RESUMO
The relationship between acrylamide and its precursors, namely, free asparagine and reducing sugars, was studied in cakes made from potato flake, wholemeal wheat, and wholemeal rye, cooked at 180 degrees C, from 5 to 60 min. Between 5 and 20 min, major losses of asparagine, water, and total reducing sugars were accompanied by large increases in acrylamide, which maximized in all three products between 25 and 30 min, followed by a slow linear reduction. Acrylamide formation did not occur to a large degree until the moisture contents of the cakes fell below 5%. Linear relationships were observed for acrylamide formation with the residual levels of asparagine and reducing sugars for all three food materials.
Assuntos
Acrilamida/análise , Secale/química , Solanum tuberosum/química , Triticum/química , Aminoácidos/análise , Asparagina/análise , Carboidratos/análise , Temperatura Alta , Água/análiseRESUMO
Melanoidins are the final, brown, high molecular weight products of the Maillard reaction. The aim of the present study was to determine the average molar extinction coefficients of melanoidins formed in heated glucose-casein and fructose-casein systems. The value of the extinction coefficient can be used to translate spectrophotometrically measured browning (absorbance values) into melanoidin concentration. In the present study the melanoidins were quantified by measuring the concentration of sugar incorporated into the melanoidins, using (14)C-labeled sugar. The extinction coefficient of the melanoidins remained constant during the observation period as the absorbance at 420 nm increased to approximately 8 units, and it was calculated to be 477 (+/- 50) L mol(-1) cm(-1) in the glucose-casein reaction and 527 (+/- 35) L mol(-1) cm(-1) in the fructose-casein reaction. This difference is not significant. An increase of the number of sugar molecules per reactive amino group during the heating of glucose-casein and the fructose-casein mixtures was observed by the radiochemical method as well as by microanalysis of the high molecular weight fraction.