotted for different H in <xref ref-type="fig" rid="fig1">Figure 1</xref>. It is clear that quantum effects cannot be ignored but become significant only when the wave number is large enough where the dispersion curves for different values of the parameter H = 0, 3, 5 are exactly superposed on each other’s at low wave numbers for unmagnetized plasm as shown in <xref ref-type="fig" rid="fig1">Figure 1</xref>. At zero wave number<img src="13-7500970\d2aa4ac9-562d-41a8-b40f-a6fc4115843a.jpg" />, the wave frequency equals the plasma frequency.</p><p>Again, for numerical analysis and using the normalized quantities and the above typical parameters, Equation (13) has been numerically solved to investigate the quantum and magnetic field effects on dispersion relation. <xref ref-type="fig" rid="fig2">Figure 2</xref> displays the normalized frequency <img src="13-7500970\a1447c2a-8c00-419d-9321-1c1c97be6ce8.jpg" /> against the normalized wave number <img src="13-7500970\58ec60b2-0eff-439c-b161-cc0d6fa61d5a.jpg" /> for different plasmonic parameter H = 0, 1, 3, 5. It is found that quantum effects in magnetized plasma also become significant only when the wave number is large enough for<img src="13-7500970\955501d2-f638-41f5-bfcb-080ef597c8ca.jpg" />. The dispersion curves for different values of the parameter H are exactly superposed on each other’s at low wave numbers with dispersion curve <img src="13-7500970\ff56c5c2-a3da-47c3-bd95-a8f655c1726b.jpg" /> and has changed faster with larger quantum effects for high wave number.</p><p>Besides, <xref ref-type="fig" rid="fig3">Figure 3</xref> displays the effect of the magnetic field on dispersion relation of laser propagation inside</p><p>quantum plasma (with H = 1) for very low wave numbers. It is shown at zero wave number that wave frequency equals plasma frequency in the case of unmagnetized plasma and it is less than the plasma frequency for stronger magnetic field (<img src="13-7500970\7e044ec0-acaf-4919-88d4-ab36ae72b1bb.jpg" />for <img src="13-7500970\fa1f4772-049c-475a-86a2-23c2acbb2f88.jpg" /> and <img src="13-7500970\2309aee9-fa55-4f92-a484-09a672b108ac.jpg" /> for<img src="13-7500970\dcb106a6-9436-4129-87af-bc3eded834e5.jpg" />). For increasing wave number, the wave frequency increased faster with larger magnetic field.</p></sec><sec id="s4"><title>4. Conclusion</title><p>In this work, we have investigated the general dispersion relation for the propagation of circularized laser beam in uniform electron magnetized quantum plasma based on the (QHD) equations and Maxwell’s equations. Using perturbation technique, the perturbed electron density and current due to the interaction of laser beam with quantum plasma have been obtained. Furthermore, for numerical analysis and using the normalized parameters, the general dispersion equation has been numerically solved to investigate the quantum and magnetic field effects on dispersion relation. It is shown that the quantum effects enhance the propagation phase velocity and for increasing wave number, the wave frequency increased faster with larger magnetic field.</p></sec><sec id="s5"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.28324-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">P. A. Markowich, C. A. Ringhofer and C. Schmeiser, “Semiconductor Equations,” Springer-Verlag, New York, 1990. doi:10.1007/978-3-7091-6961-2</mixed-citation></ref><ref id="scirp.28324-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">G. V. 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