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School of Engineering and Science - Jacobs University

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°C). The stirring speed was 300 rpm. The ethyl pyruvate was added to 70 ml <strong>of</strong> acetic<br />

acid, then the mixture was sonicated for 10 min, Ar was then flushed through the<br />

solution for 10 min to remove dissolved air. The required amount <strong>of</strong> catalyst was<br />

added, the mixture was sonicated for 5 min, transferred into the reactor, flushed with Ar<br />

for 10 min <strong>and</strong> finally after the pressure <strong>of</strong> hydrogen had been stabilized for 10-15 sec<br />

the initial time (t=0) was set <strong>and</strong> the reaction kinetics were monitored. Around one ml<br />

aliquots <strong>of</strong> the reaction mixture were taken at certain time intervals, filtrated with a G4<br />

filter <strong>and</strong> 1 μl was injected into the gas chromatograph (GC).<br />

FTIR spectra <strong>of</strong> D type <strong>of</strong> catalyst were measured with a “Thermo Nicolet Avatar”<br />

spectrometer in transmission mode, resolution 4 cm -1 , number <strong>of</strong> scans 500. IR pellets<br />

were prepared by mixing 100 mg KBr <strong>and</strong> 1.5 mg sample then pressing into a pellet<br />

under a pressure <strong>of</strong> 10 tons. For IR investigation <strong>of</strong> the B type <strong>of</strong> catalyst a “Thermo<br />

Nicolet 4700 FT-IR” spectrometer with liquid nitrogen cooled detector <strong>and</strong> DRIFT<br />

accessory was used with the following parameters: 3000 scans, 600-2000 cm -1 scan<br />

range, 4 cm -1 resolution. The DRIFT spectra were chosen for analysis because it is the<br />

more applicable technique for observing adsorbed species on finely divided metal<br />

powder [174].<br />

The carbon <strong>and</strong> nitrogen elemental analysis measurements were done on a Carlo Erba<br />

NA2500 C/N analyzer in the <strong>School</strong> <strong>of</strong> Geo<strong>Science</strong>s at Grant Institute in the <strong>University</strong><br />

<strong>of</strong> Edinburgh. Measurements were repeated several times with an error ~1%. The metal<br />

content was found from thermogravimetric Analysis (TGA) in 30-1200 °C temperature<br />

interval under nitrogen 100 ml/min with an SDTQ 600 instrument from TA<br />

Instruments.<br />

The cumulative enantiomeric excess (ee) was calculated according to the formula<br />

[ R]<br />

− [ S]<br />

ee = ⋅100%<br />

.<br />

[ S]<br />

+ [ R]<br />

The actual enantiomeric excess (ee*) was calculated by the previously established<br />

[169] formula<br />

ee y − ee y<br />

ee<br />

*<br />

i+<br />

1 i+<br />

1 i i<br />

i+<br />

1 / 2<br />

=<br />

,<br />

yi+<br />

1<br />

− yi<br />

where y i - mol <strong>of</strong> both ethyl lactates, ee –cumulative (observed) enantiomeric excess.<br />

Computational methods: Geometry optimization <strong>and</strong> calculation <strong>of</strong> IR spectra <strong>of</strong><br />

cinchonidine <strong>and</strong> quinoline were carried out using the Gaussian 03 program [175].<br />

Density functional theory (DFT) calculations were performed by using the B3LYP/6-<br />

31G method <strong>and</strong> basis set. The vibrations <strong>and</strong> orientations <strong>of</strong> dipole moment were<br />

visualized with GaussView <strong>and</strong> MOLDEN programs.<br />

4.3 Results <strong>and</strong> discussion<br />

4.3.1 General characterization<br />

Choice <strong>of</strong> conventional catalyst<br />

The Engelhard 4759 (5% Pt/Al 2 O 3 ) is known from 90 th to be one <strong>of</strong> the most studied<br />

catalyst for Orito reaction, however the Engelhard company does not produce one any<br />

more <strong>and</strong> it is not widely available. Due to this reason <strong>and</strong> the fact that under the same<br />

reaction conditions (Table 4-1) catalyst from Aldrich demonstrates higher<br />

enantioselectivity <strong>and</strong> reaction rate, we chose it to be the basic conventional catalyst for<br />

further comparisons.<br />

31

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