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Probability density function explained

Here pj = pj +pjy + pj7 and U is the potential associated with the inter-particle interaction. The function/(/ , p ) is an example of a joint probability density function (see below). The staicture of the Hamiltonian (1.184) implies that f can be factorized into a term that depends only on the particles positions and terms that depend only on their momenta. This implies, as explained below, that at equilibrium positions and momenta are statistically independent. In fact, Eqs (1.183) and (1.184) imply that individual particle momenta are also statistically independent and so are the different cartesian components of the momenta of each particle. [Pg.39]

Find out and explain the use of probability density functions to describe the behaviour of electrons in the orbitals of atoms. A probability distribution function is any function whose integral over a set gives the probability that a random variable has a value in that set. Use diagrams to illustrate your answer. [Pg.57]

The Maxwell-Boltzmann distribution curve is a probability density function. State the assumptions underlying the Maxwell-Boltzmann distribution curve and explain why it is a probability function. [Pg.57]

On the other hand, false coverage probabilities do not allow any practical interpretation. In particular, an experimenter would like to know, in practical terms, how well a method performs with respect to others and how its performance is affected by the sample size. Let s take a closer look at the behavior oi Ip. K simulation of Ip values, which will be explained later, yielded the probability density functions for the two methods illustrated in Fig. 1. For this simulation the parameters are set as m = 5, CTo = 100, p = Q.Ql, and the sample size is chosen as = 20. The density function of Ip estimated by the ML method is slightly to the right of the function estimated by the GLR method 1. Therefore, for any a p significant difference from the viewpoint of an experimenter. Further, Method 1 is one of the worst methods in Table 1, so the difference between the ML method and the GLR methods with weighted least squares is expected to be smaller. One practical way for quantifying the difference is to compute the sample size necessary for the ML method to have approximately the same density function as the GLR method 1. [Pg.221]

Damage quantification using the classical statistics procedure yields a 90 % confidence interval of (24,509 NIm, 24,612 NIni). The Bayesian approach directly calculates the probability distribution of ki as explained in section Uncertainty in Damage Estimation. The overall uncertainty in diagnosis can be calculated as in section Overall Uncertainty in Diagnosis, and the corresponding probability density function is shown in Fig. 4. From Fig. 4, it can be seen that... [Pg.3834]

The importance of N-representability for pair-density functional theory was not fully appreciated probably because most research on pair-density theories has been performed by people from the density functional theory community, and there is no W-representability problem in conventional density functional theory. Perhaps this also explains why most work on the pair density has been performed in the first-quantized spatial representation (p2(xi,X2) = r2(xi,X2 xi,X2)) instead of the second-quantized orbital representation... [Pg.447]

Consider the reversible two-compartment model that is explained by way of the semi-Markov formulation as illustrated in Figure 9.2 C. We will assume that at the starting time all molecules are present in compartment 1. A single molecule that is present at the initial time in compartment 1 stays there for a length of time that has a single-passage density function fi (a). Then, it has the possibility to definitively leave the system with probability 1 — ui or reach the compartment 2 with probability cu. The retention time in this compartment is... [Pg.217]

Quantum mechanics explains the physical stability of the planetary atom, predicts its allowed energy levels, and defines the wave functions (also called atomic orbitals), which determine the probability density for finding the electrons at particular locations in the atom. [Pg.204]

Several structure sizes caused by microphase separation occurring in the induction period as well as by crystallization were determined as a function of annealing time in order to determine how crystallization proceeds [9,18]. The characteristic wavelength A = 27r/Qm was obtained from the peak positions Qm of SAXS while the average size of the dense domains, probably having a liquid crystalline nematic structure as will be explained later, was estimated as follows. The dense domain size >i for the early stage of SD was calculated from the spatial density correlation function y(r) defined by Debye and Buche[50]... [Pg.200]

It was not until 1987, before a second model on electrocodeposition was published by Buelens [37, 58], From experimental observations on the codeposition of particles on a rotating disk electrode (RDE) as a function of current density, rotation speed and bath composition, that could not be explained by Guglielmi, she suggested that a particle will only be incorporated into the deposit if a certain amount of the adsorbed ions on the particle surface is reduced. This is one possible way to account for the field-assisted adsorption, held responsible for the transition between loosely and strongly adsorbed particles in the model of Guglielmi. This proposition yields the probability P(k/K,i) for the incorporation of a particle based on the reduction of k out of K ions, bound to its surface, at current density i... [Pg.213]


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