Modificated activation method for measurement of the yield of the astrophysical reactions
S. V. ArtemovInstitute of Nuclear Physics, Academy of Sciences, 100214, Ulugbek, Tashkent, UzbekistanS. B. IgamovInstitute of Nuclear PhysicsА. А. КараходжаевInstitute of Nuclear PhysicsO. R. TojiboyevInstitute of Nuclear PhysicsФ. Х. ЭргашевInstitute of Nuclear Physics, Academy of Sciences, 100214, Ulugbek, Tashkent, UzbekistanN. BurtebayevKazakh National University, ul. al-Farabi 71, 050040, Almaty, KazakhstanI. KholbaevResearch Institute of Physics of Semiconductors and Microelectronics at the National University of Uzbekistan, ul. Yangi Olmazor 20, 100057, Tashkent, UzbekistanR.F. RumiResearch Institute of Physics of Semiconductors and Microelectronics at the National University of Uzbekistan, ul. Yangi Olmazor 20, 100057, Tashkent, UzbekistanSh. Kh. EshkobilovResearch Institute of Physics of Semiconductors and Microelectronics at the National University of Uzbekistan, ul. Yangi Olmazor 20, 100057, Tashkent, UzbekistanR. I. KhalikovResearch Institute of Physics of Semiconductors and Microelectronics at the National University of Uzbekistan, ul. Yangi Olmazor 20, 100057, Tashkent, Uzbekistan
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The original version of the activation method is presented and yield of the astrophysical relevant reaction [Formula: see text] has been measured at the energy region 190–650[Formula: see text]keV using this method. The rate of this reaction was calculated within the temperature region [Formula: see text] through the yield values. The possibility of improving the method for measuring very small yields or cross sections was demonstrated.
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