<?xml version="1.0" encoding="UTF-8"?>
<xml>
  <records>
    <record>
       <contributors>
          <authors>
             <author>Yi, H.</author>
             <author>Wang, X.F.</author>
             <author>Yang, X.M.</author>
             <author>Zhang, W.Q.</author>
          </authors>
       </contributors>
       <titles>
          <title>
             Heating Estimation of Undulator Vacuum Chamber at S3FEL
          </title>
       </titles>
       <publisher>JACoW Publishing</publisher>
       <pub-location>Geneva, Switzerland</pub-location>
		 <isbn>978-3-95450-265-3</isbn>
		 <electronic-resource-num>10.18429/JACoW-SAP2023-TUPB033</electronic-resource-num>
		 <language>English</language>
		 <pages>151-154</pages>
       <keywords>
          <keyword>electron</keyword>
          <keyword>wakefield</keyword>
          <keyword>vacuum</keyword>
          <keyword>undulator</keyword>
          <keyword>impedance</keyword>
       </keywords>
       <work-type>Contribution to a conference proceedings</work-type>
       <dates>
          <year>2024</year>
          <pub-dates>
             <date>2024-11</date>
          </pub-dates>
       </dates>
       <urls>
          <related-urls>
              <url>https://doi.org/10.18429/JACoW-SAP2023-TUPB033</url>
              <url>https://jacow.org/sap2023/papers/tupb033.pdf</url>
          </related-urls>
       </urls>
       <abstract>
          Heating of the vacuum chambers are unavoidable when electron beams pass through the chamber channels at relativistic speeds. In the undulator vacuum chambers, such effects might lead to temperature increase of the magnets and eventually cause degradations in the FEL lasing process. Thus, in this paper, the heating of the undulator vacuum chambers at S3FEL due to wake field effects and spontaneous synchrotron radiation are estimated using an analytical approach. For the wake field effects, the contribution from finite conductivity of the vacuum chamber material and from the inner surface roughness are considered. A electron beam profile from a start-to-end simulation is used to calculate the total wake field and the induced heat. For the synchrotron radiation, a simple analytical expression is used.
       </abstract>
    </record>
  </records>
</xml>
