A model for calculating the angular momentum distribution of fission fragments

1969 ◽  
Vol 136 (2) ◽  
pp. 465-480 ◽  
Author(s):  
J.O. Rasmussen ◽  
W. Nörenberg ◽  
H.J. Mang
2014 ◽  
Vol 118 ◽  
pp. 230-232
Author(s):  
I. Stetcu ◽  
P. Talou ◽  
T. Kawano ◽  
M. Jandel

2002 ◽  
Vol 3 (1) ◽  
pp. 95-98 ◽  
Author(s):  
I. ^|^Ouml;zkan ◽  
Z. B^|^uuml;y^|^uuml;kmumcu ◽  
H. S^|^ouml;kmen ◽  
M. Kildir

2009 ◽  
Vol 5 (S265) ◽  
pp. 420-421
Author(s):  
João A. S. Amarante ◽  
Helio J. Rocha-Pinto

AbstractWe investigate the angular momentum distribution of known exoplanetary systems, as a function of the planetary mass, orbital semimajor axis and metallicity of the host star. We find exoplanets seems to be classified according to at least two ‘populations’, with respect to their angular momentum properties. This classification is independent on the composition of the planet and seems to be valid for both jovian and neptunian planets, and probably can be extrapolated to the terrestrial planets of the Solar System. We analyse these ‘populations’ considering the phenomenon of planetary migration.


2018 ◽  
Vol 16 (4) ◽  
pp. 040202 ◽  
Author(s):  
Jintai Liang Jintai Liang ◽  
Ruozhou Zhang Ruozhou Zhang ◽  
Xiaomeng Ma Xiaomeng Ma ◽  
Yueming Zhou Yueming Zhou ◽  
Peixiang Lu Peixiang Lu

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