Modificated activation method for measurement of the yield of the astrophysical reactions-Reference-Cited by-同舟云学术

Modificated activation method for measurement of the yield of the astrophysical reactions

Published:2019-01 Issue: Volume:49 Page:1960013
ISSN:2010-1945
Container-title:International Journal of Modern Physics: Conference Series
language:en
Short-container-title:Int. J. Mod. Phys. Conf. Ser.

Author:

Artemov S. V.¹,Igamov S. B.¹,Karakhodzhaev A. A.¹,Tojiboyev O. R.¹,Ergashev F. Kh.¹,Burtebayev N.²³,Kholbaev I.⁴,Rumi R. F.⁴,Eshkobilov Sh. Kh.⁴,Khalikov R. I.⁴

Affiliation:

1. Institute of Nuclear Physics, Academy of Sciences, 100214, Ulugbek, Tashkent, Uzbekistan

2. Institute of Nuclear Physics, ME Republic of Kazakhstan, ul. Ibragimova 1, 050032, Almaty, Kazakhstan

3. Kazakh National University, ul. al-Farabi 71, 050040, Almaty, Kazakhstan

4. Research Institute of Physics of Semiconductors and Microelectronics at the National University of Uzbekistan, ul. Yangi Olmazor 20, 100057, Tashkent, Uzbekistan

Abstract

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.

Publisher

World Scientific Pub Co Pte Lt

Link

https://www.worldscientific.com/doi/pdf/10.1142/S2010194519600139

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