Evaluation of Portfolio Decision Improvements by Markov Modulated Diffusion Processes: A Shapley Value Approach

Author(s):  
Benjamin Vallejo-Jimenez ◽  
Mario A. Garcia-Meza
2016 ◽  
Vol 126 (6) ◽  
pp. 1785-1818 ◽  
Author(s):  
Gang Huang ◽  
Michel Mandjes ◽  
Peter Spreij

2014 ◽  
Vol 24 (12) ◽  
pp. 825-836 ◽  
Author(s):  
Shih-Kuei Lin ◽  
Yu-Min Lian ◽  
Szu-Lang Liao

2014 ◽  
Vol 86 ◽  
pp. 74-79 ◽  
Author(s):  
Gang Huang ◽  
Michel Mandjes ◽  
Peter Spreij

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.


Author(s):  
Ari Arapostathis ◽  
Vivek S. Borkar ◽  
Mrinal K. Ghosh

1980 ◽  
Vol 41 (C6) ◽  
pp. C6-28-C6-31 ◽  
Author(s):  
R. Messer ◽  
H. Birli ◽  
K. Differt

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