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Quantum intensity trajectory

Figure 17.12 (A) Schematic presentation of deactivation and energy transfer processes in a single quantum dot placed on an Ag nanoparticle film. (B) Photoluminescence intensity trajectories of single quantum dots on a glass substrate (a) and on an Ag nanoparticle film (b). The traces in green represent background intensities. (C) Photoluminescence spectra of quantum dot solutions in the presence of... Figure 17.12 (A) Schematic presentation of deactivation and energy transfer processes in a single quantum dot placed on an Ag nanoparticle film. (B) Photoluminescence intensity trajectories of single quantum dots on a glass substrate (a) and on an Ag nanoparticle film (b). The traces in green represent background intensities. (C) Photoluminescence spectra of quantum dot solutions in the presence of...
These new trajectories are the so-called reduced quantum trajectories [30], which are only explicitly related to the system reduced density matrix. The dynamics described by Equation 8.42 leads to the correct intensity (time evolution of which is described by Equation 8.40) when the statistics of a large number of particles are considered. Moreover, Equation 8.42 reduces to the well-known expression for the velocity held in Bohmian mechanics, when there is no interaction with the environment. [Pg.117]

The reduction of chaos for 9 = 1.45 is presented in the intensity portraits of Fig. 39. However, as is seen in Fig. 38a, there is a small region (1.68 < 9 < 1.80) where the system behaves orderly in the classical case but the quantum correction leads to chaos. By way of an example for 9=1.75, the classical system, after quantum correction, loses its orderly features and the limit cycle settles into a chaotic trajectory. Generally, Lyapunov analysis shows that the transition from classical chaos to quantum order is very common. For example, this kind of transition appears for 9 = 3.5 where chaos is reduced to periodic motion on a limit cycle. Therefore a global reduction of chaos can be said to take place in the whole region of the parameter 0 < 9 < 7. [Pg.421]

In addition to experiments, a range of theoretical techniques are available to calculate thermochemical information and reaction rates for homogeneous gas-phase reactions. These techniques include ab initio electronic structure calculations and semi-empirical approximations, transition state theory, RRKM theory, quantum mechanical reactive scattering, and the classical trajectory approach. Although still computationally intensive, such techniques have proved themselves useful in calculating gas-phase reaction energies, pathways, and rates. Some of the same approaches have been applied to surface kinetics and thermochemistry but with necessarily much less rigor. [Pg.476]

The dipole moment components as a function of time are usually computed with a fixed charge approximation. Values of atomic charges are often taken from quantum chemical calculations of representative models, although absolute charge values play no role (other than influencing the MD trajectory) unless absolute infrared intensities are to be computed. FFowever, the relative values of charges are of importance for reproducing relative band intensities. [Pg.182]

For better comparison of theoretical predictions for different-order processes, we have plotted the quantum Fano factors for both interacting modes in the no-energy-transfer regime with N = 2 — 5 and r = 5 in Fig. 7. One can see that all curves start from F w(0) = 1 for the input coherent fields and become quasistationary after some relaxations. The quantum and semiclassical Fano factors coincide for high-intensity fields and longer times, specifically for t > 50/(Og), where il will be defined later by Eq. (54). In Fig. 17, we observe that all fundamental modes remain super-Poissonian [F (t) >1], whereas the iVth harmonics become sub-Poissonian (F (t) < 1). The most suppressed noise is observed for the third harmonic with the Fano factor 0.81. In Fig. 7, we have included the predictions of the classical trajectory method (plotted by dotted lines) to show that they properly fit the exact quantum results (full curves) for the evolution times t > 50/(Og). The small residual differences result from the fact that the amplitude r was chosen to be relatively small (r = 5). This value does not precisely fulfill the condition r> 1. We have taken r = 5 as a compromise between the asymptotic value r oo and computational complexity to manipulate the matrices of dimensions 1000 x 1000. Unfortunately, we cannot increase amplitude r arbitrary due to computational limitations. [Pg.508]

The reactions of 0( P) with H2 D2 and HD have become one of the most intensively studied set of reactions both experimentally and theoreti cally. Theoretically there have b ej several three-dimensional quasiclassical trajectory studies collinear exact quantum... [Pg.68]

Because the electronic energy Ee(q) in Eq. [8] and its derivatives must be calculated at each integration step of a classical trajectory, a direct dynamics simulation is usually very computationally intense. A standard numerical integration time step is /St = 10 " s. Thus, if a trajectory is integrated for 10 s, 10" evaluations of Eq. (8) are required for each trajectory. An ensemble for a trajectory simulation may be as small as 100 events, but even with such a small ensemble 10 " electronic structure calculations are required. Because of such computational demands, it is of interest to determine the lowest level of electronic structure theory and smallest basis set that gives an adequate representation for the system under study. In the following parts of this section, semiempirical and ab initio electronic structure theories and mixed electronic structure theory (quantum mechanical) and molecular mechanical (i.e. QM/MM) approaches for performing direct dynamics are surveyed. [Pg.86]


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