<?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.2012.39133</article-id><article-id pub-id-type="publisher-id">JMP-22624</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>
 
 
  Influence of a Magnetic Guide Field on Injection in Wakefield Acceleration
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>lain</surname><given-names>Bourdier</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>Sébastien</surname><given-names>Rassou</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>Guillaume</surname><given-names>Girard</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>Mathieu</surname><given-names>Drouin</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>CEA, DAM, DIF, Arpajon, France</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>alain.bourdier@gmail.com(LB)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>24</day><month>09</month><year>2012</year></pub-date><volume>03</volume><issue>09</issue><fpage>1018</fpage><lpage>1020</lpage><history><date date-type="received"><day>July</day>	<month>5,</month>	<year>2012</year></date><date date-type="rev-recd"><day>August</day>	<month>5,</month>	<year>2012</year>	</date><date date-type="accepted"><day>August</day>	<month>12,</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 influence of an external static field applied in the direction parallel to the direction of propagation of a high intensity driving laser pulse on the electron trapping in laser wakefield acceleration is explored.
 
</p></abstract><kwd-group><kwd>Laser Wakefield Acceleration; Magnetic Field; Electron Injection; Self-Trapping</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>In the LWFA process, an electron density bubble [1,2] is driven in low density plasma by the laser pulse through the ponder motive force. For intensities high enough, self injection of electrons into the wake can take place, and a charge can be accelerated. It is well known that trapping of the background electrons begins much below the longitudinal wave-breaking limit [3-5]. The transverse wavebreaking regime is the situation where a static magnetic field should play an important role.</p><p>A theoretical model for electron self-injection, in the case when a strong magnetic field is applied, is reported in this paper. The spatial distribution of the potential created by the bubble is calculated. It is shown that the magnetic field reduces the transverse motion of electrons, making trapping in the accelerating bubble more likely. It is also shown, with PIC code simulations, in good agreement with results previously published [<xref ref-type="bibr" rid="scirp.22624-ref5">5</xref>], that the electric charge accelerated can be enhanced by a static magnetic field.</p></sec><sec id="s2"><title>2. Theoretical Model</title><p>In this theoretical approach, the bubble is assumed to be a sphere moving in plasma along the z-axis with relativistic velocity <img src="18-7500829\ae2a34be-214a-4560-8e3f-3d0472c4079f.jpg" /> [<xref ref-type="bibr" rid="scirp.22624-ref6">6</xref>]. Dimensionless units are used. The time is normalized to<img src="18-7500829\f2a90dd4-d5e7-4333-881b-d901993a6ca9.jpg" />, the length to<img src="18-7500829\69020ba5-a613-46a0-a894-54a7f13aa3db.jpg" />, the velocity to c, the electric field to<img src="18-7500829\ad617ab9-97c0-498e-a0c6-44b18009a03d.jpg" />, the magnetic field to<img src="18-7500829\372f815a-244f-465c-9bc2-7be03e443397.jpg" />, and the electron density to the background density n<sub>0</sub>. The variable <img src="18-7500829\8dda787f-7e74-434a-8767-44a5c3dfd09b.jpg" /> is introduced. In the laboratory frame, the following convenient gauge is used: <img src="18-7500829\5d086e8d-1edb-4521-9fb0-593e06ba76c1.jpg" />[6-9]. Inside the bubble one can consider that <img src="18-7500829\c9f097e4-ad94-44d8-8ade-8f30f551129d.jpg" /> as the intensity of the laser pulse has a nonzero value only very close to the front of the cavity. Then one has to solve the following two equations: <img src="18-7500829\00761578-1b4e-4447-a53b-42b7999cfa4c.jpg" />and <img src="18-7500829\93bdcbb7-a8f7-432f-a249-76409a7fd40c.jpg" /> [6,7]. Considering that one has a cylindrical symmetry, the solution is</p><p><img src="18-7500829\dd7a868c-c283-4428-b3ca-063bb8a239ef.jpg" /></p><p>where C is a constant. The electron sheath around the cavity screens the ion field in the surrounding plasma. The radial electrostatic field acting on a relativistic electron is modelled as <img src="18-7500829\60e07507-0098-41b7-b41a-4847f259927e.jpg" /> where R is the sphere radius, d is the width of the electron sheath, r is given by <img src="18-7500829\e002eee0-55d4-4a1e-b36c-4e935de3f538.jpg" /> where <img src="18-7500829\832e0577-7ed9-488d-8428-332c45497223.jpg" /> is defined by:<img src="18-7500829\b9abb6b8-16ff-4b6a-8d40-57454e1f95d3.jpg" />. Vector <img src="18-7500829\817aa86b-80e0-473b-8595-56116c0f775d.jpg" /> reads:<img src="18-7500829\b566c23d-6069-4976-9ec3-eb4245f61169.jpg" />. Taking into account this screening function leads to the following scalar potential [6,8,9]</p><disp-formula id="scirp.22624-formula46140"><label>(1)</label><graphic position="anchor" xlink:href="18-7500829\1f5fd20c-04c8-49d2-b3d8-692cc69c7645.jpg"  xlink:type="simple"/></disp-formula><p>where:<img src="18-7500829\e35655b8-647e-4405-b048-78dd7f4cbeb2.jpg" />. The constant of integration was chosen such as <img src="18-7500829\e48b2e45-1678-4733-a9ba-58e02d10ec88.jpg" /> when r goes to infinity. It was shown numerically that <img src="18-7500829\02cc17c6-29d1-44c0-a10a-997dd2a98780.jpg" /> varies slowly close to the center of the bubble and decreases very rapidly close to the electron sheath.</p><p>The Hamiltonian of one electron is:</p><p><img src="18-7500829\a1b47138-ba50-4fae-997d-e18e4db39614.jpg" />where <img src="18-7500829\42d83545-3e00-419c-af48-f6325ed8cb69.jpg" /> is the canonical momentum of the electron. Then, the canonical transformation:<img src="18-7500829\c9234780-7bc3-40da-a94a-751f577ca6d2.jpg" />, given by the type-2 generating function <img src="18-7500829\0d437c93-caa0-455d-8207-066cf0961733.jpg" /> is performed. The new canonical variables are defined by <img src="18-7500829\58937dc5-7591-4231-911a-9d75e808d866.jpg" /> and<img src="18-7500829\4f25e6ad-e60d-4a27-806f-2dbc349e6608.jpg" />, the new Hamiltonian, in terms of the new variables, reads <img src="18-7500829\8e85aff3-e189-4ad5-9c8b-a81c737e38e4.jpg" />. Some electrons which are not trapped in the wakefield are trapped when a very high magnitude static magnetic field is applied (<xref ref-type="fig" rid="fig1">Figure 1</xref>).</p><p>Many trajectories are bent by the magnetic field, keeping particles closer to the rear of the bubble. Then, the electron trapping is more likely to occur.</p><p>The equation for variable <img src="18-7500829\7483d112-c6ac-4b1e-90a1-7214a098d047.jpg" /> is given by:</p><p><img src="18-7500829\7171791f-21d1-42d2-ae73-5fce8a79dddd.jpg" />. At a point of return in the cavity, the following condition must be satisfied:</p><p><img src="18-7500829\8e046a5b-9219-4805-952a-8e88341091d0.jpg" />. Assuming that particles have an initial Hamiltonian<img src="18-7500829\72c02dd4-c014-4624-be74-530223a5a8a6.jpg" />, the domain in phase space where electrons are trapped can be defined by [<xref ref-type="bibr" rid="scirp.22624-ref6">6</xref>]</p><disp-formula id="scirp.22624-formula46141"><label>(2)</label><graphic position="anchor" xlink:href="18-7500829\3ade3a08-b329-49a1-996f-5cf0e029c06f.jpg"  xlink:type="simple"/></disp-formula><p>As this condition [Equation (2)], and the potential inside the bubble are the same as those previously obtained by Kostyukov et al. ignoring the magnetic field, the trapping condition, <img src="18-7500829\96f384cd-00b4-4c9d-ad92-a7239efb5ff2.jpg" />, is still valid [6,8,9]. As we only consider very high intensity lasers interacting with low density plasma, u<sub>0</sub> will not be significantly affected by a static magnetic field. Moreover, the size of the bubble is not significantly modified by the static magnetic field in the situations considered in our PIC code simulations. Consequently, the enhancement of electron trapping, in the PIC code simulation results described in the next paragraph, seems to be mainly due to the fact that strong static magnetic fields will partly suppress the transverse motion of electrons.</p></sec><sec id="s3"><title>3. PIC Code Simulation Results</title><p>Numerical simulations were conducted using the twodimensional PIC code CALDER [<xref ref-type="bibr" rid="scirp.22624-ref10">10</xref>]. As shown in Figures 2 and 3, a static magnetic field applied in parallel with the direction of propagation of the driving laser pulse does enhance the particle trapping in the first bubble.</p></sec><sec id="s4"><title>4. Conclusion</title><p>The influence of a strong static magnetic field parallel to the direction of propagation of the laser pulse on electron trapping in the accelerating electron cavity has been studied. The trapping condition is formally the same as the one previously derived by Kostyukov et al. [<xref ref-type="bibr" rid="scirp.22624-ref6">6</xref>]. The enhanced trapping associated to the magnetic field is due to the fact that trajectories are bent which suppresses partially the particles’ transverse motion. Numerical simulations were also conducted, they confirm that a constant magnetic field is an important controlling knob for improving the electron trapping in the LWFA process.</p></sec><sec id="s5"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.22624-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">A. Pukhov and J. 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