• Title of article

    Photon flux and spectrum of Compton sources

  • Author/Authors

    Petrillo، نويسنده , , V. and Bacci، نويسنده , , A. and Ben Alى Zinati، نويسنده , , R. and Chaikovska، نويسنده , , I. and Curatolo، نويسنده , , C. M. Ferrario، نويسنده , , M. and Maroli، نويسنده , , C. and Ronsivalle، نويسنده , , C. and Rossi، نويسنده , , A.R. and Serafini، نويسنده , , L. and Tomassini، نويسنده , , P. and Vaccarezza، نويسنده , , C. and Variola، نويسنده , , A.، نويسنده ,

  • Pages
    8
  • From page
    109
  • To page
    116
  • Abstract
    We analyze the characteristics of the γ radiation produced by Compton back-scattering of a high brightness electron beam produced by a photoinjector and accelerated in a linac up to energies of 360–720 MeV and a laser operated at about 500 nm, by comparing classical and quantum models and codes. The interaction produces γ rays in the range 4.9–18.8 MeV. In view of the application to nuclear resonance fluorescence a relative bandwidth of few 10 − 3 is needed. The bandwidth is reduced by taking advantage of the frequency–angular correlation typical of the phenomenon and selecting the radiation in an angle of tens of μ rads . The foreseen spectral density is 20–6 photons per eV in a single shot, a number that can be increased by developing multi-bunch techniques and laser recirculation. In this way a final value of 10 4 photon per eV per second can be achieved.
  • Keywords
    Compton back scattering , ? Source
  • Journal title
    Astroparticle Physics
  • Record number

    2019872