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Energy differences between states

There are two important feaUires of this result. The energy difference between states 1 and 2 is A = E2 E. Wlien AE hv, the denominator of the second tenn becomes very small, and this temi dominates. This is the well known... [Pg.1157]

This is die fonn diat chemists and physicists are most accustomed to. The probabilities are calculated from the Boltzmann equation and the energy difference between state t and state it — 1. Because we are using a ratio of probabilities, the normalization factor, i.e., the partition function, drops out of the equation. Another variant when 6 is multidimensional (which it usually is) is to update one component at a time. We define 6, = 6, i,... [Pg.327]

With these relationships and the appropriate experimental data we can plot reaction coordinate diagrams that are quantitatively useful in displaying the free energy differences between states. Figure 5-9 is an example, the data being drawn from Table 4-3, System 2. For this reversible reaction. [Pg.210]

Because the population ratio is determined by the appropriate Boltzmann expression where A is the energy difference between states and k is the... [Pg.102]

JE) and the Crooks fluctuation relation (Crooks FR). ° These relations not only provide a better understanding of the behaviour of nonequilibrium systems (in particular their irreversibility), but provide new practical results that apply to many-particle systems including derivations of transport properties (viscosity, thermal conductivity and shear viscosity) and completely new ways of calculating free energy differences between states and determining potentials of mean force. [Pg.181]

Hummer and Szabo" demonstrated that in single molecule stretching experiments, the JE provides an expression for the work at different times, whereas from an experimental point of view it is of more interest to know the free energy difference between states at different extensions of the molecule. They show how this can be obtained and apply it in experiments. [Pg.200]

In this book, the major use for the energy differences between states will be in the treatment of transition-metal ions by the crystal and ligand field theories. Thus, further discussion of the energies will be deferred until then (Chapter 20). [Pg.85]

The Racah parameters are measures of the energy separations of the various Russcll-Saundcrs states of an atom. The energy differences between states of the same spin multiplicity are, in general, multiples of B only, whereas the differences between states of different multiplicity are expressed... [Pg.604]

The lowest levels of the 5f 6d manifold are shown in Table 7 and Fig. 10. The calculated minimum-to-minimum transition energies from the ground state as calculated with the same level of theory, 5f 1 rgu( l9/2), are shown together with the experimental zero-phonon levels [88] referred to the experimental ground state, which is the same as that theoretically predicted. The results referred to the lowest state of the 5f 6d manifold, 1 Tgg, are also shown in order to enhance the energy differences between states of the same excited configuration. The three electronic origins that have been detected in the experiments at 14157, 15682, and 16528 cm and appear in the table are indicated by vertical arrows in... [Pg.467]

To compute free energy differences between states with little overlap, it will usually be more efficient to compute the free energy along a pathway of intermediate states. Free energy calculations can be made significantly more efficient by optimizing the choice of intermediate states for increased phase space overlap [36, 59-61],... [Pg.46]

Molecular dynamics simulations can also be used to compute the free energy difference between state a and state b using the following formula. [Pg.175]

The concept of thermodynamic cycles is based on the status of the free energy as a thermodynamic state function. Therefore, free energy differences between states of a system are independent of the particular path followed to... [Pg.95]

Fig. 5.5 Absorption spectra (Im[a]) of the L-shaped dimer model in the presence of a coupling field resonating with the energy difference between states 2(3) and 5 (tuc = 19,976 cm ) (a) and with that between states 2(3) and 6 (tuc = 20,024 cm ) (b). The inserted numbers (2, 3, 5, 6) represent the indices of the excited states... Fig. 5.5 Absorption spectra (Im[a]) of the L-shaped dimer model in the presence of a coupling field resonating with the energy difference between states 2(3) and 5 (tuc = 19,976 cm ) (a) and with that between states 2(3) and 6 (tuc = 20,024 cm ) (b). The inserted numbers (2, 3, 5, 6) represent the indices of the excited states...
According to the diagram, the activation energy of the slow step is given by the energy difference between states... [Pg.183]


See other pages where Energy differences between states is mentioned: [Pg.1553]    [Pg.268]    [Pg.289]    [Pg.175]    [Pg.685]    [Pg.121]    [Pg.555]    [Pg.3]    [Pg.219]    [Pg.227]    [Pg.151]    [Pg.19]    [Pg.386]    [Pg.2714]    [Pg.53]    [Pg.182]    [Pg.5]    [Pg.685]    [Pg.569]    [Pg.189]    [Pg.73]    [Pg.1553]    [Pg.256]    [Pg.385]    [Pg.2713]    [Pg.428]    [Pg.436]    [Pg.215]    [Pg.22]    [Pg.448]    [Pg.203]    [Pg.123]    [Pg.117]    [Pg.295]    [Pg.33]   
See also in sourсe #XX -- [ Pg.147 ]




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