An atomistic study of defect energetics and diffusion with respect to composition and temperature in γU and γU-Mo alloys

2021 ◽  
pp. 152970
Author(s):  
Gyuchul Park ◽  
Benjamin Beeler ◽  
Maria A. Okuniewski
2008 ◽  
Vol 56 (15) ◽  
pp. 3761-3769 ◽  
Author(s):  
Shinya Taketomi ◽  
Ryosuke Matsumoto ◽  
Noriyuki Miyazaki

1976 ◽  
Vol 32 ◽  
pp. 109-116 ◽  
Author(s):  
S. Vauclair

This paper gives the first results of a work in progress, in collaboration with G. Michaud and G. Vauclair. It is a first attempt to compute the effects of meridional circulation and turbulence on diffusion processes in stellar envelopes. Computations have been made for a 2 Mʘstar, which lies in the Am - δ Scuti region of the HR diagram.Let us recall that in Am stars diffusion cannot occur between the two outer convection zones, contrary to what was assumed by Watson (1970, 1971) and Smith (1971), since they are linked by overshooting (Latour, 1972; Toomre et al., 1975). But diffusion may occur at the bottom of the second convection zone. According to Vauclair et al. (1974), the second convection zone, due to He II ionization, disappears after a time equal to the helium diffusion time, and then diffusion may happen at the bottom of the first convection zone, so that the arguments by Watson and Smith are preserved.


1997 ◽  
Vol 101-103 (1-2) ◽  
pp. 479-487
Author(s):  
H v. Wensierski
Keyword(s):  

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