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<title>Memorandum from  A. C. Menius, Jr. and R. L. Murray to C. K. Beck</title>
<title>[a machine-readable transcription]</title>
<author>Murray, Raymond L.</author>
<author>Menius, A. C., Jr.</author>
<respStmt>
<resp>Creation of machine-readable version: </resp>
<name>Russell S. Koonts</name>
<resp>Creation of digital images: </resp>
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<publisher>NCSU Libraries.</publisher>
<pubPlace>Raleigh, NC.</pubPlace>
<idno type="ETC"> Modern English, MurNBwindow041751</idno>
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<p>Available from: NC State University Archives</p>
<p>Publicly-accessible</p>
<p n="public">URL: http://www.lib.ncsu.edu/archives/etext/engineering/reactor/murray/</p>
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<date>2000</date>
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<p>Nuclear Reactor Digitization Project</p>
<p>Raymond L. Murray Reactor Project Notebook</p>
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<note>Illustrations have been included from the print version.</note>
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<title>Memorandum from  A. C. Menius, Jr. and R. L. Murray to C. K. Beck</title>
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<author>Raymond L. Murray</author>
<author>A. C. Menius, Jr.</author>
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<idno>Manuscript copy consulted: NCSU Libraries call number UA105.16</idno>
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<text id="MurNBwindow041751T">

<front><div1 type="summary" n="1">
<head><hi rend="bold"><hi rend="center">Memorandum from  A. C. Menius, Jr. and R. L. Murray to C. K. Beck</hi><lb/>
<bibl><abbr>Typescript</abbr><lb/> <extent>3 pp.</extent> <lb/><date value="1951-04-17">April 17, 1951</date><lb/> <idno rend="suppress">MurNBwindow041751</idno></bibl></hi></head>
<p>

</p>
</div1>
</front>

<body>
<pb n=""/>
<p><seg><xref id="reactorlg/MurNBwindow041751a.jpg" rend="new">
<figure entity="MurNBwindow041751a"></figure></xref></seg></p>
<div1 type="letter" n="1">

<opener>
<dateline><date value="1951-04-17">April 17, 1951</date></dateline>
<hi rend="italics">NCSC-15</hi>
<lb/>
TO:       <name type="person">C. K Beck</name><lb/>
FROM:     <name type="person">A. C. Menius, Jr.</name> and <name type="person"><abbr expan="Raymond">R.</abbr> L. Murray</name><lb/>
SUBJECT:  Water Window Thickness</opener>

<div2 type="section" n="1">
<head>A. Thermal Column</head>

<p>The position of the window relative to the thermal column and nearest<lb/>
exposure port is shown below:<lb/>
<table>
<row>
<cell><seg><xref id="reactorlg/MurNBwindow041751aa.jpg" rend="new">
<figure entity="MurNBwindow041751aa"></figure></xref></seg></cell>
</row>
</table></p>
<p>To obtain the order of magnitude of radiation at the window scattered<lb/>
from the thermal beam, a calculation of the flux at the point P (see figure<lb/>
above) was made.
</p>
<p>The flux at this point due to the scattering from a volume d&#x03C3;d&#x03C7; is<lb/>
given by<lb/>

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<lb/>
in which we have taken the probability of the neutron reaching P after<lb/>
scattering to be unity. This is realistic in that the mean free path in<lb/>
air for the neutron is several thousand centimeters. Also &#x03C6; is considered<lb/>
constant along &#x03C7;. This is a good approximation and is on the safe side.
</p>
<p>The above equation can be written as<lb/>

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</p>
<pb n="2"/>
<p><seg><xref id="reactorlg/MurNBwindow041751b.jpg" rend="new">
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<p>
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                          <mi>o</mi>
                        </mrow>
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          <mo>]</mo>
        </mrow>
        <mrow>
          <mn>0</mn>
        </mrow>
        <mrow>
          <msub>
            <mrow>
              <mi>R</mi>
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            <mrow>
              <mi>o</mi>
            </mrow>
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          <mi>s</mi>
          <mi>&alpha;</mi>
        </mrow>
      </msubsup>
    </mrow>
  </mrow>
</m:math>
-->
</formula></hi>
<lb/>
<seg rend='left'><figure entity="MurNBwindow041751form4"></figure></seg>
<hi rend="suppress"><formula notation="mathml"><!--
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          <mi>&alpha;</mi>
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-->
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</p>
<p>Assuming that the increase in the &#x03C6;s contribution on the left of the<lb/>
center line in beam will nearly be compensated by decrease on the right, we<lb/>
may <orig reg="integrate">intergrate</orig> d&#x03C3; directly, giving<lb/>

<seg rend='left'><figure entity="MurNBwindow041751form5"></figure></seg>
<hi rend="suppress"><formula notation="mathml"><!--
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          <mi>A</mi>
          <mi>&phi;</mi>
          <mi>&Sigma;</mi>
          <mi>s</mi>
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          <mi>&pi;</mi>
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          <mi>s</mi>
          <mi>i</mi>
          <mi>n</mi>
          <mi>&alpha;</mi>
        </mrow>
      </mfrac>
    </mrow>
  </mrow>
</m:math>
-->
</formula></hi>
</p>
<p>The average number of atoms will be<lb/>

<seg rend='left'><figure entity="MurNBwindow041751form6"></figure></seg>
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      <mo>=</mo>
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          <mn>0</mn>
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          <mn>2</mn>
          <mn>9</mn>
          <mi>&thinsp;</mi>
          <mi>&thinsp;</mi>
          <mi>&thinsp;</mi>
          <mi>&thinsp;</mi>
          <mi>&thinsp;</mi>
          <mn>6</mn>
          <mn>.</mn>
          <mn>0</mn>
          <mn>3</mn>
          <mi>&thinsp;</mi>
          <mo>&times;</mo>
          <msup>
            <mrow>
              <mn>1</mn>
              <mn>0</mn>
            </mrow>
            <mrow>
              <mn>2</mn>
              <mn>3</mn>
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          </msup>
        </mrow>
        <mrow>
          <mn>1</mn>
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          <mn>.</mn>
          <mn>5</mn>
        </mrow>
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    </mrow>
  </mrow>
</m:math>
-->
</formula></hi>
<lb/>
=  0.89 x 6 x 10<hi rend="sup">19</hi> = 5.4 x 10<hi rend="sup">19</hi><lb/>

and since the weighted (O and N) thermal scattering cross-section is<lb/>
about 9 x 10<hi rend="sup">-24</hi> cm<hi rend="sup">2</hi>, we have<lb/>

&#x03A3;s = 4.9 x 10<hi rend='sup'>-4</hi>
</p>
<p>Assuming a 4' x 4' beam with a flux of 10<hi rend="sup">7</hi> m/cm<hi rend="sup">2</hi>sec and R<hi rend="sub">o</hi> = 19' we have<lb/>
at a point 7' from the edge of window a flux of<lb/>

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      <msub>
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</formula></hi>
<lb/>
=  2.5 x 10<hi rend="sup">4</hi> m/cm<hi rend="sup">2</hi>sec
</p>
<p>The above value is based upon calculations assuming a collimated bean.<lb/>
This will not be exactly true. For a bean which is not collimated we can<lb/>
write<lb/>

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        </mrow>
        <mrow>
          <mn>1</mn>
          <mn>2</mn>
          <mn>.</mn>
          <mn>6</mn>
          <mrow>
            <msup>
              <mrow>
                <mrow>
                  <mo>(</mo>
                  <mn>1</mn>
                  <mn>9</mn>
                  <mo>)</mo>
                </mrow>
              </mrow>
              <mrow>
                <mn>2</mn>
              </mrow>
            </msup>
            <mn>9</mn>
            <mn>0</mn>
            <mn>0</mn>
          </mrow>
        </mrow>
      </mfrac>
      <mi>&thinsp;</mi>
      <mo>=</mo>
      <mi>&thinsp;</mi>
      <mfrac>
        <mrow>
          <mn>1</mn>
          <mn>0</mn>
          <mn>7</mn>
        </mrow>
        <mrow>
          <mn>2</mn>
          <mn>8</mn>
          <mn>0</mn>
        </mrow>
      </mfrac>
    </mrow>
  </mrow>
</m:math>
-->
</formula></hi>
<lb/>
= 3.5 x 10<hi rend="sup">4</hi> n/cm<hi rend="sup">2</hi>sec.
</p>
<p>The correct value will be somewhere between the two. Assuming the<lb/>
larger value to be correct and a tolerance of 1000 n/sec cm<hi rend="sup">2</hi> for thermal<lb/>
neutrons, the window thickness should be given by<lb/>

<seg rend='left'><figure entity="MurNBwindow041751form9"></figure></seg>
<hi rend="suppress"><formula notation="mathml"><!--
<m:math xmlns='http://www.w3.org/1998/Math/MathML' xmlns:m='http://www.w3.org/1998/Math/MathML' >
  <mrow>
    <mrow fontstyle='normal'>
      <msup>
        <mrow>
          <mi>e</mi>
        </mrow>
        <mrow>
          <mi>x</mi>
          <mo>/</mo>
          <mn>2</mn>
          <mn>.</mn>
          <mn>8</mn>
          <mn>5</mn>
        </mrow>
      </msup>
      <mo>=</mo>
      <mfrac>
        <mrow>
          <mn>3</mn>
          <mn>.</mn>
          <mn>5</mn>
          <mo>&times;</mo>
          <msup>
            <mrow>
              <mn>1</mn>
              <mn>0</mn>
            </mrow>
            <mrow>
              <mn>4</mn>
            </mrow>
          </msup>
        </mrow>
        <mrow>
          <mn>1</mn>
          <mn>0</mn>
          <mn>0</mn>
          <mn>0</mn>
        </mrow>
      </mfrac>
    </mrow>
  </mrow>
</m:math>
-->
</formula></hi>
<lb/>
This leads to a thickness of<lb/>

x = 10cm.
</p>
</div2>
<pb n="3"/>
<div2 type="image" n="1">
<p><seg><xref id="reactorlg/MurNBwindow041751c.jpg" rend="new">
<figure entity="MurNBwindow041751c"></figure></xref></seg></p>
</div2>
<div2 type="section" n="2">
<head>B. Experimental Port</head>

<p>At the experimental ports when open there will be a collimated flux of<lb/>
2 x l0<hi rend="sup">8</hi> n/cm<hi rend="sup">2</hi>sec for fast neutrons and 1.2 x 10<hi rend="sup">7</hi> n/cm<hi rend="sup">2</hi>sec. slow neutrons.<lb/>
Substituting in the first equation with A = 180 cm<hi rend="sup">2</hi> and &#x03A3;s = 5.4 x 10<hi rend="sup">-3</hi><lb/>

<seg rend='left'><figure entity="MurNBwindow041751form10"></figure></seg>
<hi rend="suppress"><formula notation="mathml"><!--
<m:math xmlns='http://www.w3.org/1998/Math/MathML' xmlns:m='http://www.w3.org/1998/Math/MathML' >
  <mrow>
    <mrow fontstyle='normal'>
      <msub>
        <mrow>
          <mi>&phi;</mi>
        </mrow>
        <mrow>
          <mi>s</mi>
        </mrow>
      </msub>
      <mo>=</mo>
      <mfrac>
        <mrow>
          <mrow>
            <mo>(</mo>
            <mn>1</mn>
            <mn>8</mn>
            <mn>0</mn>
            <mo>)</mo>
            <mrow>
              <mo>(</mo>
              <mn>2</mn>
              <mo>&times;</mo>
              <msup>
                <mrow>
                  <mn>1</mn>
                  <mn>0</mn>
                </mrow>
                <mrow>
                  <mn>8</mn>
                </mrow>
              </msup>
              <mo>)</mo>
              <mrow>
                <mo>(</mo>
                <mn>5</mn>
                <mn>.</mn>
                <mn>4</mn>
                <mo>&times;</mo>
                <msup>
                  <mrow>
                    <mn>1</mn>
                    <mn>0</mn>
                  </mrow>
                  <mrow>
                    <mo>-</mo>
                    <mn>5</mn>
                  </mrow>
                </msup>
                <mo>)</mo>
              </mrow>
            </mrow>
          </mrow>
        </mrow>
        <mrow>
          <mrow>
            <mo>(</mo>
            <mn>1</mn>
            <mn>2</mn>
            <mn>.</mn>
            <mn>6</mn>
            <mo>)</mo>
            <mrow>
              <mo>(</mo>
              <mn>5</mn>
              <mn>7</mn>
              <mn>0</mn>
              <mo>)</mo>
              <mrow>
                <mo>(</mo>
                <mn>0</mn>
                <mn>.</mn>
                <mn>3</mn>
                <mn>7</mn>
                <mo>)</mo>
              </mrow>
            </mrow>
          </mrow>
        </mrow>
      </mfrac>
    </mrow>
  </mrow>
</m:math>
-->
</formula></hi>
<lb/>
= 720 n/cm<hi rend="sup">2</hi>sec
</p>
<p>Since H<hi rend="sub">2</hi>0 is comparable to Portland cement in attenuation of fast<lb/>
neutrons, a 6" window will reduce the fast neutron component below tolerance.<lb/>
</p>
<p>The slow neutron flux at the window will be given by<lb/>

<seg rend='left'><figure entity="MurNBwindow041751form11"></figure></seg>
<hi rend="suppress"><formula notation="mathml"><!--
<m:math xmlns='http://www.w3.org/1998/Math/MathML' xmlns:m='http://www.w3.org/1998/Math/MathML' >
  <mrow>
    <mrow fontstyle='normal'>
      <msub>
        <mrow>
          <mi>&phi;</mi>
        </mrow>
        <mrow>
          <mi>s</mi>
        </mrow>
      </msub>
      <mo>=</mo>
      <mfrac>
        <mrow>
          <mi>A</mi>
          <mi>&phi;</mi>
          <mi>&Sigma;</mi>
          <mi>s</mi>
        </mrow>
        <mrow>
          <mn>4</mn>
          <mi>&pi;</mi>
          <msub>
            <mrow>
              <mi>R</mi>
            </mrow>
            <mrow>
              <mi>o</mi>
            </mrow>
          </msub>
          <mi>s</mi>
          <mi>i</mi>
          <mi>n</mi>
          <mi>&alpha;</mi>
        </mrow>
      </mfrac>
      <mo>=</mo>
      <mfrac>
        <mrow>
          <mrow>
            <mo>(</mo>
            <mn>1</mn>
            <mn>8</mn>
            <mn>0</mn>
            <mo>)</mo>
            <mrow>
              <mo>(</mo>
              <msup>
                <mrow>
                  <mn>1</mn>
                  <mn>0</mn>
                </mrow>
                <mrow>
                  <mn>9</mn>
                </mrow>
              </msup>
              <mo>)</mo>
              <mrow>
                <mo>(</mo>
                <mn>4</mn>
                <mn>.</mn>
                <mn>9</mn>
                <mo>&times;</mo>
                <msup>
                  <mrow>
                    <mn>1</mn>
                    <mn>0</mn>
                  </mrow>
                  <mrow>
                    <mo>-</mo>
                    <mn>4</mn>
                  </mrow>
                </msup>
                <mo>)</mo>
              </mrow>
            </mrow>
          </mrow>
        </mrow>
        <mrow>
          <mrow>
            <mo>(</mo>
            <mn>1</mn>
            <mn>2</mn>
            <mn>.</mn>
            <mn>6</mn>
            <mo>)</mo>
            <mrow>
              <mo>(</mo>
              <mn>5</mn>
              <mn>7</mn>
              <mn>0</mn>
              <mo>)</mo>
              <mrow>
                <mo>(</mo>
                <mn>0</mn>
                <mn>.</mn>
                <mn>3</mn>
                <mn>7</mn>
                <mo>)</mo>
              </mrow>
            </mrow>
          </mrow>
        </mrow>
      </mfrac>
    </mrow>
  </mrow>
</m:math>
-->
</formula></hi>
<lb/>
&#x2243; 3.25 x 10<hi rend="sup">4</hi> n/cm<hi rend="sup">2</hi>sec.<lb/>

Adding to this the fast neutron flux which has been assumed thermalized<lb/>
gives a window thickness as before of ~ 10 cm.
</p>
<p>To be completely safe it is believed a window of 6 inches should be<lb/>
used with Borax added to enhance slow neutron absorption as well as some<lb/>
fast.
</p>
</div2>
</div1>
</body>
</text>
</TEI.2>
