Author: Franck, C.
Paper Title Page
THPAB009 A Hard X-Ray Compton Source at CBETA 3765
 
  • K.E. Deitrick, C. Franck, G.H. Hoffstaetter
    Cornell University (CLASSE), Cornell Laboratory for Accelerator-Based Sciences and Education, Ithaca, New York, USA
  • J. Crone, H.L. Owen
    UMAN, Manchester, United Kingdom
  • G.A. Krafft
    JLab, Newport News, Virginia, USA
  • G.A. Krafft, B. Terzić
    ODU, Norfolk, Virginia, USA
  • B.D. Muratori, P.H. Williams
    STFC/DL/ASTeC, Daresbury, Warrington, Cheshire, United Kingdom
  • B.D. Muratori, P.H. Williams
    Cockcroft Institute, Warrington, Cheshire, United Kingdom
  
  In­verse Comp­ton scat­ter­ing (ICS) holds the po­ten­tial for fu­ture high flux, nar­row band­width x-ray sources dri­ven by high qual­ity, high rep­e­ti­tion rate elec­tron beams. CBETA, the Cor­nell-BNL En­ergy re­cov­ery linac (ERL) Test Ac­cel­er­a­tor, is the world’s first su­per­con­duct­ing ra­diofre­quency multi-turn ERL, with a max­i­mum en­ergy of 150 MeV, ca­pa­ble of ICS pro­duc­tion of x-rays above 400 keV. We pre­sent an up­date on the by­pass de­sign and an­tic­i­pated pa­ra­me­ters of a com­pact ICS source at CBETA. X-ray pa­ra­me­ters from the CBETA ICS are com­pared to those of lead­ing syn­chro­tron ra­di­a­tion fa­cil­i­ties, demon­strat­ing that, above a few hun­dred keV, pho­ton beams pro­duced by ICS out­per­form those pro­duced by un­du­la­tors in term of flux and bril­liance.  
DOI • reference for this paper ※ https://doi.org/10.18429/JACoW-IPAC2021-THPAB009  
About • paper received ※ 19 May 2021       paper accepted ※ 06 July 2021       issue date ※ 10 August 2021  
Export • reference for this paper using ※ BibTeX, ※ LaTeX, ※ Text/Word, ※ RIS, ※ EndNote (xml)