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Quantum distributions thermal equilibrium

Nitrosobenzene was studied by NMR and UV absorption spectra at low temperature146. Nitrosobenzene crystallizes as its dimer in the cis- and fraws-azodioxy forms, but in dilute solution at room temperature it exists only in the monomeric form. At low temperature (—60 °C), the dilute solutions of the dimers could be obtained because the thermal equilibrium favours the dimer. The only photochemistry observed at < — 60 °C is a very efficient photodissociation of dimer to monomer, that takes place with a quantum yield close to unity even at —170 °C. The rotational state distribution of NO produced by dissociation of nitrosobenzene at 225-nm excitation was studied by resonance-enhanced multiphoton ionization. The possible coupling between the parent bending vibration and the fragment rotation was explored. [Pg.806]

The quantum concept was introduced by Max Planck in 1900 to explain the distribution of energy radiated from a black body in thermal equilibrium with the surrounding. The idea that light travels as photons was originated by Einstein in 1905. [Pg.16]

Statistical mechanics gives the relation between microscopic information such as quantum mechanical energy levels and macroscopic properties. Some important statistical mechanical concepts and results are summarized in Appendix A. Here we will briefly review one central result the Boltzmann distribution for thermal equilibrium. [Pg.11]

For reactants in complete thermal equilibrium, the probability of finding a BC molecule in a specific quantum state, n, is given by the Boltzmann distribution (see Appendix A.l). Thus, in the special case of non-interacting molecules the probability PBC(n)y °f finding a BC molecule in the internal (electronic, vibrational, and rotational) quantum states with energy En is... [Pg.11]

We now proceed to develop a specific expression for the rate constant for reactants where the velocity distributions /a( )(va) and /B(J)(vB) for the translational motion are independent of the internal quantum state (i and j) and correspond to thermal equilibrium.4 Then, according to the kinetic theory of gases or statistical mechanics, see Appendix A.2.1, Eq. (A.65), the velocity distributions associated with the center-of-mass motion of molecules are the Maxwell-Boltzmann distribution, a special case of the general Boltzmann distribution law ... [Pg.26]

Schematic energy level diagrams for the most widely used probe methods are shown in Fig. 1. In each case, light of a characteristic frequency is scattered, emitted, and/or absorbed by the molecule, so that a measurement of that frequency serves to identify the molecule probed. The intensity of scattered or emitted radiation can be related to the concentration of the molecule responsible. From measurements on different internal quantum states (vibrational and/or rotational) of the system, a population distribution can be obtained. If that degree of freedom is in thermal equilibrium within the flame, a temperature can be deduced if not, the population distribution itself is then of direct interest. Schematic energy level diagrams for the most widely used probe methods are shown in Fig. 1. In each case, light of a characteristic frequency is scattered, emitted, and/or absorbed by the molecule, so that a measurement of that frequency serves to identify the molecule probed. The intensity of scattered or emitted radiation can be related to the concentration of the molecule responsible. From measurements on different internal quantum states (vibrational and/or rotational) of the system, a population distribution can be obtained. If that degree of freedom is in thermal equilibrium within the flame, a temperature can be deduced if not, the population distribution itself is then of direct interest.
At thermal equilibrium, the Boltzmann distribution determines the populations in various energy levels. For any two quantum states, the ratio of populations between the higher energy state and the lower energy state at equilibrium will always be ... [Pg.34]

Is there any reason to expect that there will be an excess of nuclei in the lower spin state The answer is a qualified yes. For any system of energy levels at thermal equilibrium, there will always be more particles in the lower state(s) than in the upper state(s). However, there will always be some particles in the upper state(s). What we really need is an equation relating the energy gap (AE) between the states to the relative populations of (numbers of particles in) each of those states. This time, quantum mechanics comes to our rescue in the form of the Boltzmann distribution ... [Pg.12]

This observation has importance when we take into account the irreversibility. Due to irreversibility, the damped oscillator proceeds to thermal equilibrium with the thermal bath. This thermal equilibrium can be characterized in terms of classical statistic theory. However, in classical statistics, random variables have a joint distribution function, which could exist in the case of quantum theory if the operators are compatible. The commutator relation (Equation (100)) is compatible this physical picture, but from Equations (100) and (101), we obtain... [Pg.65]

Consider a ballistic quantum dot between two metallic terminals. Their electronic reservoirs are held at the thermal equilibrium described by the Fermi-Dirac distribution... [Pg.640]

More importantly, a molecular species A can exist in many quantum states in fact the very nature of the required activation energy implies that several excited nuclear states participate. It is intuitively expected that individual vibrational states of the reactant will correspond to different reaction rates, so the appearance of a single macroscopic rate coefficient is not obvious. If such a constant rate is observed experimentally, it may mean that the process is dominated by just one nuclear state, or, more likely, that the observed macroscopic rate coefficient is an average over many microscopic rates. In the latter case k = Piki, where ki are rates associated with individual states and Pi are the corresponding probabilities to be in these states. The rate coefficient k is therefore time-independent provided that the probabilities Pi remain constant during the process. The situation in which the relative populations of individual molecular states remains constant even if the overall population declines is sometimes referred to as a quasi steady state. This can happen when the relaxation process that maintains thermal equilibrium between molecular states is fast relative to the chemical process studied. In this case Pi remain thermal (Boltzmann) probabilities at all times. We have made such assumptions in earlier chapters see Sections 10.3.2 and 12.4.2. We will see below that this is one of the conditions for the validity of the so-called transition state theory of chemical rates. We also show below that this can sometime happen also under conditions where the time-independent probabilities Pi do not correspond to a Boltzmann distribution. [Pg.485]

The distribution of speeds given in Equation 5.36 holds for all matter (solid, liquid, or gas) in thermal equilibrium, except for light molecules and atoms at very low temperatures, where quantum effects are large and the precise specification of the speed of a particle is limited by the Heisenberg uncertainty principle. [Pg.313]

Consider a system containing microscopic entities A in an evacuated space in thermal equilibrium at an absolute temperature, denoted T, expressed in K. The distribution of population quantum states i and j follows the classical distribution of Maxwell-Boltzmann ... [Pg.45]

Statistical physics considers the task of predicting the (often macroscopic) observables of a physical system from the knowledge of interactions between the (microscopic) constituents (such as atoms or molecules, or suitably defined subunits of a polymer chain, for instance). Consider, for example, a simple fluid of N particles in a box of volume V held at a temperature T in thermal equilibrium. In the framework of classical statistical mechanics (i.e., neglecting the quantum-mechanical effects), the average of any observable A (e.g., the total potential energy 7(X ) in the system or the pair distribution function of particles) is given by... [Pg.461]

Collision experiments with fast H atoms have been carried out using target molecules initially at thermal equilibrium, under experimental conditions suitable for application of the equations derived for short collision times [90], The experiments can be analyzed for specific electronic-vibrational transitions, for which the final rotational distributions are presented as functions of the final rotational energy Er or quantum number J rather than as a function of the amount of energy transfer e. Therefore, one should modify the Gaussian shaped double differential cross section to obtain an expression in terms of... [Pg.360]

As the solvent dynamics begin to play a role in ET, the thermal equilibrium distribution of the donor population may be broken down during ET. The case is similar to adiabatic chemical reactions in solvent. Kramers proposed a method to study the thermal rate of escape from a metastable state coupled to a dissipative environment (see the review article Ref. 67). Later, Poliak et al. formulated a unified theory-Kramers turnover theory, which covers the whole range of friction strength and is applicable to an arbitrary memory friction. The quantum tunneling was further incorporated by Rips and Poliak with use of parabolic approximation. Our strategy for ET is to extend the quantum... [Pg.311]

Thus, for changing an electronic state the nuclear configuration r is necessary for which 6i(r ) 8 j(r ). This configuration is called transitional. In a system, which is in the thermal equilibrium state, the probability of existence of some nuclear configuration is determined by the respective quantum-mechanical distribution function... [Pg.12]

The statistical distribution function (or Slatersum) expresses the relative probability of a spatial configuration of a quantum mechanical system of N molecules in equilibrium with its surroundings. For a system in thermal equilibrium Pjv, the probability that a given state of energy E, is occupied, is proportional to exp (—E,), where = IjkT. The constant of proportionality is Zm, where Zjv is partition function given by... [Pg.232]


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