1Institut für Nutztierwissenschaften,Universität Hohenheim,Emil-Wolff-Straße 10,70599 Stuttgart,Deutschland.
2Core Facility Hohenheim,Universität Hohenheim,Emil-Wolff-Straße 12,70599 Stuttgart,Deutschland.
Animal. 2018 Mar;12(3):472-480. doi: 10.1017/S1751731117001926. Epub 2017 Aug 3.
Ruminal in situ incubations are widely used to assess the nutritional value of feedstuffs for ruminants. In in situ methods, feed samples are ruminally incubated in indigestible bags over a predefined timespan and the disappearance of nutrients from the bags is recorded. To describe the degradation of specific nutrients, information on the concentration of feed samples and undegraded feed after in situ incubation ('bag residues') is needed. For cereal and pea grains, CP and starch (ST) analyses are of interest. The numerous analyses of residues following ruminal incubation contribute greatly to the substantial investments in labour and money, and faster methods would be beneficial. Therefore, calibrations were developed to estimate CP and ST concentrations in grains and bag residues following in situ incubations by using their near-infrared spectra recorded from 680 to 2500 nm. The samples comprised rye, triticale, barley, wheat, and maize grains (20 genotypes each), and 15 durum wheat and 13 pea grains. In addition, residues after ruminal incubation were included (at least from four samples per species for various incubation times). To establish CP and ST calibrations, 620 and 610 samples (grains and bag residues after incubation, respectively) were chemically analysed for their CP and ST concentration. Calibrations using wavelengths from 1250 to 2450 nm and the first derivative of the spectra produced the best results (R 2 Validation=0.99 for CP and ST; standard error of prediction=0.47 and 2.10% DM for CP and ST, respectively). Hence, CP and ST concentration in cereal grains and peas and their bag residues could be predicted with high precision by NIRS for use in in situ studies. No differences were found between the effective ruminal degradation calculated from NIRS estimations and those calculated from chemical analyses (P>0.70). Calibrations were also calculated to predict ruminal degradation kinetics of cereal grains from the spectra of ground grains. Estimation of the effective ruminal degradation of CP and ST from the near-infrared spectra of cereal grains showed promising results (R 2>0.90), but the database needs to be extended to obtain more stable calibrations for routine use.
瘤胃内原位孵育广泛用于评估反刍动物饲料的营养价值。在原位方法中,将饲料样品在不可消化的袋子中在预定义的时间段内进行瘤胃孵育,并记录袋子中营养物质的消失情况。为了描述特定营养素的降解,需要了解饲料样品和原位孵育后未降解饲料(“袋残渣”)的浓度信息。对于谷物和豌豆粒,CP 和 ST(淀粉)分析是感兴趣的。瘤胃孵育后对残渣进行大量的分析极大地增加了劳动力和资金的投入,更快的方法将是有益的。因此,通过使用从 680 到 2500nm 记录的近红外光谱,开发了校准来估计原位孵育后谷物和袋残渣中的 CP 和 ST 浓度。样品包括黑麦、小黑麦、大麦、小麦和玉米粒(每种 20 个基因型),以及 15 个硬质小麦和 13 个豌豆粒。此外,还包括瘤胃孵育后的残渣(每种物种至少有 4 个样品用于不同的孵育时间)。为了建立 CP 和 ST 校准,对 620 个和 610 个样品(孵育后的谷物和袋残渣)进行化学分析,以确定其 CP 和 ST 浓度。使用 1250 到 2450nm 之间的波长和光谱的一阶导数进行校准,得到了最佳结果(CP 和 ST 的验证 R 2=0.99;CP 和 ST 的预测标准误差分别为 0.47%和 2.10%DM)。因此,通过 NIRS 可以高精度预测谷物和豌豆粒及其袋残渣中的 CP 和 ST 浓度,可用于原位研究。从 NIRS 估算的有效瘤胃降解与化学分析计算的降解之间没有差异(P>0.70)。还计算了校准以从研磨谷物的光谱预测谷物的瘤胃降解动力学。从谷物的近红外光谱估算 CP 和 ST 的有效瘤胃降解显示出有希望的结果(R 2>0.90),但需要扩展数据库以获得更稳定的校准,以用于常规用途。