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Canonical system

There are two further usefiil results related to ((N-(N)) ). First is its coimection to the isothennal compressibility = -V dP/8V) j j, and the second to the spatial correlations of density fluctuations in a grand canonical system. ... [Pg.420]

For most practical applications, we consider not isolated systems but systems in which the temperature is fixed. This is the canonical system consistent with the fixed macroscopic properties (N, V, T), where T is the absolute temperature. [Pg.291]

We consider a canonical system of N interacting particles described by the N-body Hamiltonian HN. In such a system the energy is not fixed. We shall not give the detailed derivation here but merely state that the probability that the system is found in the th energy state given as an eigenvalue of the /V-body Hamiltonian, is... [Pg.291]

Although one could continue to demonstrate the virtues of the proposed nomenclature for the remaining boranes in [2], the models that have been postulated for each such structure seem to be getting further removed from what is truly known about the relevant geometry and topology of the respective compounds. Consequently, although the proposed system of nomenclature addressed the problem, which the presently accepted system did only belatedly and with an extremely convoluted set of terms, locant numbers, etc., it s further development must await until more laboratory results are accumulated. In the present state of knowledge, it is more speculative than is desirable for any canonical system of "scientific" nomenclature. [Pg.200]

Fig. 14 A picture of the previous regularly crosslinked polymer which emphasizes the designated cyclic monomer, while maintaining the divisions of the tessellated plane. This model produces the canonical systemic name... Fig. 14 A picture of the previous regularly crosslinked polymer which emphasizes the designated cyclic monomer, while maintaining the divisions of the tessellated plane. This model produces the canonical systemic name...
In more usual notations and words, the problem is to investigate the dynamics of a canonical system of differential equations with Hamiltonian... [Pg.3]

Canonical perturbation theory for nearly integrable systems Theorem 4 Consider a canonical system with Hamiltonian... [Pg.14]

Secondly, for any closed line L the area Qt for the canonical system (A 10) is constant. Indeed, substituting in the integrand in (A9) for P = = —8H/8y, Q = +8H/8x we obtain d/dt Qt = 0. This result is known as the Liouville theorem. A consequence of the Liouville theorem is non--existence of stationary points of a node or focus type for a canonical... [Pg.205]

As an unperturbed system we will take the canonical system... [Pg.251]

Let us now calculate the pressure in the system. For a canonical system, we have... [Pg.334]

In an analogous way, for a grand canonical system, we can define the pressure by setting... [Pg.334]

Unfortunately, this approximation cannot be generalized directly. We shall come back to this matter in the context of the diagram expansions of grand canonical systems and we shall note that the approximation used above coincides with the simple-tree approximation. [Pg.682]

The valuable expressions in terms of the partition function of a canonical system are presented in Table 2.8. [Pg.121]

For the system of equivalent but distinguishable particles (as in the solid state) the total partition function of a canonical system for one mole of particles becomes... [Pg.558]

The Lindemann mechanism consists of three reaction steps. Reactions (1.4) and (1.5) are bimolecular reactions so that the true unimolecular step is reaction (1.6). Because the system described by Eqs. (1.4)-(l. 6) is at some equilibrium temperature, the high-pressure unimolecular rate constant is the canonical k T). This can be derived by transition state theory in terms of partition functions. However, in order to illustrate the connection between microcanonical and canonical systems, we consider here the case of k(E) and use Eq.(1.3) to convert to k(T). [Pg.7]

We began this chapter by considering the phase space volume and surface area which are related to the sum and density of states for a system at a given total energy E, that is, a microcanonical system. This is the system of major interest in this book. However, during the discussion of several topics it will be necessary to make use of the partition function, which is appropriate for constant-temperature, or canonical, systems. Because the partition functions for translations, rotations, and vibrations are derived in all undergraduate physical chemistry texts, we will not derive them here, but simply summarize the results. [Pg.178]

He or, more generally, a distribution. For a canonical system there is no longer a constraint of the form // = E and thus we must allow the phase space to include essentially all points for which the position coordinates lie in the defined configurational domain (a 3-torus, if periodic boundary conditions are used). In general the momenta are unbounded. It thus becomes necessary to restrict the set of functions on which the functional -, p) acts. In the case of periodic boundary conditions we will assume that, for any observable of interest. [Pg.220]

Abstract Fluctuation Theory of Solutions or Fluctuation Solution Theory (FST) combines aspects of statistical mechanics and solution thermodynamics, with an emphasis on the grand canonical ensemble of the former. To understand the most common applications of FST one needs to relate fluctuations observed for a grand canonical system, on which FST is based, to properties of an isothermal-isobaric system, which is the most common type of system studied experimentally. Alternatively, one can invert the whole process to provide experimental information concerning particle number (density) fluctuations, or the local composition, from the available thermodynamic data. In this chapter, we provide the basic background material required to formulate and apply FST to a variety of applications. The major aims of this section are (i) to provide a brief introduction or recap of the relevant thermodynamics and statistical thermodynamics behind the formulation and primary uses of the Fluctuation Theory of Solutions (ii) to establish a consistent notation which helps to emphasize the similarities between apparently different applications of FST and (iii) to provide the working expressions for some of the potential applications of FST. [Pg.2]

Several variations of ordinary MD have been developed. Andersen has proposed "molecular dynamics at constant temperature," in which an MD system is made to represent a canonical system, by altering the momentum of random particles at sequential random Instants of time. The new momentum is picked from a Boltzmann distribution, with a given parameter p. Since the motion of the system is no longer Hamiltonian, this procedure is a statistical sampling method. A combination technique was used by Wood and Erpenbeck, who ran a set of independent MD calculations, with the initial phase of each calculatlon glcked from a canonical, or mlcrocanonical, distribution. Andersen also described molecular dynamics at constant pressure," in which the pressure is a parameter of the Lagranglan, and the system volume fluctuates. [Pg.559]


See other pages where Canonical system is mentioned: [Pg.232]    [Pg.232]    [Pg.238]    [Pg.149]    [Pg.310]    [Pg.310]    [Pg.20]    [Pg.9]    [Pg.261]    [Pg.270]    [Pg.311]    [Pg.282]    [Pg.479]    [Pg.138]    [Pg.3]    [Pg.23]    [Pg.42]    [Pg.205]    [Pg.270]    [Pg.332]    [Pg.333]    [Pg.349]    [Pg.420]    [Pg.331]    [Pg.343]    [Pg.249]    [Pg.127]    [Pg.108]    [Pg.52]    [Pg.37]   
See also in sourсe #XX -- [ Pg.291 ]




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