Catalysis on evaporated metal films. V Reactions between cyclic hydrocarbons and deuterium

Catalytic exchange reactions have been studied by means of a mass spectrometer between deuterium and cyclo Zopentane over palladium and cyclo Zohexane over rhodium, palladium, tungsten, platinum, nickel, oriented nickel and oriented rhodium. Activation energies, frequency factors and distributions of initial products were determined. The reactions involved multiple exchange by repeated second-point adsorption. Half the hydrogen atoms were readily exchanged, and a study of the temperature-dependence of the product distributions showed that it required an activation energy of 4 to 8 kcal/mole in excess of that for adcorption-desorption before the remaining half could be exchanged. Considerations of molecular geometry revealed that in order to exchange the second half of the hydrogen atoms the molecule had to ‘turn over’ on the surface, and for cyclo Zopentane the process for turning over must require second-point adsorption by the same carbon atom, but with cyclo hexane there is the alternative process of exchanging two adjacent equatorial hydrogen atoms. Theories are developed which account satisfactorily for the observed initial product distributions. The pressure-dependence of reaction rate was determined for cyclo hexane over palladium. Deuterium was strongly adsorbed and cyclo hexane weakly adsorbed. Exchange of cyclo hexane over oriented films of nickel and rhodium showed marked differences in distribution compared with unoriented films, suggesting different catalytic activity of different crystal planes. Only exchange was observed with benzene over nickel, but there was simultaneous exchange and deuteration over palladium. The initial product pattern over palladium showed that a redistribution reaction (in the sense of Wagner et al , (1952)) did not occur during deuteration and that benzene was adsorbed mainly as phenyl radicals during the exchange reaction. The reaction between cyclo propane and deuterium was examined over rhodium and simultaneous exchange and deuteration were observed. As determined by the temperature range for reaction the order of reactivity in exchange was cyclo propane > cyclo pentane > cyclo hexane, and the order of catalytic activity of the metals was similar to that observed previously for the exchange of other saturated hydrocarbons.

1967 ◽  
Vol 20 (2) ◽  
pp. 297 ◽  
Author(s):  
CG Macdonald ◽  
JS Shannon

Selective exchange of hydrogen atoms ortho to amino or hydroxyl groups, together with benzylic hydrogen atoms in aniline, phenol, and their C- alkylated derivatives, was achieved by allowing these compounds to react with deuterium oxide over nickel on kieselguhr at 99�. In addition to the benzylic hydrogen atoms, alkyl hydrogen atoms farther from the aromatic ring underwent slower exchange. Hydrogen atoms ortho to methoxyl did not exchange. Mechanisms of the catalytic exchange reactions are discussed in the light of the results of deuterium distribution measurements and poisoning experiments with electron donors.


The exchange reactions of propane and isobutane have been followed on evaporated films of tungsten, rhodium and nickel by means of a mass-spectrometer. The energies of activation and frequency factors were approximately the same as those for the exchange reaction of ethane on tungsten and rhodium. Nickel films were effective at a slightly lower temperature for the exchange of propane and iso butane than for ethane but showed the same phenomenon of decreasing energy of activation above 0° C as had been observed for the reaction of ethane. The orders of reaction with respect to gas pressures were determined for the exchange of propane on all three catalysts. It appeared from the study of the initial products that the ability of rhodium to bring about multiple exchange is a characteristic property of that metal for hydrocarbon exchange reactions, in contrast to tungsten where the exchange is mainly brought about by successive replacement of the hydrogen atoms. Nickel showed appreciable differences in the rate of exchange of primary, secondary and tertiary hydrogen atoms. The rates of exchange of the secondary hydrogens in propane and the tertiary hydrogen in tsobutane were ten times faster than the rates for the primary hydrogens in the respective compounds.


RSC Advances ◽  
2016 ◽  
Vol 6 (39) ◽  
pp. 32430-32433 ◽  
Author(s):  
Yuwen Yang ◽  
Yongyun Mao ◽  
Bin Wang ◽  
Xianwei Meng ◽  
Jiao Han ◽  
...  

A facile impregnation method has been successfully applied for synthesis of a cubical Co3O4 supported Au nanocomposites, which leads to the excellent catalytic activity for the reduction of 4-nitrophenol with a high turn over frequency of 9.83 min−1.


1997 ◽  
Vol 52 (20) ◽  
pp. 3511-3520 ◽  
Author(s):  
Tadaatsu Ido ◽  
Takanobu Yamamoto ◽  
Gong Jin ◽  
Shigeo Goto

2019 ◽  
Vol 489 (2) ◽  
pp. 2723-2731
Author(s):  
Jiro Shimoda ◽  
J Martin Laming

ABSTRACT A novel diagnostic of cosmic ray modified shocks by polarimetry of H α emissions is suggested. In a cosmic ray modified shock, the pressure of cosmic rays is sufficiently high compared to the upstream ram pressure to force the background plasma to decelerate (measured in the shock rest frame). Simultaneously, a fraction of the hydrogen atoms co-existing in the upstream plasma collide with the decelerated protons and undergo charge-exchange reactions. As a result, hydrogen atoms with the same bulk velocity of the decelerated protons are generated. We show that when the shock is observed from edge-on, the H α radiated by these upstream hydrogen atoms is linearly polarized with a sizable degree of a few per cent as a result of resonant scattering of Ly β. The polarization direction depends strongly on the velocity modification; the direction is parallel to the shock surface for the case of no modification, while the direction is parallel to the shock velocity for the case of a modified shock.


2001 ◽  
Vol 2 (3-4) ◽  
pp. 125-128 ◽  
Author(s):  
Piero Frediani ◽  
Donella Rovai ◽  
Maurizio Muniz-Miranda ◽  
Antonella Salvini ◽  
Maria Caporali

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