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Dynamical constraints

The situation is different for incompressible flow. In that case, no equation of motion for the pressure field exists and via the mass conservation equation Eq. (17) a dynamic constraint on the velocity field is defined. The pressure field entering the incompressible Navier-Stokes equation can be regarded as a parameter field to be adjusted such that the divergence of the velocity field vanishes. [Pg.157]

Another possibly problematical observation is that the D/H ratio of the Earth s oceans is roughly half that measured in comets, but is similar to that for carbonaceous chondrites (Fig. 14.10). For this reason, Dauphas et al. (2000) calculated that no more than 10% of our planet s H20 was accreted as comet ice, a conclusion consistent with dynamical constraints (Morbedelli et al., 2000). Despite the importance that D/H measurements have been given in recent publications, fractionation of these isotopes when ice is sublimated has been demonstrated experimentally. Consequently, the measurements of D/H in comet comae may not... [Pg.503]

We distinguish two limiting cases dissociation through a narrow transition state and dissociation through a wide transition state where we define the region that separates the reactants and the products (i.e., the point of no return ) as the transition state. The first case may be qualitatively considered as a direct process with the ultimate dissociation starting at the transition state. The second case may be treated by statistical methods without including dynamical constraints. We will discuss both limits separately and illustrate them with typical examples. [Pg.241]

Because of its simplicity the impulsive model is very appealing and frequently employed to model measured rotational state distributions (Dugan and Anthony 1987 Levene and Valentini 1987 Butenhoff, Car-leton, and Moore 1990). In most applications, however, it is necessary to incorporate at least one fit parameter or some dynamical constraints in order to obtain agreement with experimental results, for example, the equilibrium angle in the excited electronic state or the point at which the repulsive force vector intersects the BC-axis. The impulsive model is not an a priori theory. [Pg.253]

Muesgens F., Neuhoff, K., 2006. Modelling Dynamic Constraints in Electricity Markets and the Costs of Uncertain Wind Output. EPRG WP 05/14. [Pg.69]

Hamilton s principle exploits the power of generalized coordinates in problems with static or dynamical constraints. Going beyond the principle of least action, it can also treat dissipative forces, not being restricted to conservative systems. If energy loss... [Pg.12]

This bare-bones treatment can be elaborated in considerable variety. Coordinate changes are the most primitive possibihty dynamical constraints that are popular in molecular dynamics simulation packages can be addressed from this point of view. Slightly trickier are cases for which treats some atoms of... [Pg.30]

CARS measurements have revealed an unexpected propensity for population of the even rotational levels in v" = 0 and v" = 1 (Moore et al., 1983). No explanation based on symmetry or dynamical constraints for this interesting observation is immediately forthcoming. Further elucidation of the dynamics of (8) will probably require refinement of our understanding of the role of symmetry conservation in the dissociation of triatomic molecules. [Pg.151]

There are a number of lines of evidence that the Earth may have been affected by additions of further material subsequent to the giant impact. Similarly, there is limited evidence that there was additional core formation. Alternatively, there also are geochemical and dynamic constraints that strongly limit the amount of core formation and accretion since the giant impact. This is a very interesting area of research that is ripe for further development. Here are some of the key observations ... [Pg.538]

The foregoing developments in terms of the surprisal provide, at least, a successful parametrization for distributions of direct reactions. Nonexistence of long-lived states in these reactions would make unjustifiable the introduction of temperatures in the sense of equilibrium thermodynamics. At best, parametrization may lead to dynamical models with predictive value. These are not available at the present time, though progress is being made in this area by Hofacker and coworkers (op. dr), using model Hamiltonians that include vibrationally diabatic effects, and introducing dynamical constraints in statistical models. [Pg.45]

The molecular dynamics constraint technique presented in the previous section is designed to simulate steady solutions of the Euler equations but there is no guarantee that all of the simulated solutions are physical. Some steady solutions are characterized by unboimded volume expansion, and others may not be the particular shock wave solutions desired. This section defines mechanical stability conditions that characterize shock waves and then shows that the molecular dynamics constraint technique naturally takes the system through states that satisfy these stability conditions. [Pg.303]

An alternative philosophy is to construct a classical trajectory which is not a solution of an initial value problem. Such constrained trajectories would no longer obey Hamilton s equations, but would extremize the classical action subject to certain dynamical constraints (50-52). [Pg.604]


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