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Transitional space

From Figure 5.3 it is apparent that transition intensities are not equal and, from Table 5.1, that the transition spacings show a slight decrease as J" increases. We will now consider the reasons for these observations. [Pg.110]

In contemporary terms, we might see this plate as suggestive of the importance of holding and play for transformation, and we might even see this room as an image of D.W.Winnicott s concept of transitional space ... [Pg.154]

Sometimes, a space is left between the end of the screw(s) and the die plate. If rheological properties of the material are such that further densification takes place in this transition space, a denser extrudate is produced. In most cases, a large gap is used in high pressure screw extruders (see Section 8.4.3) where the necessary forces to obtain extrusion are solely developed by the screw(s) and high hydrostatic pressure is required to induce hydraulic flow through the extrusion channel(s). In low pressure axial extruders, extrusion blades are commonly attached to the end of the screw shaft (Fig. 8.27). In those cases, the gap is small and the plastic mass is compressed in the... [Pg.260]

Figure 8.4 NaOsOy (a) projection down [010] of the structure (b) the G-type antiferromagnetic ordering below the metal-insulator transition (space group Pnma)... Figure 8.4 NaOsOy (a) projection down [010] of the structure (b) the G-type antiferromagnetic ordering below the metal-insulator transition (space group Pnma)...
Seven-dimensional Phase Transitional Space for Protein-based Polymer Function as Molecular Machines... [Pg.124]

The position of the T,-divide that separates soluble from insoluble (hydrophobically associated) states in the phase diagram depends on seven variables on the six intensive variables of temperature, chemical potential, electrochemical potential, mechanical force, pressure, and electromagnetic radiation, and on polymer volume fraction or concentration. Therefore, diverse protein-catalyzed energy conversions by the consilient mechanism result from designs that control the location of the Tfdivide in this seven-dimensional phase transitional space. Complete mathematical description has yet to be written for representation of the T,-divide in seven-dimensional phase transitional space, but it may prove to be more relevant to... [Pg.124]

Ghaddar, N., Ghali, K., Chehaitly, S., 2011. Assessment thermal comfort of active people in transitional spaces in presence of air movement. Energy Build. 43, 2832-2842, Elsevier. [Pg.105]

But no other field in condensed matter physics has shown such a rich variety of continuous or weakly first-order phase transitions than liquid crystals order parameters of various symmetries, anisotropic scaling behaviors, coupled order parameters, multicritical points, wide critical domains, defect mediated transitions, spaces of low dimensionality, multiply reentrant topologies are currently found in liquid crystals, at easily accessible temperatures. Beside their famous technical applications in optics... [Pg.314]

The solutions can be labelled by their values of F and m.p. We say that F and m.p are good quantum. num.bers. With tiiis labelling, it is easier to keep track of the solutions and we can use the good quantum numbers to express selection rules for molecular interactions and transitions. In field-free space only states having the same values of F and m.p can interact, and an electric dipole transition between states with F = F and F" will take place if and only if... [Pg.140]

Finally the concept of fields penults clarification of the definition of the order of transitions [22]. If one considers a space of all fields (e.g. Figure A2.5.1 but not figure A2.5.3, a first-order transition occurs where there is a discontinuity in the first derivative of one of the fields with respect to anotlier (e.g. (Sp/S 7) = -S... [Pg.649]

It has long been known from statistical mechanical theory that a Bose-Einstein ideal gas, which at low temperatures would show condensation of molecules into die ground translational state (a condensation in momentum space rather than in position space), should show a third-order phase transition at the temperature at which this condensation starts. Nonnal helium ( He) is a Bose-Einstein substance, but is far from ideal at low temperatures, and the very real forces between molecules make the >L-transition to He II very different from that predicted for a Bose-Einstein gas. [Pg.661]

The photoelectron spectrum of FH,is shown in figure A3.7.6 [54]. The spectrum is highly structured, showing a group of closely spaced peaks centred around 1 eV, and a smaller peak at 0.5 eV. We expect to see vibrational structure corresponding to the bound modes of the transition state perpendicular to the reaction coordinate. For this reaction with its entrance chaimel barrier, the reaction coordinate at the transition state is... [Pg.878]

A situation that arises from the intramolecular dynamics of A and completely distinct from apparent non-RRKM behaviour is intrinsic non-RRKM behaviour [9], By this, it is meant that A has a non-random P(t) even if the internal vibrational states of A are prepared randomly. This situation arises when transitions between individual molecular vibrational/rotational states are slower than transitions leading to products. As a result, the vibrational states do not have equal dissociation probabilities. In tenns of classical phase space dynamics, slow transitions between the states occur when the reactant phase space is metrically decomposable [13,14] on the timescale of the imimolecular reaction and there is at least one bottleneck [9] in the molecular phase space other than the one defining the transition state. An intrinsic non-RRKM molecule decays non-exponentially with a time-dependent unimolecular rate constant or exponentially with a rate constant different from that of RRKM theory. [Pg.1011]

In deriving the RRKM rate constant in section A3.12.3.1. it is assumed that the rate at which reactant molecules cross the transition state, in the direction of products, is the same rate at which the reactants fonn products. Thus, if any of the trajectories which cross the transition state in the product direction return to the reactant phase space, i.e. recross the transition state, the actual unimolecular rate constant will be smaller than that predicted by RRKM theory. This one-way crossing of the transition state, witii no recrossmg, is a fiindamental assumption of transition state theory [21]. Because it is incorporated in RRKM theory, this theory is also known as microcanonical transition state theory. [Pg.1015]

The intennolecular Hamiltonian of the product fragments is used to calculate the sum of states of the transitional modes, when they are treated as rotations. The resulting model [28] is nearly identical to phase space theory [29],... [Pg.1016]

The bulk of the infomiation about anhannonicity has come from classical mechanical calculations. As described above, the aidiannonic RRKM rate constant for an analytic potential energy fiinction may be detemiined from either equation (A3.12.4) [13] or equation (A3.12.24) [46] by sampling a microcanonical ensemble. This rate constant and the one calculated from the hamionic frequencies for the analytic potential give the aidiannonic correctiony j ( , J) in equation (A3.12.41). The transition state s aidiannonic classical sum of states is found from the phase space integral... [Pg.1021]

As discussed in section A3.12.2. intrinsic non-RRKM behaviour occurs when there is at least one bottleneck for transitions between the reactant molecule s vibrational states, so drat IVR is slow and a microcanonical ensemble over the reactant s phase space is not maintained during the unimolecular reaction. The above discussion of mode-specific decomposition illustrates that there are unimolecular reactions which are intrinsically non-RRKM. Many van der Waals molecules behave in this maimer [4,82]. For example, in an initial microcanonical ensemble for the ( 211 )2 van der Waals molecule both the C2H4—C2H4 intennolecular modes and C2H4 intramolecular modes are excited with equal probabilities. However, this microcanonical ensemble is not maintained as the dimer dissociates. States with energy in the intermolecular modes react more rapidly than do those with the C2H4 intramolecular modes excited [85]. [Pg.1037]

Muns ENDOR mvolves observation of the stimulated echo intensity as a fimction of the frequency of an RE Ti-pulse applied between tlie second and third MW pulse. In contrast to the Davies ENDOR experiment, the Mims-ENDOR sequence does not require selective MW pulses. For a detailed description of the polarization transfer in a Mims-type experiment the reader is referred to the literature [43]. Just as with three-pulse ESEEM, blind spots can occur in ENDOR spectra measured using Muns method. To avoid the possibility of missing lines it is therefore essential to repeat the experiment with different values of the pulse spacing Detection of the echo intensity as a fimction of the RE frequency and x yields a real two-dimensional experiment. An FT of the x-domain will yield cross-peaks in the 2D-FT-ENDOR spectrum which correlate different ENDOR transitions belonging to the same nucleus. One advantage of Mims ENDOR over Davies ENDOR is its larger echo intensity because more spins due to the nonselective excitation are involved in the fomiation of the echo. [Pg.1581]

Figure Bl.19.22. Magnetic force microscopy image of an 8 pm wide track on a magnetic disk. The bit transitions are spaced every 2 pm along the track. Arrows point to the edges of the DC-erased region. (Taken from [109], figure 7.)... Figure Bl.19.22. Magnetic force microscopy image of an 8 pm wide track on a magnetic disk. The bit transitions are spaced every 2 pm along the track. Arrows point to the edges of the DC-erased region. (Taken from [109], figure 7.)...
For a coupled spin system, the matrix of the Liouvillian must be calculated in the basis set for the spin system. Usually this is a simple product basis, often called product operators, since the vectors in Liouville space are spm operators. The matrix elements can be calculated in various ways. The Liouvillian is the conmuitator with the Hamiltonian, so matrix elements can be calculated from the commutation rules of spin operators. Alternatively, the angular momentum properties of Liouville space can be used. In either case, the chemical shift temis are easily calculated, but the coupling temis (since they are products of operators) are more complex. In section B2.4.2.7. the Liouville matrix for the single-quantum transitions for an AB spin system is presented. [Pg.2099]


See other pages where Transitional space is mentioned: [Pg.111]    [Pg.215]    [Pg.304]    [Pg.584]    [Pg.111]    [Pg.105]    [Pg.215]    [Pg.544]    [Pg.111]    [Pg.215]    [Pg.304]    [Pg.584]    [Pg.111]    [Pg.105]    [Pg.215]    [Pg.544]    [Pg.50]    [Pg.356]    [Pg.407]    [Pg.117]    [Pg.283]    [Pg.723]    [Pg.51]    [Pg.656]    [Pg.659]    [Pg.778]    [Pg.779]    [Pg.781]    [Pg.858]    [Pg.878]    [Pg.1016]    [Pg.1069]    [Pg.1120]    [Pg.1236]    [Pg.1456]    [Pg.1751]   
See also in sourсe #XX -- [ Pg.155 ]




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Active space, transition metal compounds

Angular momentum, phase-space transition state

Angular momentum, phase-space transition state geometry

Angular momentum, phase-space transition state potential

Chaotic transitions phase-space transition states

Dimensionality phase-space transition states

Hamiltonian systems phase-space transition states

Hyperbolicity phase-space transition states

Invariant structures phase-space transition states

Kinetic energy phase-space transition states

Linearization, phase-space transition state

Nonlinear dynamics phase-space transition states

Normally hyperbolic invariant manifolds phase-space transition states

Perturbation theory phase-space transition states

Phase Transitions in Confined Spaces

Phase space theory orbiting transition state

Phase-space transition states

Phase-space transition states Hamiltonian dynamics

Phase-space transition states Melnikov integral

Phase-space transition states additional potentials

Phase-space transition states atomic clusters

Phase-space transition states breakdown

Phase-space transition states dimensions

Phase-space transition states examples

Phase-space transition states general equations

Phase-space transition states momentum

Phase-space transition states nonlinearities

Phase-space transition states reaction paths

Phase-space transition states relative equilibrium

Phase-space transition states stationary points

Phase-space transition states structure

Phase-space transition states temperature

Relative equilibria , phase-space transition

Saddle regions phase-space transition states

Stable/unstable manifolds phase-space transition states

Tangency, phase-space transition states

Temperature dependence phase-space transition states

Time scales phase-space transition states

Time-dependent equations phase-space transition states

Trajectory space, transition path ensemble

Trajectory space, transition path ensemble sampling

Transition intensities space selection

Transition metals active space selection

Vibrational frequency phase-space transition states

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