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The $$gamma$$SF method

$$gamma$$線強度関数法

宇都宮 弘章*; Goriely, S.*; 秋宗 秀俊*; 山形 民穂*; 近藤 壮雄*; 岩本 ちひろ*; 岡本 明之*; 原田 秀郎   ; 北谷 文人  ; 後神 進史*; 豊川 弘之*; 山田 家和勝*; Lui, Y.-W.*; Hilaire, S.*; Koning, A. J.*

Utsunomiya, Hiroaki*; Goriely, S.*; Akimune, Hidetoshi*; Yamagata, Tamio*; Kondo, Takeo*; Iwamoto, Chihiro*; Okamoto, Akiyuki*; Harada, Hideo; Kitatani, Fumito; Goko, Shinji*; Toyokawa, Hiroyuki*; Yamada, Kawakatsu*; Lui, Y.-W.*; Hilaire, S.*; Koning, A. J.*

The $$gamma$$-ray strength function ($$gamma$$SF) interconnects radiative neutron capture and photoneutron emission as a common ingredient in the statistical model. Outlined here is an indirect method of determining radiative neutron-capture cross sections for unstable nuclei based on the $$gamma$$-ray strength function. Application examples of the $$gamma$$SF method are demonstrated.

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分野:Astronomy & Astrophysics

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