<xml>
  <records>
    <record>
       <contributors>
          <authors>
             <author>Liu, S.</author>
             <author>Decking, W.</author>
             <author>Feng, G.</author>
             <author>Geloni, G.</author>
             <author>Kocharyan, V.</author>
             <author>Serkez, S.</author>
             <author>Zagorodnov, I.</author>
          </authors>
       </contributors>
       <titles>
          <title>
             Longitudinal Phase Space Optimization for the Hard X-ray Self-Seeding
          </title>
       </titles>
		 <publisher>JACoW</publisher>
       <pub-location>Geneva, Switzerland</pub-location>
		 <isbn>978-3-95450-179-3</isbn>
		 <electronic-resource-num>10.18429/JACoW-FEL2017-TUP004</electronic-resource-num>
		 <language>English</language>
		 <pages>259-262</pages>
       <pages>TUP004</pages>
       <keywords>
          <keyword>ion</keyword>
          <keyword>FEL</keyword>
          <keyword>simulation</keyword>
          <keyword>undulator</keyword>
          <keyword>electron</keyword>
       </keywords>
       <work-type>Contribution to a conference proceedings</work-type>
       <dates>
          <year>2018</year>
          <pub-dates>
             <date>2018-02</date>
          </pub-dates>
       </dates>
       <urls>
          <related-urls>
              <url>https://doi.org/10.18429/JACoW-FEL2017-TUP004</url>
              <url>http://jacow.org/fel2017/papers/tup004.pdf</url>
          </related-urls>
       </urls>
       <abstract>
          For the implementation of Hard X-ray Self-Seeding (HXRSS) at European XFEL, short electron-beam bunches (FWHM ≤ 50 fs) are preferred to mitigate spatio-temperal coupling effect and to fit to the seeding bump width. Therefore, operations with low charges (&lt; 250 pC) are preferred. Longitudinal phase-space optimization has been performed for the 100 pC case by flattening the current distribution. Start-to-end simulations show that, with the optimized distribution, for the photon energy of 14.4 keV, the HXRSS output power, pulse energy and spectral intensity can be increased by a factor of approximately 2 as compared to the nominal working point.
       </abstract>
    </record>
  </records>
</xml>
