Energy Calibration of the NewSUBARU Storage Ring for Laser Compton-Scattering Gamma Rays and Applications

H. Utsunomiya, Tatsushi Shima, Keiji Takahisa, D. Filipescu, O. Teşileanu, I. Gheorghe, Hilde-Therese Nyhus, Y.-W. Lui, Yasuhisa Kitagawa, Sho Amano,

IEEE Transactions on Nuclear Science · 2014 · 47 citations · 13 references

Concepts

Abstract

Using γ-ray beams produced in the inverse Compton scattering between CO <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">2</sub> laser photons and relativistic electrons, we have calibrated electron beam energies in the nominal energy range 550-974 MeV at the synchrotron radiation facility New-SUBARU. The laser Compton-scattering (LCS) γ-ray beams were produced at energies from 561 to 1728 keV and detected with a high-purity germanium detector. The electron beam energies were determined by reproducing the full energy peaks of the γ-ray beams by Monte Carlo simulations. The accuracy of the calibration is (5.5 - 9.4) ×10 <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">- 5</sup> . The reproducibility of the electron beam energy is excellent in an independent injection and deceleration. The present energy calibration of the electron beams offers a standard for the energy calibration of high-energy LCS γ-ray beams produced with a Nd:YVO <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">4</sub> laser. As applications of the energy calibration, we investigated the energy linearity of a 3.5 <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">''</sup> × 4.0 <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">''</sup> LaBr <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3</sub> (Ce) detector in the response to γ-rays at energies up to 10 MeV and the energy profile of the high-energy LCS γ-ray beams.

References

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