<xml>
  <records>
    <record>
       <contributors>
          <authors>
             <author>Kubo, T.</author>
          </authors>
       </contributors>
       <titles>
          <title>
             Model of Flux Trapping in Cooling Down Process
          </title>
       </titles>
		 <publisher>JACoW</publisher>
       <pub-location>Geneva, Switzerland</pub-location>
		 <isbn>978-3-95450-178-6</isbn>
		 <electronic-resource-num>10.18429/JACoW-SRF2015-MOPB009</electronic-resource-num>
		 <language>English</language>
		 <pages>90-94</pages>
       <pages>MOPB009</pages>
       <keywords>
          <keyword>target</keyword>
          <keyword>cavity</keyword>
          <keyword>interface</keyword>
          <keyword>experiment</keyword>
          <keyword>framework</keyword>
       </keywords>
       <work-type>Contribution to a conference proceedings</work-type>
       <dates>
          <year>2015</year>
          <pub-dates>
             <date>2015-12</date>
          </pub-dates>
       </dates>
       <urls>
          <related-urls>
              <url>http://dx.doi.org/10.18429/JACoW-SRF2015-MOPB009</url>
              <url>http://srf2015.vrws.de/papers/mopb009.pdf</url>
          </related-urls>
       </urls>
       <abstract>
          Recent findings that cooling conditions affect an amount of trapped magnetic flux attract much attention as a way to achieve a high-Q0 by SRF cavity*,**,***. Q0~2*10¹¹ has already been achieved by the full flux expulsion****. While much experimental studies have been conducted, not much theoretical progress followed on it. In this paper, I introduce a simple model that can explain how trapped fluxoids are expelled in cooling process.
       </abstract>
    </record>
  </records>
</xml>
