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Pople-Walmsley defect

Figure 4 Structure of (a) a Pople-Walmsley and (b) a Su-Schrieffer-Heeger bond-alternation defect (soliton) in PA the changes in bond orders (a, dotted and b, full line) are shown underneath. The energy of PA as a function of bond order is shown in (c) the spin-charge (s-q) relations for different occupancy of the soliton energy-level are shown in (d)... Figure 4 Structure of (a) a Pople-Walmsley and (b) a Su-Schrieffer-Heeger bond-alternation defect (soliton) in PA the changes in bond orders (a, dotted and b, full line) are shown underneath. The energy of PA as a function of bond order is shown in (c) the spin-charge (s-q) relations for different occupancy of the soliton energy-level are shown in (d)...
Fig. 36.13. Top Pople and Walmsley misfit, bottom Su, Schrieffer and Heeger soliton defect. Fig. 36.13. Top Pople and Walmsley misfit, bottom Su, Schrieffer and Heeger soliton defect.
Pople and Walmsley considered that the energy required to form a pair of defects in the linear polyene molecule [H(CH=CH) H] is relatively low and should lead to a significant thermal population. They estimated the number of unpaired spins at about one per 70 carbon atoms at room temperature [26]. The observed values were much lower, 3.0 x 10 and 2.2 x 10 spin/g, for 97% trans- and 93% c7.v-polyacetylene, respectively, or one spin per 3000 and one per 10,000 carbon atoms, re-... [Pg.199]


See other pages where Pople-Walmsley defect is mentioned: [Pg.15]    [Pg.15]    [Pg.217]    [Pg.670]    [Pg.148]    [Pg.93]    [Pg.1024]    [Pg.2]    [Pg.39]    [Pg.98]    [Pg.222]    [Pg.240]   
See also in sourсe #XX -- [ Pg.15 ]




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