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The average energy

We already know that the average kinetic energy is 3/2)NkBT, so once the average potential energy has been calculated we will have a full microscopic expression for the macroscopic energy of the system. This average potential energy is [Pg.184]

Using again the definition of the pair correlation fiinction g, this leads to = y /r2g(ri2)M(ri2) [Pg.185]

The last equality holds for an isotropic and homogeneous system. This result can be understood intuitively For each of the N particles in the system (taken to be at the origin), the potential energy is obtained as a volume integral over the density of interaction energy associated with this particle. The latter is pg(r) (density of other particles at position r), multiplied by u(r). This will lead to double-counting of all interactions and should therefore be divided by 2. The result is (5.37). [Pg.185]


Each hamionic temi in the Hamiltonian contributes k T to the average energy of the system, which is the theorem of the equipartition of energy. Since this is also tire internal energy U of the system, one can compute the heat capacity... [Pg.392]

Given such a reference, we can classify various mechanisms of energy transfer either by the probability tiiat a certain energy transfer process will occur in a Leimard-Jones reference collision , or by the average energy transferred by one Leimard-Jones collision . [Pg.1054]

Experimental access to the probabilities P(E ,E) for energy transfer in large molecules usually involves teclmiques providing just the first moment of this distribution, i.e. the average energy (AE) transferred in a collision. Such methods include UV absorption, infrared fluorescence and related spectroscopic teclmiques [11. 28. 71. 72, 73 and 74]. More advanced teclmiques, such as kinetically controlled selective ionization (KCSI [74]) have also provided infonnation on higher moments of P(E ,E), such as ((AE) ). [Pg.1055]

Figure A3.13.7. Continuation of the time evolution for the CH eln-omophore in CHF after 90 fs of irradiation (see also figure A3,13,6). Distanees between tire eontoiir lines are 10, 29, 16 and 9 x 10 rr in the order of the four images shown. The averaged energy of the wave paeket eorresponds to 9200 em (roughly 6300 em absorbed) with a quantum meehanieal imeertainty of +5700 enC (from [97]). Figure A3.13.7. Continuation of the time evolution for the CH eln-omophore in CHF after 90 fs of irradiation (see also figure A3,13,6). Distanees between tire eontoiir lines are 10, 29, 16 and 9 x 10 rr in the order of the four images shown. The averaged energy of the wave paeket eorresponds to 9200 em (roughly 6300 em absorbed) with a quantum meehanieal imeertainty of +5700 enC (from [97]).
Temperature appears in the partition fiinction in an unusual way. The average energy takes the fomi... [Pg.2274]

What is the average energy release per bond on breaking bonds in cubane Compare this with the energy released on hydrogenation of ethylene. [Pg.332]

In other words, the lower the mass of the particle, the higher its velocity, because the average energy of any particle at a given temperature is constant, kT. A dispersed particle is always in random thermal motion (Brownian motion) due to coUisions with other particles and with the walls of the container (4). If the particles coUide with enough energy and are not well dispersed, they will coagulate or flocculate. [Pg.147]

Turbulent velocity fluctuations ultimately dissipate their kinetic energy through viscous effects. MacroscopicaUy, this energy dissipation requires pressure drop, or velocity decrease. The ener dissipation rate per unit mass is usually denoted . For steady ffow in a pipe, the average energy dissipation rate per unit mass is given by... [Pg.671]

In the Self Penalty Walk (SPW) method the whole reaction path is approximated by minimizing the average energy along the path, given as a line integral between the reactant and product geometries (R and P). [Pg.330]

A measure of the average energy of the molecules of a substance. The heat intensity. [Pg.436]

FIGURE 7.10 More energy levels become accessible in a lx>x of fixed width as the temperature is raised. The change from part (a) to part (b) is a model of the effect of heating an ideal gas at constant volume. The thermally accessible levels are shown by the tinted band. The average energy of the molecules also increases as the temperature is raised that is, both internal energy and entropy increase with temperature. [Pg.400]


See other pages where The average energy is mentioned: [Pg.424]    [Pg.95]    [Pg.376]    [Pg.409]    [Pg.533]    [Pg.547]    [Pg.1021]    [Pg.1067]    [Pg.2010]    [Pg.3011]    [Pg.316]    [Pg.80]    [Pg.316]    [Pg.34]    [Pg.392]    [Pg.398]    [Pg.107]    [Pg.2401]    [Pg.181]    [Pg.59]    [Pg.401]    [Pg.246]    [Pg.161]    [Pg.432]    [Pg.238]    [Pg.325]    [Pg.433]    [Pg.433]    [Pg.434]    [Pg.59]    [Pg.26]    [Pg.547]    [Pg.464]    [Pg.228]    [Pg.473]    [Pg.187]    [Pg.801]    [Pg.835]    [Pg.950]   


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Energy average

Energy-conserving path-branching with the force averaging

Existence of the Free Energy and Self-Averaging

Quantum-Mechanical Average Value of the Potential Energy

The Absolute Entropy and Free Energy as Ensemble Averages

The average binding energy per nucleon

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