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On Monitoring on the Under-Development \({\gamma}\) Source Based on Backward Compton Scattering for Photonuclear Research at \(\boldsymbol{E}_{{\gamma}}\boldsymbol{\leq 40}\) MeV

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Moscow University Physics Bulletin Aims and scope

Abstract

Proceeding from the comparison of parameters for the \(\gamma\)-ray source based on backward Compton scattering, which is under development now, and the known methods of monitoring \(\gamma\)-ray beams themselves to monitor the intensity and energy spectrum of \(\gamma\) quanta in the beams from this \(\gamma\)-ray source during photonicuclear research in the energy range from a few megaelectronvolts to \(\sim\)40 MeV, a system comprising scintillation plastic and inorganic detectors, as well as a magnetic pair spectrometer, has been proposed.

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Funding

This work was supported by the National Center for Physics and Mathematics (NCPM) project no. 6 ‘‘Nuclear and Radiation Physics,’’ direction 6.5.1.

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Correspondence to L. Z. Dzhilavyan.

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Belyshev, S.S., Varlamov, V.V., Dzhilavyan, L.Z. et al. On Monitoring on the Under-Development \({\gamma}\) Source Based on Backward Compton Scattering for Photonuclear Research at \(\boldsymbol{E}_{{\gamma}}\boldsymbol{\leq 40}\) MeV. Moscow Univ. Phys. 78, 278–283 (2023). https://doi.org/10.3103/S0027134923030037

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  • DOI: https://doi.org/10.3103/S0027134923030037

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