<?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">WJCMP</journal-id><journal-title-group><journal-title>World Journal of Condensed Matter Physics</journal-title></journal-title-group><issn pub-type="epub">2160-6919</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/wjcmp.2018.84013</article-id><article-id pub-id-type="publisher-id">WJCMP-88391</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>
 
 
  Ac Recombination Velocity in a Lamella Silicon Solar Cell
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Matar</surname><given-names>Gueye</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>Hawa</surname><given-names>Ly Diallo</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>Attoumane</surname><given-names>Kosso Mamadou Moustapha</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Youssou</surname><given-names>Traore</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>Ibrahima</surname><given-names>Diatta</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>Gregoire</surname><given-names>Sissoko</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>School of Mines and Geology, Niamey, Niger</addr-line></aff><aff id="aff1"><addr-line>Laboratory of Semiconductors and Solar Energy, Physics Department, Faculty of Science and Technology, University Cheikh Anta Diop, Dakar, Senegal</addr-line></aff><pub-date pub-type="epub"><day>30</day><month>09</month><year>2018</year></pub-date><volume>08</volume><issue>04</issue><fpage>185</fpage><lpage>196</lpage><history><date date-type="received"><day>18,</day>	<month>October</month>	<year>2018</year></date><date date-type="rev-recd"><day>9,</day>	<month>November</month>	<year>2018</year>	</date><date date-type="accepted"><day>12,</day>	<month>November</month>	<year>2018</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 silicon solar cell with series-connected vertical junction is studied with different lamella widths—the expression of the ac recombination velocity of the excess minority carrier at the back surface is established. Spectroscopy technique reveals dominated impact of the lamella widths of the base.
 
</p></abstract><kwd-group><kwd>Silicon Solar Cell-Vertical Junction Series</kwd><kwd> Ac Recombination Velocity</kwd><kwd> Lamella Width</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The techniques of characterization of solar cell for quality control [<xref ref-type="bibr" rid="scirp.88391-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref3">3</xref>] improve the fabrication processes, go through experimental [<xref ref-type="bibr" rid="scirp.88391-ref4">4</xref>] and theoretical [<xref ref-type="bibr" rid="scirp.88391-ref5">5</xref>] studies in static [<xref ref-type="bibr" rid="scirp.88391-ref6">6</xref>] or dynamic transient [<xref ref-type="bibr" rid="scirp.88391-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref9">9</xref>] and frequency [<xref ref-type="bibr" rid="scirp.88391-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref12">12</xref>] .</p><p>The phenomenological parameters [<xref ref-type="bibr" rid="scirp.88391-ref13">13</xref>] , which allow this quality control, are the carrier recombination velocity:</p><p>1) in the bulk [<xref ref-type="bibr" rid="scirp.88391-ref14">14</xref>] , defined by the diffusion length (L) and coefficient (D), lifetime (τ) of excess minority carrier.</p><p>2) on the surfaces [<xref ref-type="bibr" rid="scirp.88391-ref15">15</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref16">16</xref>] , i.e., recombination velocity (Sf) at the junction (n-p) [<xref ref-type="bibr" rid="scirp.88391-ref17">17</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref18">18</xref>] , (Sb) at the junction (p-p<sup>+</sup>) [<xref ref-type="bibr" rid="scirp.88391-ref19">19</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref20">20</xref>] , and (Sg) at the grain boundaries in the 3-dimensional [<xref ref-type="bibr" rid="scirp.88391-ref21">21</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref22">22</xref>] model.</p><p>The solar cell is placed under different operating modes [<xref ref-type="bibr" rid="scirp.88391-ref23">23</xref>] and for different illuminations: monochromatic [<xref ref-type="bibr" rid="scirp.88391-ref24">24</xref>] , polychromatic [<xref ref-type="bibr" rid="scirp.88391-ref25">25</xref>] , constant multspectral [<xref ref-type="bibr" rid="scirp.88391-ref26">26</xref>] .</p><p>The solar cell can be maintained under different experimental conditions while varying: temperature [<xref ref-type="bibr" rid="scirp.88391-ref27">27</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref28">28</xref>] , electric field [<xref ref-type="bibr" rid="scirp.88391-ref29">29</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref30">30</xref>] , magnetic field [<xref ref-type="bibr" rid="scirp.88391-ref31">31</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref32">32</xref>] , or irradiation energy of particles [<xref ref-type="bibr" rid="scirp.88391-ref33">33</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref34">34</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref35">35</xref>] .</p><p>To achieve low cost solar concentrator cell, vertical multi-junction (VMJ) cells have been manufactured [<xref ref-type="bibr" rid="scirp.88391-ref36">36</xref>] . There are two types of VMJ [<xref ref-type="bibr" rid="scirp.88391-ref28">28</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref37">37</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref38">38</xref>] , according to the connection between cell units, in view to improve, either charge carrier current collection or tension. Thus, series-connected VMJ [<xref ref-type="bibr" rid="scirp.88391-ref39">39</xref>] and parallel-connected VMJ [<xref ref-type="bibr" rid="scirp.88391-ref40">40</xref>] have been process, allowing poor minority carrier diffusion length to be collected, by use of silicon material regardless of crystal orientation (multi-crystalline or ribbon).</p><p>In our study, the structure of the series-connected vertical junction solar cell [<xref ref-type="bibr" rid="scirp.88391-ref39">39</xref>] with different lamella widths (H), is investigated in order to determine the recombination velocity of the excess minority carrier at the back surface. This new expression of the ac recombination velocity is analyzed through Bode and Nyquist diagrams, and is shown to depend strongly upon the lamella widths of the base (H).</p></sec><sec id="s2"><title>2. Theory</title><p><xref ref-type="fig" rid="fig1">Figure 1</xref> shows series-connected vertical multi-junction solar cells where each base (lamella) is framed by two emitters. Between emitter (n<sup>+</sup>) and base (p) we have the space charge region (SCR), called the junction. And at the back side of each base region, there is a high doping layer (p<sup>+</sup>) giving rise to a back surface field (BSF), which induced the back surface recombination velocity (Sb) (<xref ref-type="fig" rid="fig2">Figure 2</xref>).</p><p>In this series-connected architecture, each solar cell unitis separated on both sides by metal contacts [<xref ref-type="bibr" rid="scirp.88391-ref36">36</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref37">37</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref39">39</xref>] .</p><p>The continuity equation at which the density of minority charge carriers in excess obeyed δ ( x , t ) at the position x in the base, in an instant t, is given by [<xref ref-type="bibr" rid="scirp.88391-ref41">41</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref42">42</xref>]:</p><p>D ( ω ) ⋅ ∂ 2 δ ( x , t ) ∂ x 2 − δ ( x , t ) τ = − G ( z , t ) + ∂ δ ( x , t ) ∂ t (1)</p><p>The ac component of the excess minority density is in the following form:</p><p>δ ( x , t ) = δ ( x ) ⋅ e j ω t (2)</p><p>j is the complex notation.</p><p>With δ ( x ) is the steady state minority carrier density position dependent.</p><p>The expression of the ac generation rate G ( z , t ) of the minority carrier at depth z, is given by [<xref ref-type="bibr" rid="scirp.88391-ref43">43</xref>]:</p><p>G ( z , t ) = g ( ω , α , z ) ⋅ e J ω ⋅ t (3)</p><p>with:</p><p>g ( ω , α , z ) = K ( ω , α ) ⋅ exp ( − α ⋅ z ) (4)</p><p>and</p><p>K ( ω , α ) = − [ α ⋅ I ( λ ) ⋅ ( 1 − R ( λ ) ) D ( ω ) ⋅ [ α 2 − 1 L ( ω ) 2 ] ] (5)</p><p>I (λ) is the intensity of the monochromatic illumination of wavelength λ. α is the absorption coefficient of the monochromatic light incident on the cell and R (λ) its reflectance coefficient.</p><p>D (ω) and L (ω) are respectively, the excess ac minority carrier diffusion coefficient and diffusion length in the base subjected to illumination in frequency modulation (ω).</p><p>L (ω) and D (ω) ac expressions are giving by [<xref ref-type="bibr" rid="scirp.88391-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref44">44</xref>]:</p><p>D ( ω ) = D ⋅ [ 1 1 + ( ω ⋅ τ ) 2 − j ⋅ ω ⋅ τ 1 + ( ω ⋅ τ ) 2 ] (6)</p><p>L ( ω ) = D ⋅ [ τ 1 + ( ω ⋅ τ ) 2 − j ⋅ ω ⋅ τ 2 1 + ( ω ⋅ τ ) 2 ] (7)</p><p>where D denotes the diffusion constant and τ the bulk lifetime in steady state.</p><p>By substituting Equation (1) together with Equation (2) and Equation (3), leads to:</p><p>∂ 2 δ ( x , ω ) ∂ x 2 − δ ( x , ω ) L ( ω ) 2 + g ( ω , α , z ) D ( ω ) = 0 (8)</p><p>Thus the resolution of Equation (6) gives the excess minority carrier density in the base through the following expression:</p><p>δ ( x , ω , α , z ) = A cosh ( x L ( ω ) ) + B sinh ( x L ( ω ) ) + K ( ω , α ) ⋅ exp ( − α ⋅ z ) (9)</p><p>with coefficients A et B are deduced from the boundary conditions:</p><p>1) At the junction (x = 0), the expression of the photocurrent J p h ( 0 , ω , α , z ) [<xref ref-type="bibr" rid="scirp.88391-ref20">20</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref45">45</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref46">46</xref>] is given by:</p><p>q ⋅ D ( ω ) ∂ δ ( x , ω , α , z ) ∂ x | x = 0 = q ⋅ S f ⋅ δ ( 0 , ω , α , z ) = J p h ( 0 , ω , α , z ) (10)</p><p>2) On the back side in the base at x = H.</p><p>∂ δ ( x , ω , α , z ) ∂ x | x = H = − S b D ( ω ) δ ( H , ω , α , z ) (11)</p><p>Sf and Sb are respectively the recombination velocities of the excess minority carrier at the junction and at the back surface. The recombination velocity Sf reflects the charge carrier velocity of passage at the junction, in order to participate in the photocurrent. It is then imposed, by the external load which fixes the solar cell operating point [<xref ref-type="bibr" rid="scirp.88391-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref45">45</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref46">46</xref>] . It has an intrinsic component, which represents the carrier losses associated with the shunt resistor in the solar cell electrical equivalent model [<xref ref-type="bibr" rid="scirp.88391-ref47">47</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref48">48</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref49">49</xref>] . The excess minority carrier recombination velocity Sb on the back surface is associated with the presence of the p<sup>+</sup> layer, which generates an electric field for throwing back the charge carrier toward the junction [<xref ref-type="bibr" rid="scirp.88391-ref50">50</xref>] .</p><p>After calculation, the following expression of the ac excess minority carrier density is obtained by:</p><p>δ ( x , ω , α , z ) = A ( H , ω , α , z , S f , S b ) cosh ( x L ( ω ) )     + B ( H , ω , α , z , S f , S b ) sinh ( x L ( ω ) )     + K ( ω , α ) ⋅ exp ( − α ⋅ z ) (12)</p></sec><sec id="s3"><title>3. Results and Discussions</title><p>The excess minority carrier recombination velocity at the back surface is deduced from the resolution of the following equation [<xref ref-type="bibr" rid="scirp.88391-ref45">45</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref46">46</xref>]:</p><p>∂ J p h ( H , ω , α , z , S f , S b ) ∂ S f = 0 (13)</p><p>Solving Equation (13) leads to two solutions [<xref ref-type="bibr" rid="scirp.88391-ref45">45</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref46">46</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref47">47</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref49">49</xref>] . The intrinsic solution, i.e., that which is not a function of the absorption coefficient, is retained and its expression is given by:</p><p>S b ( ω , H ) = − D ( ω ) L ( ω ) ⋅ tanh ( H L ( ω ) ) (14)</p><p>Sb in complex form (real and imaginary components) is presented by analogy of the effect of Maxwell-Wagner-Sillars (MWS) model [<xref ref-type="bibr" rid="scirp.88391-ref50">50</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref51">51</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref52">52</xref>] and can be written as:</p><p>S b ( ω , H ) = S b ′ ( ω , H ) + J ⋅ S b ″ ( ω , H ) (15)</p><p>We define the ac phase as following equation:</p><p>tan ( ϕ ( ω , H ) ) = S b ″ ( ω , H ) S b ′ ( ω , H ) (16)</p><p>S b a m p l ( ω , H ) and ϕ ( ω , H ) correspond to the amplitude and phase component of Sb.</p><p>We represent in <xref ref-type="fig" rid="fig3">Figure 3</xref> the spectra of the excess minority carrier recombination velocity at the back surface for different lamella H thickness values.</p><p><xref ref-type="fig" rid="fig3">Figure 3</xref> shows a decrease in the amplitude of the excess minority carrier recombination at the back surface when (H) the thickness of the lamella increases.</p><p>The large (H) thicknesses give weak oscillation periods. Thus whatever the lamella width, the oscillation is around a fixed (Sb0) value of the excess minority carrier recombination velocity.</p><p><xref ref-type="fig" rid="fig4">Figure 4</xref> gives the profile of Sb the amplitude of the recombination velocity as a function of H the base thickness, for given values of the modulation frequency of the illumination.</p><p>For high range frequencyvalues (ωτ &gt; 1) we observe a damped sinusoid (aperiodic response), to then give the appearance of an exponential growth. For large lamella width, these curves tend towards an asymptote (Sb0 = 4184 cm/s), whatever the frequency.</p><p>The amplitude and the phase spectra of the recombination velocity (Sb) are given respectively in <xref ref-type="fig" rid="fig5">Figure 5</xref>(a) and <xref ref-type="fig" rid="fig5">Figure 5</xref>(b) with different thicknesses (Bode diagrams).</p><p>On the frequency axis, the region corresponding to the frequencies below 10<sup>4</sup> rd/s (i.e. ω τ ≪ 1 ), constitutes the steady state.</p><p>In this zone the amplitude of Sb<sub>Ampl</sub> believes with the thickness H. The phase remains constant and obviously equal to zero.</p><p>In high frequency region 10<sup>4</sup> rd/s &lt; ω, tarts the dynamic regime i.e. ω τ ≫ 1 ), showing a sinusoid of amplitude (Sb<sub>Ampl</sub>), oscillating around Sb0, the asymptotical recombination velocity, with periods T<sub>Sb</sub> decreasing with H (see <xref ref-type="table" rid="table1">Table 1</xref>).</p><p>The phase spectrum shows regular sinusoids with constant amplitudes f<sub>ampl</sub>, for each given H lamella widths, but decreases with H. The period Tf<sub>ampl</sub> of these oscillations decreases with the lamella thickness H (see <xref ref-type="table" rid="table2">Table 2</xref>).</p><p><xref ref-type="fig" rid="fig6">Figure 6</xref> produces the representation of the imaginary part as a function of the real part of the recombination velocity Sb.</p><p>The circles obtained have for their center Sb0, on the axis of the reals. The radius of the circles increases when the lamella thickness H decreases. According to the spectroscopy techniques [<xref ref-type="bibr" rid="scirp.88391-ref51">51</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref52">52</xref>] , the intersections of the circles with the real axis, at high frequency range, indicate the presence of a series resistance which decreases with H the lamella thickness. The negative part of circles indicates a capacitive phenomenon (C), while the positive part, an inductive</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Sb periods for different lamella widths</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >H (cm)</th><th align="center" valign="middle" >0.013</th><th align="center" valign="middle" >0.015</th><th align="center" valign="middle" >0.017</th><th align="center" valign="middle" >0.02</th></tr></thead><tr><td align="center" valign="middle" >(SbAmpl) (10<sup>5</sup> rad/s)</td><td align="center" valign="middle" >10.070<sup> </sup></td><td align="center" valign="middle" >8.776<sup> </sup></td><td align="center" valign="middle" >7.700<sup> </sup></td><td align="center" valign="middle" >6.472<sup> </sup></td></tr><tr><td align="center" valign="middle" >T (SbAmpl) (10<sup>−</sup><sup>6</sup> s)</td><td align="center" valign="middle" >6.240</td><td align="center" valign="middle" >7.160</td><td align="center" valign="middle" >8.160</td><td align="center" valign="middle" >9.700</td></tr><tr><td align="center" valign="middle" >Sb (Ampl) (cm/s)</td><td align="center" valign="middle" >4573</td><td align="center" valign="middle" >4422</td><td align="center" valign="middle" >4329</td><td align="center" valign="middle" >4254</td></tr></tbody></table></table-wrap><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Phase period for different lamella widths</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >H(cm)</th><th align="center" valign="middle" >0.013</th><th align="center" valign="middle" >0.015</th><th align="center" valign="middle" >0.017</th><th align="center" valign="middle" >0.02</th></tr></thead><tr><td align="center" valign="middle" >f (Ampl)</td><td align="center" valign="middle" >0.089<sup> </sup></td><td align="center" valign="middle" >0.055<sup> </sup></td><td align="center" valign="middle" >0.034</td><td align="center" valign="middle" >0.017</td></tr><tr><td align="center" valign="middle" >ω<sub>f</sub> (Ampl) (10<sup>5</sup> rad/s)</td><td align="center" valign="middle" >10.120<sup> </sup></td><td align="center" valign="middle" >8.584<sup> </sup></td><td align="center" valign="middle" >7.952<sup> </sup></td><td align="center" valign="middle" >6.604<sup> </sup></td></tr><tr><td align="center" valign="middle" >T<sub>f</sub> (10<sup>−6</sup> s)</td><td align="center" valign="middle" >6.200</td><td align="center" valign="middle" >7.320</td><td align="center" valign="middle" >7.902</td><td align="center" valign="middle" >9.515</td></tr></tbody></table></table-wrap><p>phenomenon (Lh), both decrease with the lamella thickness H. The ac equivalent circuit of Sb, suggests that, the capacitor and the inductor are associated in parallel and connected in series with a resistance (obtained for large frequency) [<xref ref-type="bibr" rid="scirp.88391-ref53">53</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref54">54</xref>] [<xref ref-type="bibr" rid="scirp.88391-ref55">55</xref>] .</p></sec><sec id="s4"><title>4. Conclusion</title><p>The series-connected vertical multi-junction silicon solar cell was studied under frequency modulated illumination and yielded the determination of the ac back surface recombination velocity of the excess minority carrier. It is expressed as dependent of both lamella thickness and illumination frequency. The excess minority carrier recombination is investigated through the Bode diagrams of its amplitude and phase. The study also showed through the Nyquist diagram, the capacitive, inductive and resistive responses of the ac recombination velocity Sb, as well as the effect of the thickness of the lamella based solar cell.</p></sec><sec id="s5"><title>Conflicts of Interest</title><p>The authors declare no conflicts of interest regarding the publication of this paper.</p></sec><sec id="s6"><title>Cite this paper</title><p>Gueye, M., Diallo, H.L., Moustapha, A.K.M., Traore, Y., Diatta, I. and Sissoko, G. (2018) Ac Recombination Velocity in a Lamella Silicon Solar Cell. World Journal of Condensed Matter Physics, 8, 185-196. https://doi.org/10.4236/wjcmp.2018.84013</p></sec></body><back><ref-list><title>References</title><ref id="scirp.88391-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">(1995) Silicon Solar Cells, Advanced Principles and Practice. 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