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根据其成分的紫外和红外光谱推测的退化玉米淀粉的可能结构。

A possible structure of retrograded maize starch speculated by UV and IR spectra of it and its components.

机构信息

The Tianjin Key Laboratory of Food Biotechnology, School of Food Science and Biotechnology, Tianjin University of Commerce, Tianjin, PR China.

出版信息

Int J Biol Macromol. 2012 Jan 1;50(1):119-24. doi: 10.1016/j.ijbiomac.2011.10.009. Epub 2011 Oct 15.

Abstract

"Retrogradation" has been used to describe the changes that occur in starch after gelatinization, from an initially amorphous state to a more ordered or crystalline state, which has a significant impact on starch application in food, textiles and materials fields. But mechanism of starch retrogradation is still unclear until now and there is no breakthrough in this area. Here we are speculating a possible structure of retrograded maize starch by UV (binding with iodine) and IR spectra of it and its compositions. We speculate that nucleation of retrograded starch origins from combination of reducing end of amylopectin and non-reducing end of amylose, and retrogradation terminates at combining of non-reducing end of amylopectin and reducing end of amylose. The chain length of resistant digestion retrograded starch should be nearly same. The hydroxyl associated with sixth carbon atoms of glucan must form hydrogen bond with other hydroxyl of starch.

摘要

“回生”用来描述淀粉糊化后发生的变化,从最初的无定形状态到更有序或结晶状态,这对淀粉在食品、纺织和材料领域的应用有重大影响。但是,直到现在,淀粉回生的机制仍不清楚,在这方面也没有突破。在这里,我们通过对其及其成分的紫外(与碘结合)和红外光谱来推测回生玉米淀粉的可能结构。我们推测,支链淀粉的成核起源于支链淀粉的还原端和直链淀粉的非还原端的结合,而回生在支链淀粉的非还原端和直链淀粉的还原端结合时终止。抗性消化回生淀粉的链长应该几乎相同。与葡聚糖第六碳原子上的羟基必须与淀粉的其他羟基形成氢键。

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