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<xml>
  <records>
    <record>
       <contributors>
          <authors>
             <author>Unel, G.</author>
             <author>Adiguzel, A.</author>
             <author>Cetinkaya, H.</author>
             <author>Esen, S.</author>
             <author>Ogur, S.</author>
             <author>Ozcan, E.V.</author>
          </authors>
       </contributors>
       <titles>
          <title>
             Linear Approach to Space Charge Calculations Proton Testbeam at KAHVELab (PTAK)
          </title>
       </titles>
       <publisher>JACoW Publishing</publisher>
       <pub-location>Geneva, Switzerland</pub-location>
       <abstract>
          In Kandilli Detector, Accelerator, and Instrumentation Laboratory, a proton accelerator system is produced using local resources consists of 2 types of ion sources, a low energy beam transfer line (LEBT)and a 1-meter-long RFQ that will operate at 800 MHz. A bespoke Python program calculated the space charge effect created by internal interactions of the beam along the line before entering the RFQ. The results were validated with CERN’s TRAVEL program. The growth of the beam with a 1.4 mA current value in the transverse axis due to the effect of space charge has been calculated with a maximum margin of error of 4% for different current and frequency values. Studies using different emittance calculation methods on emittance growth due to space charge dominance continues to be developed. In addition, studies on comparing new methods’ findings with outputs of A Space Charge Tracking Algorithm (ASTRA) and RF-Track Programs are ongoing and aim to finalize by the end of 2023.
       </abstract>
    </record>
  </records>
</xml>
