1986 ◽  
Vol 93 (1-4) ◽  
pp. 193-196 ◽  
Author(s):  
Abdulhahid A. Hasan ◽  
Sümer Şahin ◽  
Chien Chung

1968 ◽  
Vol 173 (4) ◽  
pp. 1159-1165 ◽  
Author(s):  
A. A. Delucchi ◽  
A. E. Greendale ◽  
P. O. Strom

2020 ◽  
Vol 163 ◽  
pp. 249-260
Author(s):  
B.D. Pierson ◽  
L.R. Greenwood ◽  
S.C. Stave ◽  
J.T. Burke ◽  
S.W. Padgett ◽  
...  

2019 ◽  
Vol 155 ◽  
pp. 86-97 ◽  
Author(s):  
B.D. Pierson ◽  
A.M. Prinke ◽  
L.R. Greenwood ◽  
S.C. Stave ◽  
R.S. Wittman ◽  
...  

1960 ◽  
Vol 10 ◽  
pp. 677-679 ◽  

1. p. SELINOV: Anomalous abundances of Te and Xe isotopes in meteorites and in the Earth permit us to draw some conclusions concerning the age of uranium and the processes of nucleogenesis. According to the estimate by Hoyle the amount of 254Cf disintegrated during a super-nova outburst is of the order of io29 g or io~4 of the stellar mass. According to the fission-yield curve the isotopes of Te comprise about 1 % of the mass of fission products. The abundances of Te 128-131 are anomalously high, due to the fission of heavy nuclei. The element abundances do not permit us to draw any conclusions about the r-process. The isotopes of Te and Xe with even mass numbers give evidence in favour of the r-process (anomalously high abundances). But the amount of Te in meteorites and in Earth is about 1000 times less than it should be if formed during the outburst. The Sikhote- Alin meteorite shows the same anomaly. We may conclude that the heavy elements of the solar system have been formed not in a single super-nova outburst, but as a result of mixing from the totality of outbursts. According to Hoyle, this gives a definite estimate for the age of uranium.


2018 ◽  
Vol 4 ◽  
pp. 26 ◽  
Author(s):  
Brieuc Voirin ◽  
Grégoire Kessedjian ◽  
Abdelaziz Chebboubi ◽  
Sylvain Julien-Laferrière ◽  
Olivier Serot

Studies on fission yields have a major impact on the characterization and the understanding of the fission process and are mandatory for reactor applications. Fission yield evaluation represents the synthesis of experimental and theoretical knowledge to perform the best estimation of mass, isotopic and isomeric yields. Today, the output of fission yield evaluation is available as a function of isotopic yields. Without the explicitness of evaluation covariance data, mass yield uncertainties are greater than those of isotopic yields. This is in contradiction with experimental knowledge where the abundance of mass yield measurements is dominant. These last years, different covariance matrices have been suggested but the experimental part of those are neglected. The collaboration between the LPSC Grenoble and the CEA Cadarache starts a new program in the field of the evaluation of fission products in addition to the current experimental program at Institut Laue-Langevin. The goal is to define a new methodology of evaluation based on statistical tests to define the different experimental sets in agreement, giving different solutions for different analysis choices. This study deals with the thermal neutron induced fission of 235U. The mix of data is non-unique and this topic will be discussed using the Shannon entropy criterion in the framework of the statistical methodology proposed.


Author(s):  
F. TOVESSON ◽  
C. W. ARNOLD ◽  
T. BREDEWEG ◽  
M. JANDEL ◽  
A. B. LAPTEV ◽  
...  
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