Abstract
A procedure for and the results from the energy calibration of a ΔE-E scintillation telescope used in experiments performed at the INR to study the nd-breakup reaction are described. The telescope was calibrated using a beam of α particles with an energy of 30 MeV of the U-120 cyclotron (INP). Secondary protons from the 10,11B(α, p) reaction were recorded by the ΔE-E telescope at several recording angles and with the application of different absorbing foils. The calibration results from the ΔE-E telescope were obtained over the interval E p = 10–30 MeV, allowing us to measure the energies of secondary protons in the ndbreakup reaction when the energy of primary neutrons is 20–60 MeV.
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Original Russian Text © S.V. Zuev, E.S. Konobeevskii, V.M. Lebedev, M.V. Mordovskoi, A.V. Spasskii, S.I. Potashev, I.M. Sharapov, 2012, published in Izvestiya Rossiiskoi Akademii Nauk. Seriya Fizicheskaya, 2012, Vol. 76, No. 4, pp. 453–455.
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Zuev, S.V., Konobeevskii, E.S., Lebedev, V.M. et al. Energy calibration of a ΔE-E scintillation telescope in (α, p) reaction. Bull. Russ. Acad. Sci. Phys. 76, 396–399 (2012). https://doi.org/10.3103/S1062873812040387
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DOI: https://doi.org/10.3103/S1062873812040387