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Gaussian constraint

In constrained simulations near the transition state, it is difficult to sample from the delta function constraint (3.41), especially if a Monte Carlo sampling is used. It is therefore convenient to approximate the constrained weight function (3.41) by using the Gaussian approximation of the delta function in Eq. (3.15). This Gaussian constraint corresponds to a harmonic constraint potential Vconstr,y(r) [30,32] ... [Pg.78]

When is identified with a real friction coefficient, one has to include fluctuating Brownian forces in the expression for F, in addition to a deterministic force, in order to have the particle moving such that it has a (peculiar) kinetic energy in accord with the temperature of the fluid. As an alternative, we use here the Gaussian constraint to ensure that... [Pg.274]

Owing to the constraints, no direct solution exists and we must use iterative methods to obtain the solution. It is possible to use bound constrained version of optimization algorithms such as conjugate gradients or limited memory variable metric methods (Schwartz and Polak, 1997 Thiebaut, 2002) but multiplicative methods have also been derived to enforce non-negativity and deserve particular mention because they are widely used RLA (Richardson, 1972 Lucy, 1974) for Poissonian noise and ISRA (Daube-Witherspoon and Muehllehner, 1986) for Gaussian noise. [Pg.405]

These filler constraints can be represented by a Gaussian potential... [Pg.611]

Equations 22.3-22.14 represent the simplest formulation of filled phantom polymer networks. Clearly, specific features of the fractal filler structures of carbon black, etc., are totally neglected. However, the model uses chain variables R(i) directly. It assumes the chains are Gaussian the cross-links and filler particles are placed in position randomly and instantaneously and are thereafter permanent. Additionally, constraints arising from entanglements and packing effects can be introduced using the mean field approach of harmonic tube constraints [15]. [Pg.611]

If basic assumptions concerning the error structure are incorrect (e.g., non-Gaussian distribution) or cannot be specified, more robust estimation techniques may be necessary. In addition to the above considerations, it is often important to introduce constraints on the estimated parameters (e.g., the parameters can only be positive). Such constraints are included in the simulation and parameter estimation package SIMUSOLV. Beeause of numerical inaccuracy, scaling of parameters and data may be necessary if the numerical values are of greatly differing order. Plots of the residuals, difference between model and measurement value, are very useful in identifying systematic or model errors. [Pg.114]

The latter approach has the advantage that the exact J is approached strictly from above, however for technical reasons it is only applicable if Gaussian basis functions are employed (Dunlap, Connolly, and Sabin, 1979). Both schemes are of course subject to the constraint that the fitted density is normalized to the total number of electrons, i. e ... [Pg.119]

Here x=qNb/6=qR where Ru is the radius of an undeformed Gaussian random flight chain. I deriving Eq. 10, the sum in Eq. 7 is replaced by an integral. The effect of the free chain segments, exclusive of the position of the junctions appears in the first two terms in the exponential. The deformations of the chains depend on the constraints on the junctions. Results are immediately derivable from Eq. 10. [Pg.262]

As was shown, the conventional method for data reconciliation is that of weighted least squares, in which the adjustments to the data are weighted by the inverse of the measurement noise covariance matrix so that the model constraints are satisfied. The main assumption of the conventional approach is that the errors follow a normal Gaussian distribution. When this assumption is satisfied, conventional approaches provide unbiased estimates of the plant states. The presence of gross errors violates the assumptions in the conventional approach and makes the results invalid. [Pg.218]

The dWi are Gaussian white noise processes, and their strength a is related to the kinetic friction y through the fluctuation-dissipation relation.72 When deriving integrators for these methods, one has to be careful to take into account the special character of the random forces employed in these simulations.73 A variant of the velocity Verlet method, including a stochastic dynamics treatment of constraints, can be found in Ref. 74. The stochastic... [Pg.17]

Figure 9. Mass - radius relations for compact star configurations with different EoS purely hadronic star with HHJ EoS (long-dashed), stable hybrid stars for HHJ - INCQM EoS with 2SC (solid) and without 2SC phase (dash-dotted) for the Gaussian formfactor. We show the influence of a tiny variation of the coupling constant Gi by the filled grey band. The difference between the models 2SC and 2SC corresponds to a shift in the bag function (see Fig. 8) 3 MeV/fm3. For comparison, observational constraints on the compactness are given from the "small compact star RX J1856.5-3754 and from the high surface redshift object EXO 0748-676 which can both be obeyed by our hybrid star EoS. Figure 9. Mass - radius relations for compact star configurations with different EoS purely hadronic star with HHJ EoS (long-dashed), stable hybrid stars for HHJ - INCQM EoS with 2SC (solid) and without 2SC phase (dash-dotted) for the Gaussian formfactor. We show the influence of a tiny variation of the coupling constant Gi by the filled grey band. The difference between the models 2SC and 2SC corresponds to a shift in the bag function (see Fig. 8) 3 MeV/fm3. For comparison, observational constraints on the compactness are given from the "small compact star RX J1856.5-3754 and from the high surface redshift object EXO 0748-676 which can both be obeyed by our hybrid star EoS.
The commercially available software (Maximum Entropy Data Consultant Ltd, Cambridge, UK) allows reconstruction of the distribution a.(z) (or f(z)) which has the maximal entropy S subject to the constraint of the chi-squared value. The quantified version of this software has a full Bayesian approach and includes a precise statement of the accuracy of quantities of interest, i.e. position, surface and broadness of peaks in the distribution. The distributions are recovered by using an automatic stopping criterion for successive iterates, which is based on a Gaussian approximation of the likelihood. [Pg.189]

Early-time motion, for segments s such that UgM(s)activated exploration of the original tube by the free end. In the absence of topological constraints along the contour, the end monomer moves by the classical non-Fickian diffusion of a Rouse chain, with spatial displacement f, but confined to the single dimension of the chain contour variable s. We therefore expect the early-time result for r(s) to scale as s. When all prefactors are calculated from the Rouse model [2] for Gaussian chains with local friction we find the form... [Pg.219]

With four-point collocation using gaussian roots (the A-stable case), we fail to find an optimal solution. Because of this, we include an additional constraint on the control profile error (third time derivative of the control profile less than a tolerance, see Russell and Christiansen, 1978). The resulting... [Pg.243]

How do the form Qm of a prior object and the number z of degrees of freedom affect the estimate nm This was the problem (37) augmented by data constraints (50). Suppose in addition that the image data im suffer from Gaussian additive noise, so that Eq. (54) is true. Then the total estimator given by Eqs. (56) and (57) becomes... [Pg.254]


See other pages where Gaussian constraint is mentioned: [Pg.334]    [Pg.334]    [Pg.24]    [Pg.73]    [Pg.336]    [Pg.360]    [Pg.100]    [Pg.257]    [Pg.610]    [Pg.116]    [Pg.168]    [Pg.17]    [Pg.64]    [Pg.260]    [Pg.455]    [Pg.35]    [Pg.64]    [Pg.93]    [Pg.300]    [Pg.8]    [Pg.140]    [Pg.118]    [Pg.201]    [Pg.269]    [Pg.280]    [Pg.295]    [Pg.297]    [Pg.455]    [Pg.17]    [Pg.29]   
See also in sourсe #XX -- [ Pg.274 , Pg.279 ]




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