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Protein Aggregation in White Wines: Influence of the Temperature on Aggregation Kinetics and Mechanisms

机译:白葡萄酒中的蛋白质聚集:温度对聚集动力学和机理的影响

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High temperatures (typically 80 °C) are widely used to assess wine stability with regard to protein haze or to study mechanisms involved in their formation. Dynamic light scattering experiments were performed to follow aggregation kinetics and aggregate characteristics in white wines at different temperatures (30-70 °C). Aggregation was followed during heating and cooling to 25 °C. Results were coupled with the study of the time-temperature dependence of heat-induced protein aggregation. At low temperature (40 °C), aggregation developed during heating. Colloidal equilibria were such that attractive interactions between species led to the rapid formation of micrometer-sized aggregates. At higher temperatures (60 and 70 °C), enhanced protein precipitation was expected and observed. However, high temperatures prevented aggregation, which mainly developed during cooling. Depending on the wine, cooling induced the formation of sub-micronic metastable aggregates stabilized by electrostatic repulsions, or the rapid formation of micrometer-sized aggregates, prone to sedimentation.
机译:高温(通常为80°C)被广泛用于评估葡萄酒在蛋白质浊度方面的稳定性或研究其形成机理。进行动态光散射实验,以追踪白葡萄酒在不同温度(30-70°C)下的聚集动力学和聚集特征。在加热和冷却至25℃期间进行聚集。结果与热诱导蛋白质聚集的时间-温度依赖性研究相结合。在低温(40°C)下,加热过程中会发生聚集。胶体平衡使得物种之间的吸引相互作用导致微米级聚集体的快速形成。在较高的温度(60和70°C)下,预计并观察到蛋白质沉淀增加。但是,高温阻止了聚集,聚集主要在冷却过程中形成。根据葡萄酒的不同,冷却会导致亚微亚稳聚集体的形成,该聚集体会受到静电排斥作用的稳定,或者会迅速形成微米级的聚集体,易于沉淀。

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