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Transition matrix

Prom the reciprocity relation for the amplitude matrix we easily derive the reciprocity relation for the phase and extinction matrices  [Pg.57]

The reciprocity relations can be used in practice for testing the results of theoretical computations and laboratory measurements. It should be remarked that reciprocity relations give also rise to symmetry relations for the dyadic Green functions [229]. [Pg.57]

The transition matrix relates the expansion coefficients of the incident and scattered fields. The existence of the transition matrix is postulated by the T-Matrix Ansatz and is a consequence of the series expansions of the incident and scattered fields and the linearity of the Maxwell equations. Historically, the transition matrix has been introduced within the null-field method formalism (see [253,256]), and for this reason, the null-field method has often been referred to as the T-matrix method. However, the null-field method is only one among many methods that can be used to compute the transition matrix. The transition matrix can also be derived in the framework of the method of moments [88], the separation of variables method [208], the discrete dipole approximation [151] and the point matching method [181]. Rother et al. [205] foimd a general relation between the surface Green function and the transition matrix for the exterior Maxwell problem, which in principle, allows to compute the transition matrix with the finite-difference technique. [Pg.57]

In this section we review the general properties of the transition matrix such as imitarity and symmetry and discuss anafjdical procedures for averaging scattering characteristics over particle orientations. These procedures [Pg.57]

In this section we shall consider how to choose a transition matrix P consistent with (16) that is (in some sense) the optimum matrix. We first note that we have a good deal of freedom in our choice of P since (16) is not very restrictive. To decide among these matrices we require a suitable criterion and an obvious choice would be to choose P to minimize the resulting variance, var (M ),of the estimate [Eq. (19)] over successive states of a Markov chain [Pg.144]

An important consequence of this result is that the Metropolis transition matrix defined by (17) yields a lower asymptotic variance than does the Barker transition matrix defined by (18). [Pg.144]

The corresponding transition matrix with the transition probabilities given by Eq. (18) is [Pg.145]

Several suggestions have been made about possible choices of P. Usually (for fluid problems) a particle is chosen at random and moved through a distance uniformly distributed in a unit cube of side centered on the initial position of the particle. Convergence rates will normally depend critically on the value of d chosen. If d is too small, the space will not be adequately sampled, although most moves will be accepted, while, if d is too large, most moves will be rejected (at least in a dense system) and the sampling will again be inadequate. The rule of thumb often used is to choose d so that about half of the moves are accepted. [Pg.146]

Other choices for P include moving several or all of the particles at each step, and moving the particles sequentially instead of in a random order. Little seems to be known about the relative merits of these approaches, although it is clear that varying P may radically alter the convergence rate in a particular problem. [Pg.146]

Material flows along multi-product pipelines are far more complicated to plan. The most prominent field of application for multi-product pipelines is the distribution of refinery products among a network of distribution terminals. The operating principle is essentially the same as for single product pipelines. However, as multiple materials pass the pipeline sequentially, the different materials have to be separated in some sense. Basically there are two options to separate batches of different materials [Pg.67]

The second option is simply to allow a mixture of successively injected materials. This transition mixture is often labelled as interface. This option is preferable as in many cases the set of materials to be transported is chemically homogeneous (e.g. crude oil derivatives). However, the interface is stiff a problem as it typically does not meet the chemical specifications of one of the parental materials. There are two ways to deal with the interface Either the interface is added to one of both parental materials where it does not harm in the further production processes or the interface has to be extracted (e.g. at the end of a serial pipeline) for a special treatment. No matter how interfaces are treated, transition efforts have to be faced. Hence, minimizing the number of interfaces is one objective to aim at when planning multi-product pipeline schedules. [Pg.67]

If transition efforts can be expressed in terms of costs, the total costs for pipeline transport can be used as the planning objective. In this context, total costs comprise transition costs, transport costs, and inventory costs. Transport costs account for operational pipeline costs, such as the energy costs for pumping. These costs are affected by the pipeline s pump rate which needs to be explicitly controlled and planned when the transported materials differ in viscosity or other physical properties. Inventory costs are [Pg.67]

In the batch flow system, the pipeline connects two locations where a set of products is produced and consumed. The subset of products that are used at both locations is denoted by S. These products have to be balanced between both locations by pipeline transports. [Pg.68]

In the literature, basically two directions can be distinguished. A concise comparison of the problem features tackled in both directions is contained in Table 3.5. [Pg.68]


State I ) m the electronic ground state. In principle, other possibilities may also be conceived for the preparation step, as discussed in section A3.13.1, section A3.13.2 and section A3.13.3. In order to detemiine superposition coefficients within a realistic experimental set-up using irradiation, the following questions need to be answered (1) Wliat are the eigenstates (2) What are the electric dipole transition matrix elements (3) What is the orientation of the molecule with respect to the laboratory fixed (Imearly or circularly) polarized electric field vector of the radiation The first question requires knowledge of the potential energy surface, or... [Pg.1059]

Luce T A and Bennemann K H 1998 Nonlinear optical response of noble metals determined from first-principles electronic structures and wave functions calculation of transition matrix elements P/rys. Rev. B 58 15 821-6... [Pg.1302]

In equation (bl. 15.7) p(co) is tlie frequeney distribution of the MW radiation. This result obtained with explieit evaluation of the transition matrix elements oeeurring for simple EPR is just a speeial ease of a imieh more general result, Femii s golden mle, whieh is the basis for the ealeulation of transition rates in general ... [Pg.1550]

The transition matrix T(b)f is therefore the probability of scattering particles with impact parameter b. B2.2.6.4 DIFFERENTIAL CROSS SECTIONS... [Pg.2032]

The transition matrix J is synnnetrical, o= and the cross sections satisfy detailed balance. Each... [Pg.2045]

Projecting the nuclear solutions Xt( ) oti the Hilbert space of the electronic states (r, R) and working in the projected Hilbert space of the nuclear coordinates R. The equation of motion (the nuclear Schrddinger equation) is shown in Eq. (91) and the Lagrangean in Eq. (96). In either expression, the terms with represent couplings between the nuclear wave functions X (K) and X (R). that is, (virtual) transitions (or admixtures) between the nuclear states. (These may represent transitions also for the electronic states, which would get expressed in finite electionic lifetimes.) The expression for the transition matrix is not elementaiy, since the coupling terms are of a derivative type. [Pg.151]

The elements of the transition matrix from state j to state i can be estimated in the transition state theory approximation... [Pg.209]

The equilibrium distribution of the system can be determined by considering the result c applying the transition matrix an infinite number of times. This limiting dishibution c the Markov chain is given by pij jt = lim, o p(l)fc -... [Pg.431]

We can illustrate the use of this transition matrix as follows. Suppose the initial probabilit vector is (1,0) and so the system starts with a 100% probability of being in state 1 and n probability of being in state 2. Then the second state is given by ... [Pg.431]

When the limiting distribution is reached then application of the transition matrix mu return the same distribution back ... [Pg.431]

Closely related to the transition matrix is the stochastic matrix, whose elements are labelle a . TTiis matrix gives the probability of choosing the two states m and n between whic the move is to be made. It is often known as the underlying matrix of the Markov chain, the probability of accepting a trial move from m to n is then the probability of makir a transition from m to n (7r, ) is given by multiplying the probability of choosing states... [Pg.431]

A simple method for predicting electronic state crossing transitions is Fermi s golden rule. It is based on the electromagnetic interaction between states and is derived from perturbation theory. Fermi s golden rule states that the reaction rate can be computed from the first-order transition matrix and the density of states at the transition frequency p as follows ... [Pg.169]

The exponential matrix e in equation (8.46) is ealled the state-transition matrix < t) and represents the natural response of the system. Henee... [Pg.240]

Consider a plant that is subjeet to a Gaussian sequenee of disturbanees w(kT) with disturbanee transition matrix Cd(r). Measurements z(/c+ )T eontain a Gaussian noise sequenee v(/c + )T as shown in Figure 9.6. [Pg.286]

Q(7 ) is the disturbanee transition matrix Q is the disturbanee noise eovarianee matrix R is the measurement noise eovarianee matrix... [Pg.287]

A discrete simulation was undertaken using equations (9.85) and (9.86) together with a disturbance transition matrix Cd(T ), which was calculated using in equation (9.84) and equation (8.80) for B(r), with a sampling time of 2 seconds. [Pg.293]

Step 2 - Specify the Arc-to-Arc Transition Matrix V Each element [Pij]... [Pg.307]


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Continuous time state transition matrix

Dipole transition matrix element

Discrete-time state transition matrix

Disturbance transition matrix

Electronic transition energies, matrix

Hamiltonian matrix transition metals

Matrices glass transition

Matrix element magnetic transition

Matrix element of transitions

Matrix element transition gradient

Matrix phase transitions

Matrix-bound transition-metal complexe

Matrix-isolation studies, transition

Nonadiabatic transition matrix

Risk-neutral transition matrix

Scattering theory, resonances transition matrix

State-transition matrix

Symmetries of the Transition Matrix

System transition matrix

The Transition Matrix

The one-step transition probability matrix

Three-photon transition matrix elements

Transition density matrix

Transition dipole matrix

Transition dipole matrix elements states

Transition matrix elements

Transition matrix-bound

Transition metal vapor cryochemistry in alkane matrices

Transition metals hybridization matrix element

Transition probability matrix

Transition probability matrix between surfaces

Transition probability matrix chains

Transition rate using density matrices

Transition reduced density matrix

Transition, complex probability matrix

Transition, radiative matrix method

Transition-Matrix Estimators

Transition-Monopole Treatments of Interaction Matrix Elements and Mixing with Charge-Transfer Transitions

Transition-matrix technique

Transitions host matrices

Wave function expansions transition matrix elements

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