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 Physics, Academy of Sciences, 100214, Ulugbek, Tashkent, UzbekistanА. А. КараходжаевInstitute of Nuclear Physics, Academy of Sciences, 100214, Ulugbek, Tashkent, UzbekistanO. R. TojiboyevInstitute of Nuclear Physics, Academy of Sciences, 100214, Ulugbek, Tashkent, UzbekistanФ. Х. ЭргашевInstitute of Nuclear Physics, Academy of Sciences, 100214, Ulugbek, Tashkent, UzbekistanN. BurtebayevInstitute of Nuclear Physics, ME Republic of Kazakhstan, ul. Ibragimova 1, 050032, 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
ABI
Annotatsiya
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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