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Carbon chain, model

However, a few moments of reflection (or access to a molecular model kit) should convince you that these are in fact equivalent to structures written previously. In particular, the first one, like isomer I, has a five-carbon chain in which no carbon atom is attached to more than two other carbons. The second structure, like II, has a four-carbon chain with one carbon atom bonded to three other carbons. Structures I, II, and III represent the three possible isomers of CsH12 there are no others. [Pg.581]

Cram s open-chain model 229 Cram s rule 229, 233 Cram chelate model 229 Cram cyclic model 229 Cram-Felkin-Anh model 191,207, 236 f 246 cubane 12,318 cyanoacetic acid 636 f. cyanohydrin, protected 145, 150 f. cyclic carbonate protection 541 f., 657, 659 f., 666, 670 cyclization -,6-endo 734 -, 5-exo 733 f. [Pg.791]

The Gibbs equation allows the amount of surfactant adsorbed at the interface to be calculated from the interfacial tension values measured with different concentrations of surfactant, but at constant counterion concentration. The amount adsorbed can be converted to the area of a surfactant molecule. The co-areas at the air-water interface are in the range of 4.4-5.9 nm2/molecule [56,57]. A comparison of these values with those from molecular models indicates that all four surfactants are oriented normally to the interface with the carbon chain outstretched and closely packed. The co-areas at the oil-water interface are greater (heptane-water, 4.9-6.6 nm2/molecule benzene-water, 5.9-7.5 nm2/molecule). This relatively small increase of about 10% for the heptane-water and about 30% for the benzene-water interface means that the orientation at the oil-water interface is the same as at the air-water interface, but the a-sulfo fatty acid ester films are more expanded [56]. [Pg.479]

The important issue of size effects was addressed by Karaborni and Siepmann [368]. They used the same chain model and other details employed in the Karaborni et al. simulations described earlier [362-365] and the 20-carbon chain. System sizes of 16, 64, and 256 molecules were employed with areas of 0.23, 0.25 and 0.27 nm molecule simulations with 64 molecules were also performed for areas ranging from 0.185 to 0.40 nm molecule . The temperature used was 275 K, as opposed to 300 K used in the previously discussed work by Karaborni et al. with the 20-carbon chain. At the smaller areas no significant system size dependence was found. However, the simulation at 0.27 nm molecule showed substantial differences between N = 64 and N = 256 in ordering and tilt angle. The 64-molecule system showed more order than the 256-molecule system and a slightly lower tilt angle. The pressure-area isotherm data for these simulations are not... [Pg.124]

A step closer toward realism is taken by off-lattice models in which the backbone is specified in some detail, while side chains, if they are represented at all, are taken to be single, unified spheres [44-50]. One indication that this approach is too simplistic was given in [51], which proved that for a backbone representation in which only Ca carbons were modeled, no contact potential could stabilize the native conformation of a single protein against its nonnative ( decoy ) conformations. However, Irback and co-workers were able to fold real protein sequences, albeit short ones, using a detailed backbone representation, with coarse-grained side chains modeled as spheres [49, 52-54]. [Pg.342]

Figure 2. The new species added to our chemical models of interstellar clouds. The species range in complexity from 10-64 carbon atoms and comprise the following groups of molecules linear carbon chains, monocyclic rings, tricyclic rings, and fullerenes. The synthetic pathways are also indicated. See ref. 83. Reproduced from the International Journal of Mass Spectrometry and Ion Processes, vol. 149/150, R.P.A. Bettens, Eric Herbst "The interstellar gas phase production of highly complex hydrocarbons construction of a model", pp 321-343 (1995) with kind permission from Elsevier Science-NL, Sara Burgerhartstraat 25,1055 KV, Amsterdam, The Netherlands. Figure 2. The new species added to our chemical models of interstellar clouds. The species range in complexity from 10-64 carbon atoms and comprise the following groups of molecules linear carbon chains, monocyclic rings, tricyclic rings, and fullerenes. The synthetic pathways are also indicated. See ref. 83. Reproduced from the International Journal of Mass Spectrometry and Ion Processes, vol. 149/150, R.P.A. Bettens, Eric Herbst "The interstellar gas phase production of highly complex hydrocarbons construction of a model", pp 321-343 (1995) with kind permission from Elsevier Science-NL, Sara Burgerhartstraat 25,1055 KV, Amsterdam, The Netherlands.
Having initiated the chemistry within the atmospheric model, the elongation of the carbon-chain polyyne species occurs by successive addition of the C2H radical ... [Pg.300]

Manoalide (164), a marine natural product which inhibits the release of arachidonic acid from phospholipids by phospholipase A2 [397,398], showed topical anti-inflammatory activity in mouse ear models [399]. Activity in ISN and cRBL (< 1 M) have also been reported [400]. A series of analogues consisting of the furanone ring of manoalide bearing simple unsaturated 16-20 carbon chains showed similar activity in rabbit neutrophils and isolated guinea-pig neutrophil 5-LO [401] interestingly, however, topical anti-inflammatory activity was seen in phorbol ester ear oedema but not in AAE [399]. The importance of 5-LO inhibition to the anti-inflammatory activity of manoalide is unknown effects on phospholipase C and calcium channels have also been shown [402, 403]. [Pg.39]

This representation fits into the more general treatment of prochirality and prostereoisomerism (42, 50-52). Using the infinite chain model the + and — bonds must be considered enantiotopic (53) because they are related by a mirror plane perpendicular to the chain axis and passing through every tertiary carbon atom. [Pg.7]

Nowak et al. (63) presented a comparative study of the diffusivities of rigid models of methane, ethane, and propane in silicalite. (The details of the calculation are reported in the preceding section.) The calculated diffusion coefficients decreased as the length of the carbon chain increased, and the effect was found to be far more pronounced for ethane than propane. The calculated diffusivities, in units of 108 m2/s, were 0.62, 0.47, and 0.41 for methane, ethane, and propane, respectively. The ethane value is in satisfactory agreement with PFG-NMR measurements [0.38 (77), 0.3 (80), 0.4 (42) for silicalite. The value for propane, however, was calculated to be almost an order of magnitude larger than the NMR results of Briscoe et al. (80). [The agreement with the value of Caro et al. (71) is better, but still an overestimation.]... [Pg.34]

In 1985. similar experiments were conducted at Rice University. In a 1988 paper. Curl and Smalley (Rice University) outlined their experiments with carbon cluster beams, essentially using the clusler-generaung apparatus previously described by the Exxon researchers. Initially, this experimentation was motivated by an interest that had been shown by die astrophysicist, Krotu (University of Sussex), who had been modeling the formation of carbon molecules in circumstellar shells. As a consequence, the Rice University team concentrated its studies on the smaller (2- to 30-atom) carbon clusters. As pointed out in the Curl-Smalley paper, the objective was to determine if some or all of the species had the same form as the long linear carbon chains known to be abundant in interstellar space."... [Pg.287]

A simple model of molecules with conjugated double bonds assumes that n elections can move freely along the carbon chain. The length given in Problem 4 is appropriate to butadiene (1). It is necessary to invoke the exclusion principle (see Chapter 5), according to which no level may hold more than two electrons. In ground state of 1 therefore, the four it electrons must go two each into the n = 1 and n = 2 particlc-in-a-box levels. [Pg.35]

Fig. 6. Model of asphaltene structure (wavy lines represent the zigzag configuration of a saturated carbon chain or a loose net of naphthenic rings and straight lines represent the edge of flat sheets of condensed aromatic rings) (Yen et at., 1961). Fig. 6. Model of asphaltene structure (wavy lines represent the zigzag configuration of a saturated carbon chain or a loose net of naphthenic rings and straight lines represent the edge of flat sheets of condensed aromatic rings) (Yen et at., 1961).
With regard to the shape of the MO s themselves, consider a set of four parallel and equally spaced -orbitals of a carbon chain, as a model... [Pg.193]


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See also in sourсe #XX -- [ Pg.261 ]




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