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The ADG was significantly decreased (P<0.05) for pigs that received a diet containing 0.69 g MJ−1 SID lysine:NE ratio when compared with pigs fed a diet containing 0.76 or 0.83 g MJ−1 SID lysine:NE ratio.
The feed to gain ratio (F G) decreased (linearly, P<0.05; quadratically, P<0.05) as the NE density or SID lysine:NE ratio increased, but no interaction of NE density and SID lysine: NE ratio on the F G.
The ADG was affected both linearly (P<0.05) and quadratically (P<0.05) as the SID lysine:NE ratio increased.
The NE density or SID lysine:NE ratio and their interaction had no effect on the average daily feed intake (ADFI) and serum urea nitrogen (SUN) (P>0.05).
The NE density or SID lysine:NE ratio and their interaction had no effect on the average daily feed intake, SUN, and carcass characteristic for finishing barrows (P>0.05).
Two 3×3 factorial design trials with 1 080 of Yorkshire×Landrace×Duroc barrows were conducted to investigate the effects of dietary net energy (NE) density and standardized ileal digestible (SID) lysine: NE ratio on the performance of growing-finishing pigs and carcass characteristic of finishing pigs fed low crude protein (CP) supplemented with crystalline amino acids (CAA) diets.
Similar(50)
These Ne ratios give approximately two-fold excesses of pu and up changes, respectively, for a gene with initial MCU = 0.7.
Under reduced Ne, the ratio of fixation probabilities of pu and up mutations decreases less as a function of MCU than under stationarity.
To evaluate our argument, it is necessary to determine the precise Ne isotopic ratios and the He/Ne elemental ratio for the solar energetic particle component by space craft/satellite observations or by theoretical calculations in the future.
Therefore, we argue that the 3He excess in D10IB130 originated from a component having solar-like Ne isotopic ratios and a higher 3He/4He ratio than the SW value.
The Ne isotopic ratios for ice-AMMs by Osawa and Nagao (2002) and Osawa et al. (2003a) are also shown for comparison.
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