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A spectrometer for ultrashort gamma-ray pulses with photon energies greater than 10 MeV.
Behm, K T; Cole, J M; Joglekar, A S; Gerstmayr, E; Wood, J C; Baird, C D; Blackburn, T G; Duff, M; Harvey, C; Ilderton, A; Kuschel, S; Mangles, S P D; Marklund, M; McKenna, P; Murphy, C D; Najmudin, Z; Poder, K; Ridgers, C P; Sarri, G; Samarin, G M; Symes, D; Warwick, J; Zepf, M; Krushelnick, K; Thomas, A G R.
Affiliation
  • Behm KT; Center for Ultrafast Optical Science, University of Michigan, Ann Arbor, Michigan 48109-2099, USA.
  • Cole JM; The John Adams Institute for Accelerator Science, Imperial College London, London SW7 2AZ, United Kingdom.
  • Joglekar AS; Physics and Astronomy, University of California, Los Angeles, Los Angeles, California 90095, USA.
  • Gerstmayr E; The John Adams Institute for Accelerator Science, Imperial College London, London SW7 2AZ, United Kingdom.
  • Wood JC; The John Adams Institute for Accelerator Science, Imperial College London, London SW7 2AZ, United Kingdom.
  • Baird CD; York Plasma Institute, Department of Physics, University of York, York YO10 5DD, United Kingdom.
  • Blackburn TG; Department of Physics, Chalmers University of Technology, SE-41296 Gothenburg, Sweden.
  • Duff M; SUPA Department of Physics, University of Strathclyde, Glasgow G4 0NG, United Kingdom.
  • Harvey C; Department of Physics, Chalmers University of Technology, SE-41296 Gothenburg, Sweden.
  • Ilderton A; Department of Physics, Chalmers University of Technology, SE-41296 Gothenburg, Sweden.
  • Kuschel S; Institut für Optik und Quantenelektronik, Friedrich-Schiller-Universität, 07743 Jena, Germany.
  • Mangles SPD; The John Adams Institute for Accelerator Science, Imperial College London, London SW7 2AZ, United Kingdom.
  • Marklund M; Department of Physics, Chalmers University of Technology, SE-41296 Gothenburg, Sweden.
  • McKenna P; SUPA Department of Physics, University of Strathclyde, Glasgow G4 0NG, United Kingdom.
  • Murphy CD; York Plasma Institute, Department of Physics, University of York, York YO10 5DD, United Kingdom.
  • Najmudin Z; The John Adams Institute for Accelerator Science, Imperial College London, London SW7 2AZ, United Kingdom.
  • Poder K; The John Adams Institute for Accelerator Science, Imperial College London, London SW7 2AZ, United Kingdom.
  • Ridgers CP; York Plasma Institute, Department of Physics, University of York, York YO10 5DD, United Kingdom.
  • Sarri G; School of Mathematics and Physics, The Queen's University of Belfast, BT7 1NN Belfast, United Kingdom.
  • Samarin GM; School of Mathematics and Physics, The Queen's University of Belfast, BT7 1NN Belfast, United Kingdom.
  • Symes D; Central Laser Facility, Rutherford Appleton Laboratory, Didcot OX11 0QX, United Kingdom.
  • Warwick J; School of Mathematics and Physics, The Queen's University of Belfast, BT7 1NN Belfast, United Kingdom.
  • Zepf M; Institut für Optik und Quantenelektronik, Friedrich-Schiller-Universität, 07743 Jena, Germany.
  • Krushelnick K; Center for Ultrafast Optical Science, University of Michigan, Ann Arbor, Michigan 48109-2099, USA.
  • Thomas AGR; Center for Ultrafast Optical Science, University of Michigan, Ann Arbor, Michigan 48109-2099, USA.
Rev Sci Instrum ; 89(11): 113303, 2018 Nov.
Article in En | MEDLINE | ID: mdl-30501337
ABSTRACT
We present a design for a pixelated scintillator based gamma-ray spectrometer for non-linear inverse Compton scattering experiments. By colliding a laser wakefield accelerated electron beam with a tightly focused, intense laser pulse, gamma-ray photons up to 100 MeV energies and with few femtosecond duration may be produced. To measure the energy spectrum and angular distribution, a 33 × 47 array of cesium-iodide crystals was oriented such that the 47 crystal length axis was parallel to the gamma-ray beam and the 33 crystal length axis was oriented in the vertical direction. Using an iterative deconvolution method similar to the YOGI code, modeling of the scintillator response using GEANT4 and fitting to a quantum Monte Carlo calculated photon spectrum, we are able to extract the gamma ray spectra generated by the inverse Compton interaction.

Full text: 1 Collection: 01-internacional Database: MEDLINE Language: En Journal: Rev Sci Instrum Year: 2018 Document type: Article Affiliation country: United States

Full text: 1 Collection: 01-internacional Database: MEDLINE Language: En Journal: Rev Sci Instrum Year: 2018 Document type: Article Affiliation country: United States