scholarly journals Simulations of Radiative‐Convective‐Dynamical Equilibrium

2020 ◽  
Vol 12 (3) ◽  
Author(s):  
Robert A. Warren ◽  
Martin S. Singh ◽  
Christian Jakob
1997 ◽  
Vol 476 (1) ◽  
pp. L7-L10 ◽  
Author(s):  
R. G. Carlberg ◽  
H. K. C. Yee ◽  
E. Ellingson ◽  
S. L. Morris ◽  
R. Abraham ◽  
...  

Author(s):  
H. J. Schröder ◽  
P. Schuster

When dealing with axisymmetric rotating flow through turbomachines of a given geometry, the existence of discontinuities, due to incidence at the leading edges of the blades, has to be accepted as a logical consequence of axisymmetry. By introducing special conditions resulting from dynamical equilibrium considerations, a relaxation method has been enabled to cope with these discontinuities.


Crystals ◽  
2020 ◽  
Vol 10 (9) ◽  
pp. 766
Author(s):  
Oier Bikondoa ◽  
Dina Carbone

X-ray photon correlation spectroscopy accesses a wide variety of dynamic phenomena at the nanoscale by studying the temporal correlations among photons that are scattered by a material in dynamical equilibrium when it is illuminated with a coherent X-ray beam. The information that is obtained is averaged over the illuminated area, which is generally of the order of several square microns. We propose here that more local information can be obtained by using nanobeams with great potential for the study of heterogeneous systems and show the feasibility of this approach with the support of numerical simulations.


1992 ◽  
Vol 150 ◽  
pp. 205-210
Author(s):  
Sheo S. Prasad

Evolutionary chemical models are ultimately unavoidable for a full understanding of interstellar clouds. They include not only the chemical processes but also the dynamical processes by which the modeled object came to be the way it is. From an evolutionary perspective, dark cores may be ephemeral objects and dynamical equilibrium an exception rather than norm. Evolutionary models have numerous advantages over “classical” fixed condition equilibrium models. They have the potential to provide more elegant explanations for the observed inter-cloud and intra-cloud chemical differences. The problem of the depletion of gas phase molecules by condensation onto the grain may also be less serious in evolutionary models. Hence, these models should be actively developed.


2012 ◽  
Vol 86 (20) ◽  
Author(s):  
K. Pussi ◽  
H. I. Li ◽  
Heekeun Shin ◽  
L. N. Serkovic Loli ◽  
A. K. Shukla ◽  
...  

2000 ◽  
Vol 610 ◽  
Author(s):  
Alain Claverie ◽  
Filadelfo Cristiano ◽  
Benjamin Colombeau ◽  
Nicholas Cowern

AbstractIn this paper, we discuss the mechanisms by which small clusters evolve through “magic” sizes into {113} defects and then, at sufficiently high dose levels, transform into dislocation loops of two types. This ripening process is mediated by the interchange of free Si(int)s between different extended defects, leading to a decrease of their formation energy. The calculation of the supersaturation of free Si-interstitials in dynamical equilibrium with these defects shows a hierarchy of levels of nonequilibrium diffusion, ranging from supersaturations S of about 106 in the presence of small clusters, through 103 in the presence of {113} defects, to S in the range 100 down to 1 as loops are formed, evolve and finally evaporate. A detailed analysis of defect energetics has been carried out and it is shown that Ostwald ripening is the key concept for understanding and modelling defect interactions during TED of dopants in silicon.


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