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Quantum statistical mechanics probability distribution

Much of the recent literature on RDM reconstruction functionals is couched in terms of cumulant decompositions [13, 27-38]. Insofar as the p-RDM represents a quantum mechanical probability distribution for p-electron subsystems of an M-electron supersystem, the RDM cumulant formalism bears much similarity to the cumulant formalism of classical statistical mechanics, as formalized long ago by by Kubo [39]. (Quantum mechanics introduces important differences, however, as we shall discuss.) Within the cumulant formalism, the p-RDM is decomposed into connected and unconnected contributions, with the latter obtained in a known way from the lower-order -RDMs, q < p. The connected part defines the pth-order RDM cumulant (p-RDMC). In contrast to the p-RDM, the p-RDMC is an extensive quantity, meaning that it is additively separable in the case of a composite system composed of noninteracting subsystems. (The p-RDM is multiphcatively separable in such cases [28, 32]). The implication is that the RDMCs, and the connected equations that they satisfy, behave correctly in the limit of noninteracting subsystems by construction, whereas a 2-RDM obtained by approximate solution of the CSE may fail to preserve extensivity, or in other words may not be size-consistent [40, 42]. [Pg.262]

Note the qualitative — not merely quantitative — distinction between the thermodynamic (Boltzmann-distribution) probability discussed in Sect. 3.2. as opposed to the purely dynamic (quantum-mechanical) probability Pg discussed in this Sect. 3.3. Even if thermodynamically, exact attainment of 0 K and perfect verification [22] that precisely 0 K has been attained could be achieved for Subsystem B, the pure dynamics of quantum mechanics, specifically the energy-time uncertainty principle, seems to impose the requirement that infinite time must elapse first. [This distinction between thermodynamic probabilities as opposed to purely dynamic (quantum-mechanical) probabilities should not be confused with the distinction between the derivation of the thermodynamic Boltzmann distribution per se in classical as opposed to quantum statistical mechanics. The latter distinction, which we do not consider in this chapter, obtains largely owing to the postulate of random phases being required in quantum but not classical statistical mechanics [42,43].]... [Pg.283]

We consider only the equilibrium case so that the distribution of these points phase space is time-independent. In quantum statistical mechanics, we had a discrete list of possible states. In classical statistical mechanics, we have coordinates and momentum components that can range continuously. We denote the probability disttibution (probability density) for the ensemble by / and define the probability that the phase point of a randomly selected system of the ensemble will lie in the 6A -dimensional volume element d tNci pi to be... [Pg.1134]

The prefactor in terms of h is used to expUdtly show the correspondence of Zt with the corresponding PF in the quantum statistical mechanics in the classical limit h O. Despite the classical limit requirement h O.we are not allowed to set h = 0 in the final result, but keep its actual nonzero value. Accordingly, some problems remain such as Wigner s distribution function not being a classical probability distribution, which we do not discuss any further but refer the reader to the Uterature [117]. Keeping h at its nonzero value avoids infinities as we will see below but in no way implies that we are dealing with quantum effects. In particular, it does not imply that the entropy is nonnegative, as we have discussed elsewhere [75]. We... [Pg.490]

In spite of stubborn efforts to reduce it to a statistical probability distribution over states of hidden variables D. Bohm, Phys, Rev. 85, 166 and 180 (1952) F.J. Belinfante, A Survey of Hidden-Variables Theories (Pergamon, Oxford 1973) E. Nelson, Quantum Fluctuations (Princeton University Press, Princeton, NY 1985) J.S. Bell, Speakable and Unspeakable in Quantum Mechanics (Cambridge University Press, Cambridge 1987). [Pg.422]

Elementary concepts of probability and statistics play an important role in this book. Thus, these concepts are an integral part of, e.g., quantum mechanics and statistical mechanics. The probability that some continuous variable x lies between x and x + dx is denoted by P x)dx. Often we refer to P x) as the probability distribution for x (although P(x) strictly speaking is a probability density). The average value or mean value of a variable x, which can take any value between —oo and oo, is defined by... [Pg.14]

Finally, we adopt a notation involving conditional averages to express several of the important results. This notation is standard in other fields (Resnick, 2001), not without precedent in statistical mechanics (Febowitz et al, 1967), and particularly useful here. The joint probability P A, B) of events A and B may be expressed as P A, B) = P A B)P B) where P B) is the marginal distribution, and P A B) is the distribution of A conditional on B, provided that P B) 0. The expectation of A conditional on B is A B, the expectation of A evaluated with the distribution P(A B) for specified B. In many texts (Resnick, 2001), that object is denoted as E(A B) but the bracket notation for average is firmly established in the present subject so we follow that precedent despite the widespread recognition of a notation (A B) for a different object in quantum mechanics texts. [Pg.18]

At last, we can resolve the paradox between de Broglie waves and classical orbits, which started our discussion of indeterminacy. The indeterminacy principle places a fundamental limit on the precision with which the position and momentum of a particle can be known simultaneously. It has profound significance for how we think about the motion of particles. According to classical physics, the position and momentum are fully known simultaneously indeed, we must know both to describe the classical trajectory of a particle. The indeterminacy principle forces us to abandon the classical concepts of trajectory and orbit. The most detailed information we can possibly know is the statistical spread in position and momentum allowed by the indeterminacy principle. In quantum mechanics, we think not about particle trajectories, but rather about the probability distribution for finding the particle at a specific location. [Pg.140]

Theoretical studies of the properties of the individual components of nanocat-alytic systems (including metal nanoclusters, finite or extended supporting substrates, and molecular reactants and products), and of their assemblies (that is, a metal cluster anchored to the surface of a solid support material with molecular reactants adsorbed on either the cluster, the support surface, or both), employ an arsenal of diverse theoretical methodologies and techniques for a recent perspective article about computations in materials science and condensed matter studies [254], These theoretical tools include quantum mechanical electronic structure calculations coupled with structural optimizations (that is, determination of equilibrium, ground state nuclear configurations), searches for reaction pathways and microscopic reaction mechanisms, ab initio investigations of the dynamics of adsorption and reactive processes, statistical mechanical techniques (quantum, semiclassical, and classical) for determination of reaction rates, and evaluation of probabilities for reactive encounters between adsorbed reactants using kinetic equation for multiparticle adsorption, surface diffusion, and collisions between mobile adsorbed species, as well as explorations of spatiotemporal distributions of reactants and products. [Pg.71]

In classical mechanics It Is assumed that at each Instant of time a particle is at a definite position x. Review of experiments, however, reveals that each of many measurements of position of Identical particles in identical conditions does not yield the same result. In addition, and more importantly, the result of each measurement is unpredictable. Similar remarks can be made about measurement results of properties, such as energy and momentum, of any system. Close scrutiny of the experimental evidence has ruled out the possibility that the unpredictability of microscopic measurement results are due to either inaccuracies in the prescription of initial conditions or errors in measurement. As a result, it has been concluded that this unpredictability reflects objective characteristics inherent to the nature of matter, and that it can be described only by quantum theory. In this theory, measurement results are predicted probabilistically, namely, with ranges of values and a probability distribution over each range. In constrast to statistics, each set of probabilities of quantum mechanics is associated with a state of matter, including a state of a single particle, and not with a model that describes ignorance or faulty experimentation. [Pg.259]

Such a chain is also called a chain of random (free) walk, since Kquation 89 matches the distribution calculation of random walk probability of a structural element in space with 71 jumps (steps) from one position to another vvith the length of each jump (step) defined by the probability distribution t Rj) (Flory, 1953 Yamakawa, 1971). Hence. Kquation 89 relates the statistics of polymer chains to the problems of random walk and diffusion. As the diffusion equation is mathematically similar to Schrddinger s one, the common ideology and common mathematical solutions unite the conformational tasks of a polymer chain, the state of quantum-mechanical systems, and the field theory. [Pg.267]

The statistical formulation is based on the premise that the macroscopic properties of a system should be directly deducible firom the properties, disposition, and interactions of the constituent particles (atoms, electrons, nuclei, etc.). Quantum mechanics furnishes the latter information in terms of the elementary statistics to which the particles are subject, and via the energy levels f,- and their associated degeneracies g, among which the particles are distributed. Each such distribution corresponds to a possible macroscopic manifestation of the system. At equilibrium, it is the most probable distribution that prevails overwhelmingly as compared to any other configuration, and that corresponds to the maximum entropy of the macroscopic system. Deviations from this configuration are inevitable they come under the topic of fluctuations that are taken up in Section 1.17. However, the system away from equilibrium will spontaneously revert back to the most probable configuration. [Pg.41]

In previous chapters, we saw that the volume of an atom is taken up primarily by its electrons (Chapter 2) occupying quantum-mechanical orbitals (Chapter 7). We also saw that these orbitals do not have a definite boundary but represent only a statistical probability distribution for where the electron is found. So how do we define the size of an atom One way to define atomic radii is to consider the distance between nonbonding atoms that are in direct contact. For example, krypton can be frozen into a solid in which the krypton atoms are touching each other but are not bonded together. The distance between the centers of adjacent krypton atoms—which can be determined from the solid s density—is then twice the radius of a krypton atom. An atomic radius determined in this way is called the nonbonding atomic radius or the van der Waals radius. The van der Waals radius represents the radius of an atom when it is not bonded to another atom. [Pg.350]

For chemical kinetics, transition state theory is most useM in the form that starts from reactants in thermal equilibrium. For our purpose we want a more detailed version, that of reactants with a total energy in the range E oE + AE. If we know how to do that, we can and will average over a Boltzmann distribution in E to obtain the thermal results. The first task at hand is to define what is meant by reactants at equilibrium at a total energy within the range (and at given values of any other conserved quantum numbers). It is the foundation of statistical mechanics that equilibrium under such conditions means that all possible quantum states of the reactants are equally probable. ... [Pg.204]

Morante S, Rossi GC, Testa M (2006) The stress tensor of a molecular system an exercise in statistical mechanics. J Chem Phys 125 034101 66. Nelson DF, Lax M (1976) Asymmetric total stress tensor. Phys Rev B 13 1770-1776 Das A (1978) Stress tensor in a class of gauge theraies. Phys Rev D 18 2065-2067 Cohen L (1979) Local kinetic energy in quantum mechanics. J Chem Phys 70 788-789 Cohen L (1984) Representable local kinetic tmergy. J Chem Phys 80 4277-4279 Cohen L (1996) Local values in quantum mechanics. Phys Lett A 212 315-319 Ayers PW, Parr RG, Nagy A (2002) Local kinetic tmergy and local temperature in the density-functional theory of electronic structure. Int J Quantum Chem 90 309-326 Cohen L (1966) Generalized phase-space distribution functions. J Math Phys 7 781-786 Cohen L (1966) Can quantum mechanics be formulated as classical probability theory. Philos Sci 33 317-322... [Pg.123]

An underlying idea in the statistical mechanical analysis of chemical systems is that all quantum states with the same energy are equally probable. For any one molecule, or any one quantum mechanical system, there is no a priori reason to favor one state of a given energy over another. This is a postulate we take it to hold so long as there are no violations in the predictions that follow from it. This idea was invoked in Chapter 1 in the statistical analysis that lead to the Maxwell-Boltzmann distribution law (Equation 1.11), and in Chapter 9 we found one direct experimental confirmation of the distribution law in the... [Pg.344]

Next take an ensemble of replicas of a system, distributed over wave functions i (v) with probabilities wv. The il/(v) may be any set of normalized functions, not necessarily orthogonal to one another. An observable A has in each if/(v) a quantum-mechanical expectation (1.2), and the statistical average over the ensemble is... [Pg.424]

However, in quantum mechanics, as is well known, a particle cannot lie absolutely at rest on a certain point. That would contradict the uncertainty relation. According to quantum mechanics our isotropic oscillators, even in their lowest states, make a so-called zero-point motion which one can only describe statistically, for example, by a probability function which defines the probability with which any configuration occurs whilst one cannot describe the way in which the different configurations follow each other. For the isotropic oscillators these probability functions give a spherically symmetric distribution of configurations round the rest position. (The rare gases, too, have such a spherically symmetrical distribution for the electrons around the nucleus.)... [Pg.7]

Quantum mechanical, classical and statistical probabilities agree, on average, reasonably well with the experimental results [133] shown in Fig. 37 (vibrational distributions of NO were also measured by Harrison et al. [310]). In the experiment a high population of the state n o = 1 is found already 100 cm above its threshold. Moreover, the measured probabilities show some indications of fluctuations. Because of the limited number of data points, the inevitable incoherent averaging over several overall rotational states of NO2 and the averaging over the various possible electronic states of the 0 and NO products, these fluctuations are less pronounced than in the quantum mechanical calculations on a single adiabatic PES and for J = 0. [Pg.197]


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