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O>, evolution

As discussed previously, the surface states responsible for the reduction peak could be intrinsic surface states or states associated with a surface-attached intermediate in the series of reactions leading to O-evolution. The latter possibility was deemed to be more likely since no change in voltage across the Helmholtz layer (no change in capacitance) was observed when these states are in the oxidized form. [Pg.112]

Figure 4. Experimental CO2 (o) evolution and simulated peaks during TPO (10 °C min" ) in 0.939 % O2 of a spent cracking catalyst. Figure 4. Experimental CO2 (o) evolution and simulated peaks during TPO (10 °C min" ) in 0.939 % O2 of a spent cracking catalyst.
The only waste of this process, ethylene chlorination using chlorine generated eleotroohemically, is hydrogen. Under the proper experimental conditions chlorine doesn o evoluted and explosive mixture doesn t form. [Pg.666]

It seems that His residues are also involved in O evolution... [Pg.373]

The observed differences in O -evolution are assumed to be due to different response of the clones especially with increasing temperature and rradiance, which may reflect the adaptation of the clones within the species to the changes in light environment during growth (4). This fact may explain lack of correlation between photosynthesis and growth observed previously (2,3). [Pg.952]

The basic relationship for the experimental determination of first-order rate constants is the extent of reaction (E.R.)-time profile where E.R. is defined either as ([R]o — [R])/[R]o (decay of reactant concentration) or as [P]/[R]o (evolution of product concentration). With these definitions in mind, we see that the scale on both x and y axes in the two plots in Figure 1.1 are actually apparent E.R. if [A]o is unity. In spectrophotometric kinetic analysis concentrations are not measured and it is necessary to assume that absorbance... [Pg.4]

On the basis of his studies with photosynthetic bacteria van Niel (362-364) reached the conclusion that the mechanism for COi fixation was separate and distinct from the energy-yielding process. Support for this hypothesis comes from the work of Hill and Scaris-brick (161), who obtained O evolution without the reduction of COj. Evidence that light was not immediately essential for COi fixation was provided by Ruben, Hassid, and Kamen (304) when they observed the formation of carbohydrate from CXlz in the dark intervals immediately following illumination of barley leaves. [Pg.3]

Figures Decomposition of hydrogen peroxide by Fe(III)-oaPc. [Fe(IlI)-oaPcl = 5 X 10 mol L [Fl O ] = 10 mol L pH = 7.0, 25°C. values calculated from the O evolution , titration with KMnO,. Figures Decomposition of hydrogen peroxide by Fe(III)-oaPc. [Fe(IlI)-oaPcl = 5 X 10 mol L [Fl O ] = 10 mol L pH = 7.0, 25°C. values calculated from the O evolution , titration with KMnO,.
Cheshnovsky O, Taylor K J, Conceicao J and Smalley R E 1990 Ultraviolet photoeieotron spectra of mass-selected copper clusters evolution of the 3d band Phys. Rev. Lett. 64 1785... [Pg.2404]

Fig. 1. Comparison of two different dynamical simulations for the Butane molecule Verlet discretization with stepsize r = O.OOSfs. Initial spatial deviation 10 A. Left Evolutions of the total length (=distance between the first and the last carbon atom) of the molecule (in A). Right Spatial deviation (in A) of the two trajectories versus time. Fig. 1. Comparison of two different dynamical simulations for the Butane molecule Verlet discretization with stepsize r = O.OOSfs. Initial spatial deviation 10 A. Left Evolutions of the total length (=distance between the first and the last carbon atom) of the molecule (in A). Right Spatial deviation (in A) of the two trajectories versus time.
The limit equation governing limj -,o qc can be motivated by referring to the quantum adiabatic theorem which originates from work of Born and FOCK [4, 20] The classical position g influences the Hamiltonian very slowly compared to the time scale of oscillations of in fact, infinitely slowly in the limit e — 0. Thus, in analogy to the quantum adiabatic theorem, one would expect that the population of the energy levels remain invariant during the evolution ... [Pg.386]

Prepare a mixture of 30 ml, of aniline, 8 g. of o-chloro-benzoic acid, 8 g. of anhydrous potassium carbonate and 0 4 g. of copper oxide in a 500 ml. round-bottomed flask fitted with an air-condenser, and then boil the mixture under reflux for 1 5 hours the mixture tends to foam during the earlier part of the heating owing to the evolution of carbon dioxide, and hence the large flask is used. When the heating has been completed, fit the flask with a steam-distillation head, and stcam-distil the crude product until all the excess of aniline has been removed. The residual solution now contains the potassium. V-phenylanthrani-late add ca. 2 g. of animal charcoal to this solution, boil for about 5 minutes, and filter hot. Add dilute hydrochloric acid (1 1 by volume) to the filtrate until no further precipitation occurs, and then cool in ice-water with stirring. Filter otT the. V-phcnylanthranilic acid at the pump, wash with water, drain and dry. Yield, 9-9 5 g. I he acid may be recrystallised from aqueous ethanol, or methylated spirit, with addition of charcoal if necessary, and is obtained as colourless crystals, m.p. 185-186°. [Pg.217]

Nitrogen. To one portion of the filtrate, add z-3 ml. of 10, aqueous sodium hydroxide solution, then add about o-2 g. of ferrous sulphate and proceed as in the Lassaigiie nitrogen test (p, 322). Note, however, that the fiUal acidification with dilute siiphiiric acid must be made with care, owing to the vigorous evolution of carbon dioxide from the carbonate present. [Pg.327]

Action of nitrous acid. To a few ml. of 20% NaNO, solution add a few drops of cold dil. acetic acid. Pour the mixture into a cold aqueous solution of glycine, and note the brisk evolution of nitrogen. NH CH COOH -h HNO2 = HO CH2COOH + N + H O. Owing to the insolubility of cystine in acetic acid use a suspension in dU. acetic acid for this test. In each case care must be taken not to confuse the evolution of nitrogen with any possible thermal decomposition of the nitrous acid cf. footnote, p, 360). [Pg.381]

In a 1 or 1-5 htre round-bottomed flask prepare a solution of 53-5 g. of o-toluidine in 170 ml. of 48 per cent, hydrobromic acid, cool to 5° by immersion in a bath of ice and salt. Diazotise by the gradual addition of a solution of 36 -5 g. of sodium nitrite in 50 ml. of water stopper the flask after each addition and shake until all red fumes are absorbed. Keep the temperature between 5° and 10°. When the diazotisation is complete, add 2 g. of copper powder or copper bronze, attach a reflux condenser to the flask, and heat very cautiously on a water bath. Immediately evolution of gas occurs, cool the flask in crushed ice unless the... [Pg.606]

CAUTION. The preparation of o-nitrobenzoyl chloride, o-nitrophenacetyl chloride and all o nitroacid chlorides should not be attempted by the above methods a violent explosion may occur upon distilling the product or when the last traces of thionyl chloride are removed in vacuo at 100°. Perhaps the safest method is to treat the pure acid in benzene solution with 1 1 mols of thionyl chloride and to reflux until evolution of sulphur dioxide and hydrogen chloride has ceased the solution of the acid chloride in benzene may then bo employed for most reactions. [Pg.792]

The reactant corresponding to retrosynthetic path b in Scheme 2.2 can be obtained by Meerwein arylation of vinyl acetate with o-nitrophcnyldiazonium ions[9], Retrosynthetic path c involves oxidation of a 2-(o-nitrophenyl)ethanol. This transformation has also been realized for 2-(o-aminophenyl)ethanols. For the latter reaction the best catalyst is Ru(PPhj)2Cl2. The reaction proceeds with evolution of hydrogen and has been shown to be applicable to a variety of ring-substituted 2-(o-aminophenyl)ethanols[10]. [Pg.15]

When the partial pressures of the radicals become high, their homogeneous recombination reactions become fast, the heat evolution exceeds heat losses, and the temperature rise accelerates the consumption of any remaining fuel to produce more radicals. Around the maximum temperature, recombination reactions exhaust the radical supply and the heat evolution rate may not compensate for radiation losses. Thus the final approach to thermodynamic equiUbrium by recombination of OH, H, and O, at concentrations still many times the equiUbrium value, is often observed to occur over many milliseconds after the maximum temperature is attained, especially in the products of combustion at relatively low (<2000 K) temperatures. [Pg.516]


See other pages where O>, evolution is mentioned: [Pg.192]    [Pg.303]    [Pg.169]    [Pg.141]    [Pg.351]    [Pg.449]    [Pg.741]    [Pg.255]    [Pg.539]    [Pg.786]    [Pg.867]    [Pg.1791]    [Pg.165]    [Pg.368]    [Pg.192]    [Pg.303]    [Pg.169]    [Pg.141]    [Pg.351]    [Pg.449]    [Pg.741]    [Pg.255]    [Pg.539]    [Pg.786]    [Pg.867]    [Pg.1791]    [Pg.165]    [Pg.368]    [Pg.123]    [Pg.51]    [Pg.2398]    [Pg.318]    [Pg.383]    [Pg.495]    [Pg.182]    [Pg.607]    [Pg.739]    [Pg.798]    [Pg.988]    [Pg.117]    [Pg.366]    [Pg.401]    [Pg.422]    [Pg.552]    [Pg.66]    [Pg.200]   
See also in sourсe #XX -- [ Pg.35 ]




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Os isotope evolution

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