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JOURNALS // Bulletin of the L.N. Gumilyov Eurasian National University. Physics. Astronomy Series // Archive

Bulletin of the L.N. Gumilyov Eurasian National University. Physics. Astronomy Series, 2019, Volume 127, Issue 2, Pages 8–15 (Mi vepha48)

The emission of secondary protons from reaction (p,xp) at an energy of 30 MeV in the nucleus of $^{103}$Rh

G. Zh. Aliyevaa, G. D. Kabdrakhimovaa, B. M. Sadykovb, M. Nassurllabc, Zh. Mukanbc, G. Ussabaevac, Y. Kucukd, T. K. Zholdybayevcb

a Eurasian National University named after L.N. Gumilyov, Nur-Sultan
b Institute of Nuclear Physics
c Al-Farabi Kazakh National University
d Akdeniz University

Abstract: On the beam of accelerated protons of the U-150M cyclotron of the Institute of Nuclear Physics, double – differential reaction cross sections (p, xp) were measured on a $^{103}$Rh nucleus at an energy E$_p$=30 MeV. A self-sustaining foil with a thickness of 3 $\mu{m}$ with an isotope content of $^{103}$Rh$\sim$98% was used as targets. To identify the reaction products, a two-detector telescope was used, consisting of a transient thin silicon detector with a thickness of 100 $\mu{m}$ and a total absorption detector (CsI (Tl) scintillator) 2.5 cm thick. The integral spectra were obtained from the double – differential cross sections with the subsequent determination of the total partial cross sections for the reactions (p, xp). The experimental results obtained were analyzed in the framework of a modified version of the exciton model of pre-equilibrium decay within the PRECO-2006 calculation code. It has been established that the cross sections for the reactions $^{103}$Rh (p, xp) at a proton energy of 30 MeV are predominantly formed by the mechanism of pre-equilibrium decay.

Received: 25.04.2019

DOI: 10.32523/2616-68-36-2019-127-2-8-15



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