Dynamic evolution model

Lin, H.F, Li, S.G, Cheng, L.H, et al. 2011. Experimental analysis of dynamic evolution model of mining-induced fissure zone in overlying strata. Mining and Sleety Engineering 28(2) 298-303. 

In the mixed quantum-classical molecular dynamics (QCMD) model (see [11, 9, 2, 3, 5] and references therein), most atoms are described by classical mechanics, but an important small portion of the system by quantum mechanics. The full quantum system is first separated via a tensor product ansatz. The evolution of each part is then modeled either classically or quan-tally. This leads to a coupled system of Newtonian and Schrbdinger equations. 

In order to describe correctly the dynamic evolution of a fluid/fluid interface, a number of boundary conditions have to be implemented into the computational models. 

Sharon D., Glusman G., Pilpel Y., Hom-Saban S. and Lancet D. (1998). Genome dynamics, evolution, and protein modelling in the olfactory gene superfamily. Ann NY Acad Sci 855, 182-193. 

Abstract. In an effort to determine accurate stellar parameters and abundances for a large sample of nearby stars, we have performed the detailed analysis of 350 high-resolution spectra of FGK dwarfs and giants. This sample will be used to investigate behavior of chemical elements and kinematics in the thick and thin disks, in order to better constrain models of chemical and dynamical evolution of the Galaxy. 

We have now to go one step further and to build stellar evolution models where the transport of angular momentum will be followed self-consistently under the action of meridional circulation, shear turbulence, and internal gravity waves. In this path some important aspects still need to be clarified Can we better describe the excitation mechanisms and evaluate in a more reliable way the quantitative properties of the wave spectra What is the direct contribution of 1GW to the transport of chemicals, especially in the dynamical shear layer produced just below the convective envelope by the wave-mean flow interaction What is the influence of the Coriolis force on IGW How do 1GW interact with a magnetic field Work is in progress in this direction. 

Welch, C. (2007). HyDIVE (Hydrogen Dynamic Infrastructure and Vehicle Evolution) model analysis. Hydrogen Analysis Workshop, August 9—10. Washington ... 

Closing the section on the entire filter scale we may remark that at the multichannel level the dynamic ash model of Konstandopoulos et al. (2003) and Rodriguez-Perez et al. (2004) can reproduce ash deposition patterns occurring in fuel-additive assisted regeneration (Blanchard et al., 2004) as seen in Fig. 44 as well as describe the pressure drop evolution due to ash accumulation as seen in Fig. 45. 

External stress, locally applied, can have nonlocal static effects in ferroelastics (see Fig. 4 of Ref. [7]). Dynamical evolution of strains under local external stress can show striking time-dependent patterns such as elastic photocopying of the applied deformations, in an expanding texture (see Fig.5 of Ref. [8]). Since charges and spins can couple linearly to strain, they are like internal (unit-cell) local stresses, and one might expect extended strain response in all (compatibility-linked) strain-tensor components. Quadratic coupling is like a local transition temperature. The model we consider is a (scalar) free energy density term... 

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