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  <name xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Solar Cells</name>
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  <md:version xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">**new**</md:version>
  <md:created xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">2003/06/17 15:50:29.301 GMT-5</md:created>
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      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Bill</md:firstname>
      
      <md:surname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Wilson</md:surname>
      <md:email xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">wlw@rice.edu</md:email>
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      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Elizabeth</md:firstname>
      
      <md:surname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Gregory</md:surname>
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      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Jeffrey</md:firstname>
      
      <md:surname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Silverman</md:surname>
      <md:email xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">jsilv@rice.edu</md:email>
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    <md:keyword xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">solar cells</md:keyword>
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  <md:abstract xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Solar Cells</md:abstract>
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  <content xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">
    <para xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="opposite"> 
      Now let us look at the opposite process of light generation for
      a moment. Consider the following situation.
      <figure xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="illumination">
	<name xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">P-N diode under illlumination</name>
	<media xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" type="image/png" src="2_63.png"/>
      </figure>      
      We have just a plain old normal p-n junction, only now, instead
      of applying an external voltage, we imagine that the junction is
      being illuminated with light whose photon energy is greater than
      the band-gap.  In this situation, instead of recombination, we
      will get photo-generation of electron hole pairs.  The photons
      simply excite electrons from the full states in the valance
      band, and "kick" them up into the conduction band, leaving a
      hole behind.  As you can see from <cnxn xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" target="illumination"/>,
      this creates excess electrons in the conduction band in the
      p-side of the diode, and excess holes in the valance band of the
      n-side.  These carriers can diffuse over to the junction, where
      they will be swept across by the built-in electric field in the
      depletion region.  If we were to connect the two sides of the
      diode together with a wire, a current would flow through that
      wire as a result of the electrons and holes which move across
      the junction.
    </para>
    <para xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="flow">      
      Which way would the current flow?  A quick look at <cnxn xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" target="illumination"/> shows that holes (positive charge
      carriers) are generated on the n-side and they float up to the
      p-side as they go across the junction.  Hence positive current
      must be coming out of the anode, or p-side of the junction.
      Likewise, electrons generated on the p-side fall down the
      junction potential, and come out the n-side, but since they have
      negative charge, this flow represents current going
      <emphasis xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">into</emphasis> the cathode.  We have constructed a
      <term xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">photovoltaic diode</term>, or <term xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">solar cell</term>
      (<cnxn xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" target="cell"/>)!  Here is a picture of what this would
      look like schematically.  We might like to consider the
      possibility of using this device as a source of energy, but the
      way we have things set up now, since the potential across the
      diode is zero, and since power equals current times voltage, we
      see that we are getting nada from the cell.  What we need,
      obviously, is a load resistor, so let's put one in.  It should
      be clear from <cnxn xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" target="loadresistor"/> that the photo
      current will go through the load resistor in such a way that it
      biases the diode in the <emphasis xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">forward</emphasis> direction,
      which, of course will cause current to flow back into the anode.
      This complicates things, it seems we have current coming
      <emphasis xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">out</emphasis> of the diode and current going
      <emphasis xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">into</emphasis> the diode all at the same time!  How
      are we going to figure out what is going on?
      <figure xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="cell">
	<name xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Schematic representation of a photovoltaic cell</name>
	<media xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" type="image/png" src="2_64.png"/>
      </figure>
      <figure xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="loadresistor">
	<name xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Photovoltaic cell with a load resistor</name>
	<media xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" type="image/png" src="2_65.png"/>
      </figure>      
      The answer is to make a model.  The current which arises due to
      the photon flux can be conveniently represented as a current
      source, we can leave the diode as a diode, and we have the
      circuit shown in <cnxn xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" target="model"/>.  Even though we show
      <m:math><m:ci><m:msub><m:mi>I</m:mi><m:mi>out</m:mi>
      </m:msub></m:ci></m:math> coming out of the device, we know by
      the usual polarity convention that when we define
      <m:math><m:ci><m:msub><m:mi>V</m:mi><m:mi>out</m:mi>
      </m:msub></m:ci></m:math> as being positive at the top, then we
      should show the current for the photovoltaic,
      <m:math><m:ci><m:msub><m:mi>I</m:mi><m:mi>pv</m:mi>
      </m:msub></m:ci></m:math> as current going into the top, which
      is what was done in <cnxn xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" target="model"/>.  Note that
      <m:math>
	<m:apply>
	  <m:eq/>
	  <m:ci><m:msub>
	      <m:mi>I</m:mi>
	      <m:mi>pv</m:mi>
	    </m:msub></m:ci>
	  <m:apply>
	    <m:minus/>
	    <m:ci><m:msub>
	      <m:mi>I</m:mi>
	      <m:mi>diode</m:mi>
	    </m:msub></m:ci>
	    <m:ci><m:msub>
	      <m:mi>I</m:mi>
	      <m:mi>photo</m:mi>
	    </m:msub></m:ci>
	  </m:apply>
	</m:apply>
      </m:math>, so all we need to do graphically is to subtract the
      two currents Note that we have numbered the four quadrants in
      the I-V plot of the total PV current.  In quadrant I and III,
      the product of <m:math><m:ci>I</m:ci></m:math> and
      <m:math><m:ci>V</m:ci></m:math> is a positive number, meaning
      that power is being <emphasis xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">dissipated</emphasis> in the cell.
      For quadrant II and IV, the product of
      <m:math><m:ci>I</m:ci></m:math> and
      <m:math><m:ci>V</m:ci></m:math> is negative, and so we are
      getting power <emphasis xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">from</emphasis> the device.  Clearly we
      want to operate in quadrant IV.  In fact, without the addition
      of an external battery or current source, the circuit, will
      <emphasis xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">only</emphasis> run in the IV'th quadrant.  Consider
      adjusting <m:math><m:ci><m:msub><m:mi>R</m:mi><m:mi>L</m:mi>
      </m:msub></m:ci></m:math>, the load resistor from 0 (a short) to
      <m:math><m:infinity/></m:math> (an open). With 
      <m:math>
	<m:apply>
	  <m:eq/>
	  <m:ci><m:msub>
	      <m:mi>R</m:mi>
	      <m:mi>L</m:mi>
	    </m:msub></m:ci>
	  <m:cn>0</m:cn>
	</m:apply>
      </m:math>, we would be at point A on <cnxn xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" target="combination"/>.  As
      <m:math><m:ci><m:msub><m:mi>R</m:mi><m:mi>L</m:mi>
      </m:msub></m:ci></m:math> starts to increase from zero, the
      voltage across the device will start to increase also, and we
      will move to point B, say.  As
      <m:math><m:ci><m:msub><m:mi>R</m:mi><m:mi>L</m:mi>
      </m:msub></m:ci></m:math> gets bigger and bigger, we keep moving
      along the curve until, at point C, where
      <m:math><m:ci><m:msub><m:mi>R</m:mi><m:mi>L</m:mi>
      </m:msub></m:ci></m:math> is an open and we have the maximum
      voltage across the device, but, of course, no current coming
      out!
      <figure xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="model">
	<name xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Model of PV cell</name>
	<media xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" type="image/png" src="2_66.png"/>
      </figure>  
      <figure xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="combination">
	<name xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Combining the diode and the current source</name>
	<media xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" type="image/png" src="2_67.png"/>
      </figure>       
      Power, of course, is 
      <m:math>
	<m:apply>
	  <m:times/>
	  <m:ci>V</m:ci>
	  <m:ci>I</m:ci>
	</m:apply>
      </m:math> so at B for instance, the power coming out would be
      represented by the area enclosed by the two dotted lines and the
      coordinate axes.  Someplace about where I have point B would be
      where we would be getting the most power out of out solar cell.
    </para>
    <para xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="real">      
      <cnxn xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" target="solarcell"/> shows you what a real solar cell
      would look like.  They are usually made from a complete wafer of
      silicon, to maximize the usable area.  A shallow (0.25 μm)
      junction is made on the top, and top contact are applied as
      stripes of metal conductor as shown.  An anti-reflection (AR)
      coating is applied on top of that, which accounts for the bluish
      color which a typical solar cell has.
      <figure xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="solarcell">
	<name xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">A real solar cell</name>
	<media xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" type="image/png" src="2_68.png"/>
      </figure> 
      
      The solar power flux on the earth's surface is (conveniently)
      about 
      <m:math>
	<m:apply>
	  <m:times/>
	  <m:cn>1</m:cn>
	  <m:apply>
	    <m:divide/>
	    <m:ci>kW</m:ci>
	    <m:apply>
	      <m:power/>
	      <m:ci>m</m:ci>
	      <m:cn>2</m:cn>
	    </m:apply>
	  </m:apply>
	</m:apply>
      </m:math> or 
      <m:math>
	<m:apply>
	  <m:times/>
	  <m:cn>100</m:cn>
	  <m:apply>
	    <m:divide/>
	    <m:ci>mW</m:ci>
	    <m:apply>
	      <m:power/>
	      <m:ci>cm</m:ci>
	      <m:cn>2</m:cn>
	    </m:apply>
	  </m:apply>
	</m:apply>
      </m:math>. So if we made a solar cell from a 4 inch diameter
      wafer (typical) it would have an area of about 
      <m:math>
	<m:apply>
	  <m:times/>
	  <m:cn>81</m:cn>
	  <m:apply>
	    <m:power/>
	    <m:ci>cm</m:ci>
	    <m:cn>2</m:cn>
	  </m:apply>
	</m:apply>
      </m:math> and so would be receiving a flux of about 8.1 Watts.
      Typical cell efficiencies run from about 10% to maybe 15% unless
      special (and costly) tricks are made.  This means that we will
      get about 1.2 Watts out from a single wafer.  Looking at B on
      2.59 we could guess that
      <m:math><m:ci><m:msub><m:mi>V</m:mi><m:mi>out</m:mi>
      </m:msub></m:ci></m:math> will be about 0.5 to 0.6 volts, thus
      we could expect to get maybe around 2.5 amps from a 4 inch wafer
      at 0.5 volts with 15% efficiency under the illumination of one
      sun.
      
	  
    </para>
  </content>
  
</document>
