Starch Content in a Wheat Genotypes Collection – Comparative Study
DOI:
https://doi.org/10.58509/enqz9j53Keywords:
breeding programme, clustering, model, regression analysis, wheat quality indicesAbstract
Wheat is an important crop for food safety and security. Starch is the main component by weight in the structure of wheat grains, with high importance for the processing process and the quality of the finished products. The present study evaluated the starch content in wheat grains in a collection of 25 genotypes. The field experiment was organized within ARDS Lovrin, in the agricultural year 2023 – 2024. The wheat genotypes were noted L5026 to L5050. The wheat crop was located on a chernozem type soil, with medium fertility, in a non-irrigated system. The previous crop was field peas, and uniform crop technology was applied for wheat. The starch content (STA, %) was determined in the Wheat Breeding Laboratory, ARDS Lovrin. Values between STA = 61.80±0.83% (L5045) and STA = 82.50±0.83% (L5042) were recorded, with normal distribution of the data series. In the case of the L5045 genotype, the outlier value was confirmed, at the p<0.05 level. Mann-Kendall trend test showed a decreasing trend in the data series, and regression analysis described the trend of the values in statistical safety conditions. In relation to the average value at the experiment level ( = 77.62%), 14 genotypes were recorded that presented differences in statistical safety conditions. Nine genotypes were recorded with positive differences, and five genotypes were recorded with negative differences. Genotype L5042 presented an increase in starch content DSTA = 4.876%, under p<0.001 conditions. Six genotypes (L5026, L5028, L5030, L5031, L5036, L5050) presented values above the average, with differences at the p<0.01 level, and two genotypes (L5027, L5037) presented differences at the p<0.05 level. Cluster analysis grouped the genotypes based on similarity, in relation to the starch content of the grains, under conditions of statistical safety (Coph.corr. = 0.960).
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