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Reactions rebounding

To prevent a rebound hypoglycemic reaction from the sudden withdrawal of TPN containing a concentrated dose of dextrose, the rate of administration is slowly reduced or the concentration of dextrose gradually decreased. If TPN must be abruptly withdrawn, a solution of 5% or 10% dextrose is begun to gradually reduce the amount of dextrose administered. [Pg.646]

Allylic rearrangements with 3,3,6,6-dj-cyclohexene occurred in 20% of the MMO hydroxylation products compared to 33% for cytochrome P-450. These two experiments suggest that, with M. trichospor-ium OB3b, a rebound reaction must occur with a greater rate constant than with cytochrome P-450, in accord with the radical clock substrate work. [Pg.287]

Another method for conducting cyclizations catalytic in Cp2TiCl is shown in Scheme 14. It relies on the thermodynamically favorable ring closure of THF from 5-titanoxy radicals [81,82]. This step is mechanistically related to the oxygen rebound steps of oxidation reactions. While the scope of this transformation remains to be established, the presence of substituted THF-derivatives in many natural products renders the method potentially attractive. [Pg.46]

Zolpidem, chemically unrelated to benzodiazepines or barbiturates, acts selectively at the y-aminobutyric acidA (GABAA)-receptor and has minimal anxiolytic and no muscle relaxant or anticonvulsant effects. It is comparable in effectiveness to benzodiazepine hypnotics, and it has little effect on sleep stages. Its duration is approximately 6 to 8 hours, and it is metabolized to inactive metabolites. Common side effects are drowsiness, amnesia, dizziness, headache, and GI complaints. Rebound effects when discontinued and tolerance with prolonged use are minimal, but theoretical concerns about abuse exist. It appears to have minimal effects on next-day psychomotor performance. The usual dose is 10 mg (5 mg in the elderly or those with liver impairment), which can be increased up to 20 mg nightly. Cases of psychotic reactions and sleep-eating have been reported. [Pg.830]

These results are inconsistent with a radical rebound mechanism because this mechanism is a two-step process that requires the involvement of intermediates. Instead the results suggest that the hydroxylation is a concerted process, much like a singlet carbene reaction, which does not involve intermediates. However, this conclusion is in conflict with the properties of singlet carbene reactions discussed above. Subsequent studies on a number of substituted methylcyclopropanes and other stained hydrocarbon systems established that these findings were not anomalous. [Pg.39]

The O-dealkylation of ethers, while not as frequently encountered as N-dealkylation in drug metabolism studies, is still a common metabolic pathway. Mechanistically it is less controversial than N-dealkylation in that it is generally believed to proceed by the HAT pathway, i.e., a-hydrogen atom abstraction followed by hydroxyl radical rebound, and not a SET pathway (Fig. 4.58). The product of the reaction is unstable, being a hemiacetal or hemiketal depending on the number of hydrogens on the a-carbon, which dissociates to generate an alcohol and an aldehyde or ketone. [Pg.80]

Boundar y conditions need to be assessed based on the type of connections to be used for the member supports. The engineer must keep in mind that support details must provide sufficient strength, ductility and stability to enable the member to develop full collapse mechanism. Support capability to resist reaction forces for both the loading and rebound phases of the response must be considered when assessing boundary conditions. [Pg.54]

The peak rebound reaction is -2.33 kips (-10.36 kN) at t - 0.05 sec. Use the dynamic reaction for the roof in-plane loads analysis. [Pg.80]

The peak rebound dynamic reaction (not shown above) is -743.06 kips (-3 305 kN)... [Pg.85]

Note that the peak rebound reaction occurs after a number of cycles, and after the blast load disappears. [Pg.103]

A and BC approach to centre of mass, A strips off B and then AB and C return roughly in the direction from which they came. These reactions are said to occur by a rebound mechanism and generally occur when the surface are repulsive. In such reactions the life-time of activated complex, i.e. (ABC) must be short and reaction is said to be direct or impulsive. If life-time is much, rotation may occur and the products may separate in random directions. For many such reactions, the life-time of complexes has been observed less then 5 x 10 13sec. J.C. Polanyi discussed the relationship of these reactions with shapes of PES with special attention to mass effects. [Pg.244]

Mechanistic studies, including density functional theory (DFT) calculations, reveal that M -peroxynitrite (M = Fe and Mn) species, generated in the reactions of [(TAML)Fem(02)] and [(TAML)MnIV(02)]2" with NO, are converted into MIV(0) and N02 species through 0-0 bond homolysis of the peroxynitrite ligand. Then, a rebound of Fe (O) with N02 affords... [Pg.126]

Triazolam (ti/2 of elimination -1.5-5.5 h) is especially likely to impair memory (anterograde amnesia) and to cause rebound anxiety or insomnia and daytime confusion. The severity of these and other adverse reactions (e.g., rage, violent hostility, hallucinations), and their increased frequency in the elderly, has led to curtailed or suspended use of triazolam in some countries (UK). [Pg.226]

The following stage is core collapse caused by electron capture or photodisintegration of iron. According to the traditional view, collapse leads to formation of a neutron star which cools by neutrino emission and decompression of matter when it reaches nuclear density (10 g cm ). The rebound that follows generates a shock wave which is capable of reigniting a good few nuclear reactions as it moves back out across the stellar envelope. [Pg.101]

Fig. 5.4. Schematic evolution of the internal structure of a star with 25 times the mass of the Sun. The figure shows the various combustion phases (shaded) and their main products. Between two combustion phases, the stellar core contracts and the central temperature rises. Combustion phases grow ever shorter. Before the explosion, the star has assumed a shell-like structure. The centre is occupied by iron and the outer layer by hydrogen, whilst intermediate elements are located between them. CoUapse followed by rebound from the core generates a shock wave that reignites nuclear reactions in the depths and propels the layers it traverses out into space. The collapsed core cools by neutrino emission to become a neutron star or even a black hole. Most of the gravitational energy liberated by implosion of the core (some 10 erg) is released in about 10 seconds in the form of neutrinos. (Courtesy of Marcel Amould, Universite Libre, Brussels.)... Fig. 5.4. Schematic evolution of the internal structure of a star with 25 times the mass of the Sun. The figure shows the various combustion phases (shaded) and their main products. Between two combustion phases, the stellar core contracts and the central temperature rises. Combustion phases grow ever shorter. Before the explosion, the star has assumed a shell-like structure. The centre is occupied by iron and the outer layer by hydrogen, whilst intermediate elements are located between them. CoUapse followed by rebound from the core generates a shock wave that reignites nuclear reactions in the depths and propels the layers it traverses out into space. The collapsed core cools by neutrino emission to become a neutron star or even a black hole. Most of the gravitational energy liberated by implosion of the core (some 10 erg) is released in about 10 seconds in the form of neutrinos. (Courtesy of Marcel Amould, Universite Libre, Brussels.)...
Type E (end-of-use) reactions occur with rebound withdrawal phenomena. [Pg.260]


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