Удаан нейтроноор цэнэгт бөөм үүсэх урвалын астрофизикийн хэрэглээ

Authors

  • Altansukh M
  • Khuukhenkhuu G МУИС, Цөмийн судалгааны төв
  • Chadraabal L МУИС, Цөмийн судалгааны төв
  • Unenbat G МУИС, Цөмийн судалгааны төв

DOI:

https://doi.org/10.22353/physics.v2i125.475

Keywords:

IREN neutron source projected

Abstract

Results of statistical model calculations for average (n,a) cross sections arc compared with experimental values at E=30 keV. Using the results of theoretical calculations for the (n,a) and (n,p) cross sections were proposed new measurement for nuclear astrophysics study on the IREN neutron source projected at the Frank Laboratory of Neutron Physics, JINR, Dubna.

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Published

2022-03-12

How to Cite

[1]
A. M, K. G, C. L, and U. G, “Удаан нейтроноор цэнэгт бөөм үүсэх урвалын астрофизикийн хэрэглээ”, Sci. tran. NUM, Phys., vol. 2, no. 125, pp. 94–96, Mar. 2022.

Issue

Vol. 2 No. 125 (1996): Физик

Section

Research article

License

Copyright (c) 2022 Физик сэтгүүл

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