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High brightness gamma-ray production at Fermilab Accelerator Science and Technology (FAST) facility
Author(s) -
D. Mihalcea,
Bryce Jacobson,
A. Murokh,
P. Piot,
J. Ruan
Publication year - 2017
Publication title -
aip conference proceedings
Language(s) - English
Resource type - Conference proceedings
eISSN - 1551-7616
pISSN - 0094-243X
DOI - 10.1063/1.4975900
Subject(s) - thermal emittance , physics , brightness , photon , compton scattering , particle accelerator , fermilab , cathode ray , beam emittance , gamma ray , radiation , electron , synchrotron radiation , optics , beam (structure) , nuclear physics
Electron beams with energies of the order of a few 100's of MeV and low transverse emittance, in combination with powerful infrared lasers, allow for the production of high quality gamma rays through Inverse Compton Scattering (ICS). At Fermilab Accelerator Science and Technology (FAST) facility, a 300 MeV beam will be used to generate gamma rays with maximum photon energies of up to ~1.5 MeV and brightness of the order of 10 21 photons/[s-(mm-mrad) 2- 0.1%BW]. Due to the low electron-beam transverse emittance, the relative bandwidth of the scattered radiation is expected to be ≤ 1%. A key challenge toward the production of high radiation dose and brightness is to enhance the energy of the infrared 3 ps laser pulses to the joule level. Finally, in this contribution, we present the plans for the experimental setup, along with comprehensive numerical simulations of the ICS process.

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