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Statistics Maxwell-Boltzmann

Except at temperatures close to absolute zero, the (as will be shown) and the [Pg.300]

In this classical limit, we can compute A from the requirement that [Pg.300]

The total volume of a cell in phase space is Ax Ap = h, where Ax = V, the total volume of the system. Therefore, the number of cells of phase space between E and E + dE is [Pg.300]

Putting this in Equation 15.16 and replacing the sum with an integral, [Pg.300]

The B-E distribution applies to bosons (particles with integral spin) for which no restrictions are placed on the occupancy number. The negative 1 in the denominator allows the occupancy of the groimd state to get very large as T 0 which is known as Bose condensation. The transition of He to superfluid He-11 at 2.17 K (the so-called lambda transition) is an example of Bose condensation. [Pg.301]


Examining transition state theory, one notes that the assumptions of Maxwell-Boltzmann statistics are not completely correct because some of the molecules reaching the activation energy will react, lose excess vibrational energy, and not be able to go back to reactants. Also, some molecules that have reacted may go back to reactants again. [Pg.166]

The probability that an atom will successfully move can be estimated by using Maxwell-Boltzmann statistics. The probability p that an atom will move from one position of minimum energy to an adjacent position is... [Pg.232]

In a special case where g, nu Eq. (5.22) can be reduced to the corrected Maxwell-Boltzmann statistics (note the classical Maxwell-Boltzmann statistics is for distinguishable particles) as... [Pg.171]

Uk U k Up Velocity vector of phase k Fluctuating velocity vector of phase k Velocity vector of particles W mb Total number of possible arrangements for a certain set of in the corrected Maxwell-Boltzmann statistics... [Pg.238]

The Fermi-Dirac and Maxwell-Boltzmann statistical distribution functions are widely used in semiconductor physics, with the latter commonly used as an approximation to the former. The point of this problem is to make you familiar with these distribution functions their forms, their temperature dependencies, and under what conditions they become interchangeable. Throughout this problem, use the energy of silicon s valence band (Evb) as the zero of your energy scale. [Pg.82]

This velocity of the electron is independent of temperature, in contradiction to the Maxwell-Boltzmann statistic, which states that... [Pg.24]

Fig. V-2.—Distribution functions for Fermi-Dirac statistics (a) Maxwell-Boltzmann statistics (b) and Finstoin-Bose statistics (c). Fig. V-2.—Distribution functions for Fermi-Dirac statistics (a) Maxwell-Boltzmann statistics (b) and Finstoin-Bose statistics (c).
In Fermi-Dirac statistics each state can accommodate at most only two particles with opposed spins. In Bose-Einstein statistics, just as in the classical Maxwell-Boltzmann statistics, there is no limitation to the number of particles in a given state. In classical statistics the particles in the same state were assumed to be distinguishable one from the other. As this assumption has been shown in quantum theory to be incorrect the particles in the same state in Bose-Einstein quantum statistics are indistinguishable. Interchanges of two of the par-... [Pg.292]

Systems containing more than one identical particles are invariant under the interchange of these particles. The permutations form a symmetry group. If these particles have several degrees of freedom, the group theoretical analysis is essential to extract symmetry properties of the permissible physical states. Examples include Bose-Einstein, Fermi-Dirac, Maxwell-Boltzmann statistics, Pauli exclusion principle, etc. [Pg.6]

The statistics required in macroscopic physical chemistry at ambient temperatures are invariably Maxwell-Boltzmann statistics, the principles and application of which have been laid down in chapter 1.3. In a number of situations, especially in solids at not too high temperatures, the number of systems in an ensemble is not small compared to the number of quantum states, leading to degeneracies. Then Fermi-Dtrac statistics are needed. Equations (3.10.21) remain acceptable at high temperatures, though. [Pg.415]

Turning to electric fields and classical Maxwell-Boltzmann statistics, soluble analytical models now exist which allow calculations of non-degenerate electron densities as a function of thermodynamic state in intense electric fields (low density high temperature). Semiclassical methods are available for switching on atomic potentials to models studied presently, though numerical results are not yet available here. [Pg.89]

Let us investigate the nonrelativistic ideal gas of identical particles governed by the classical Maxwell-Boltzmann statistics in the framework of the Tsallis and Boltzmann-Gibbs statistical mechanics. [Pg.317]

Tet us consider the nonrelativistic ideal gas of N identical particles governed by the classical Maxwell-Boltzmann statistics in the framework of the Tsallis and Boltzmann-Gibbs statistics in the microcanonical ensemble. For this special model, the statistical weight (111) can be written as (see [6] and reference therein)... [Pg.324]

In other words, applying Maxwell—Boltzmann statistics (see, e.g., ref 83 for a general treatment) to the calculated energy differences leads to estimated probabilities of obtaining re and si insertion (eq 2). [Pg.297]

Ludwig Boltzmann (1844-1906), the Austrian physicist, is famous for his outstanding contributions to heat transfer, thermodynamics, statistical mechanics, and kinetic theory of gases. Boltzmann was a student of Josef Stefan and received his doctoral degree in 1866 under his supervision. The Stefan-Boltzmann law (1884) for black body radiation is the result of the associated work of Josef Stefan and Boltzmann in the field of heat transfer. Boltzmann s most significant works were in kinetic theory of gases in the form of Maxwell-Boltzmann distribution and Maxwell-Boltzmann statistics in classical statistical mechanics. [Pg.94]

Classically, the dependence of a number of objects with their energy-per-object is modeled with statistics. When objects are independent of each other (more exactly, are sulgected to independent probabilities of presence) and in suffidaitly large numbers for allowing the approximation of factorials by exponentials, this dependence is modeled by Maxwell-Boltzmann statistics. [Pg.76]

The mathematical formulation of the diffuse layer region was worked out by Gouy and Chapman and has been treated fully in several reviews [1,4, 7]. Maxwell-Boltzmann statistics were assumed to relate the concentration of ions at a specified position in the interface to its bulk concentration, and the electrostatic potential ... [Pg.161]


See other pages where Statistics Maxwell-Boltzmann is mentioned: [Pg.166]    [Pg.363]    [Pg.116]    [Pg.10]    [Pg.581]    [Pg.83]    [Pg.84]    [Pg.85]    [Pg.471]    [Pg.471]    [Pg.76]    [Pg.62]    [Pg.471]    [Pg.763]    [Pg.2353]    [Pg.107]    [Pg.429]    [Pg.299]    [Pg.560]    [Pg.504]    [Pg.461]    [Pg.1]    [Pg.32]    [Pg.62]    [Pg.158]    [Pg.364]   
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