Nuclear model calculation and targetry recipe for production of 110mIn

2015 ◽  
Vol 104 ◽  
pp. 60-66 ◽  
Author(s):  
T. Kakavand ◽  
M. Mirzaii ◽  
M. Eslami ◽  
A. Karimi
2017 ◽  
Vol 314 (3) ◽  
pp. 1759-1766 ◽  
Author(s):  
Malihe Rostampour ◽  
Mohammadreza Aboudzadeh ◽  
Mahdi Sadeghi ◽  
Saeid Hamidi ◽  
Behroz Alirezapour ◽  
...  

2012 ◽  
Vol 70 (1) ◽  
pp. 257-262 ◽  
Author(s):  
M. Al-Abyad ◽  
A.S. Abdel-Hamid ◽  
F. Tárkányi ◽  
F. Ditrói ◽  
S. Takács ◽  
...  

Radiocarbon ◽  
2019 ◽  
Vol 61 (5) ◽  
pp. 1135-1142 ◽  
Author(s):  
Walter Kutschera

ABSTRACTThe half-life of radiocarbon (14C) is 5700 ± 30 yr, which makes it particularly useful for dating in archaeology. However, only an exceptional hindrance of the beta decay from 14C to 14N—a so-called Gamow-Teller ß-decay—makes this half-life so long. A normal strength would result in a half-life of only a few days, completely useless for archaeological dating. The unusual hindrance is based on the nuclear structure of the two nuclei, resulting in strongly destructive interferences of the nuclear transition matrix element. Nuclear model calculation with great computational efforts have been performed in the literature to reproduce the very low transition probability. Here, we will attempt to describe the nuclear physics behind this most unusual half-life.


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