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Barrier states

The SQ method extracts resonance states for the J = 25 dynamics by using the centrifugally-shifted Hamiltonian. In Fig. 20, the SQ wavefunc-tion for a trapped state at Ec = 1.2 eV is shown. The wavefunction has been sliced perpendicular to the minimum energy path and is plotted in the symmetric stretch and bend normal mode coordinates. As anticipated, the wavefunction shows a combination of one quanta of symmetric stretch excitation and two quanta of bend excitation. The extracted state is barrier state (or quantum bottleneck state) and not a Feshbach resonance. [Pg.78]

If the localized electron tunnels out through the barrier (state 1 in Fig. 12 b) a certain amount of f-f overlapping is present. States like 1 in Fig. 12 b are called sometimes resonant states or "virtually bound" states. In contrast with case 2 in Fig. 12b, which we may call of full localization , the wave function of a resonant state does not die out rapidly, but keeps a finite amplitude in the crystal, even far away from the core. For this reason, overlapping may take place with adjacent atoms and a band may be built as in ii. (If the band formed is a very narrow band, sometimes the names of localized state or of resonance band are employed, too. Attention is drawn, however, that in this case one refers to a many-electron, many-atoms wave function of itinerant character in the sense of band theory whereas in the case of resonant states one refers to a one-electron state, bound to the central potential of the core (see Chap. F)). [Pg.28]

One expects to observe a barrier resonance associated with each vibra-tionally adiabatic barrier for a given chemical reaction. Since the adiabatic theory of reactions is closely related to the rate of reaction, it is perhaps not surprising that Truhlar and coworkers [44, 55] have demonstrated that the cumulative reaction probability, NR(E), shows the influence barrier resonances. Specifically, dNR/dE shows peaks at each resonance energy and Nr(E) itself shows a staircase structure with a unit step at each QBS energy. It is a more unexpected result that the properties of the QBS seem to also imprint on other reaction observables such as the state-to-state cross sections [1,56] and even can even influence the helicity states of the products [57-59]. This more general influence of the QBS on scattering observables makes possible the direct verification of the existence of barrier-states based on molecular beam experiments. [Pg.127]

The calculated energy difference between the ground state and the barrier state is less than 0.2 eV for most of the perovskites studied, which is much less than the experimentally observed... [Pg.246]

We now define an effective Hamiltonian matrix in the subspace of the barrier states (a TV x TV matrix)... [Pg.345]

Figure 4.1 Illustration of the pump-dump scheme for a slightly asymmetric one-dimensional double minimum potential. In a first step a pump pulse excites the system from the initial state an above-the-barrier state From there a second pulse dumps the population into the target state Pf. Figure 4.1 Illustration of the pump-dump scheme for a slightly asymmetric one-dimensional double minimum potential. In a first step a pump pulse excites the system from the initial state an above-the-barrier state From there a second pulse dumps the population into the target state Pf.
A Support Safety Barrier (SSB) contributes to the adequate function of the Primary Safety Barriers and influence the probability with which the primary safety barrier-states occur. Support Safety Barriers for contact with moving parts of a machine are ... [Pg.705]

The equilibrium states in Fig. 3 can be listed in the likely order in which they are physically encountered as the air is trapped in the cavity (Fig. 4). This order gives the possible stable and barrier (unstable) states. For example, when > 0.67, the Cassie-Baxter state will be encountered first followed by the first equilibrium state, the second equilibrium state, the bubble state and lastly the Wenzel state (Fig. 4). Thus, the first equilibrium and the bubble states are expected to be the energy barrier states that separate the remaining stable equilibrium states. Similarly, for 0 < 0.67 the bubble state is expected to be the barrier state. These expectations will be checked below by exploring a part of the energy landscape and finding the minimum (or stable) energy states. [Pg.62]

There are two types of situations in Table 1 or Fig. 3 — one with five equilibrium states and the other with three. Fcav vs % is plotted for one case of each type in Fig. 5a and 5b. Figure 5a shows the five equilibrium states case at Co = 0.88 (i.e. 00 = 40.5°). It is seen that the Cassie-Baxter state at 0h = 0o = 40.5° is a border minimum. If the liquid-air interface moves in, at mechanical equilibrium, as assumed here, then the energy Ecav increases until it reaches a maximum value at 0H = Thus, represents the energy barrier state where the equi-... [Pg.63]

Fig. 12.17 Berreman-Heffner bistable cell. Director configuration of the cell with two stable states (unwound with n = 0 and twisted with n = 2 half-turns) in the absence of field and the barrier state S in a weak electric field... Fig. 12.17 Berreman-Heffner bistable cell. Director configuration of the cell with two stable states (unwound with n = 0 and twisted with n = 2 half-turns) in the absence of field and the barrier state S in a weak electric field...
Fig. 12.18 Zero field free energy of the states with different number of half turns n as a function of cell thickness d normalized to pitch Pg. Solid lines show the energy of the two stable states to be switched. Low energy (n = 1) state is excluded from consideration for topological reasons. B marks the high energy barrier state playing the dominant role in the field-on state... Fig. 12.18 Zero field free energy of the states with different number of half turns n as a function of cell thickness d normalized to pitch Pg. Solid lines show the energy of the two stable states to be switched. Low energy (n = 1) state is excluded from consideration for topological reasons. B marks the high energy barrier state playing the dominant role in the field-on state...
Fig. 12.19 Voltage dependence of the free energy for the uniform (n = 0) and twisted (n = 2) states. R is the turn point from the barrier state to one of the two stable initial states... Fig. 12.19 Voltage dependence of the free energy for the uniform (n = 0) and twisted (n = 2) states. R is the turn point from the barrier state to one of the two stable initial states...
But how to force the system relax to a particular state selected by an experimentalist Berreman and Heffner [20] suggested to exploit the backflow ejfect discussed in Section. 11.2.6. We know that, upon relaxation of the director from the field-ON quasi-homeotropic state (barrier state B) to a field-OFF state, a flow appears within the cell. The direction of the flow depends on the curvature of the director field, which is more pronounced near the electrodes. Moreover it has the opposite sign at the top and bottom electrodes, see the molecules distribution in state B in Fig. 12.17. Due to this, the close-to-electrode flows create a strong torque exerted on the director mostly in the middle of the cell that holds the director to be more or less parallel to the boundaries in favour of the n = 2) initial state in Fig. 12.17. [Pg.373]


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See also in sourсe #XX -- [ Pg.48 ]




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