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In-vitro instrumental stimulation of oral breakdown of rice gels with different amylose contents
Yonggi Kim,suyong lee 한국산업식품공학회 2017 학술대회 및 심포지엄 Vol.2017 No.11
In-vitro food mastication has been simulated by incorporating size reduction process, followed by incubation with human saliva. However, they do not suffice to simulate the actual oral breakdown process where disruption by mastication (chewing) and wetting/lubrication by salivation take place simultaneously. In this study, in-vitro oral digestion of rice gels with different amylose contents was simulated by instrumentally performing mastication and salivation. The hardness of artificial saliva-treated rice gels was distinctly lowered with increasing chewing cycles and the rice gels with high amylose contents showed the highest degradation rate. When the rice gels were subjected to non-destructive tomographic analysis, the high amylose rice gels were clearly shown to be favorably fragmented into smaller pieces by chewing, followed by the low and intermediate amylose samples. These results could be explained by their cohesive texture rather than hardness. Therefore, this study may help understanding the changes in the physical properties of cereal-based foods during oral digestion.
Yonggi Kim,Sanhoon Ko,Wanil Cho,Suyong Lee 한국산업식품공학회 2017 학술대회 및 심포지엄 Vol.2017 No.04
Chewing and swallowing disorders such as dysphagia are common in the elderly people whose number is reported to continuously increase throughout the world. With this trend, the aging populations have recently become the global focus of substantial research interest in a variety of industrial fields and the food industry is also no exception. Further studies are also necessary to establish the guidelines or criteria for controlling the food texture for the elderly with different living and cultural backgrounds. An experimental attempt was made to bridge the gap between instrumental and sensory texture in a model solid food system, providing a reference texture range for the elderly diets. For doing so, uniaxial compression was applied to measure the instrumental hardness of corn starch gels that was correlated with their sensory properties perceived by the elderly aged 60 and older. A polynomial trend line was satisfactorily obtained with the formula (y=0.2188x2-5.7917x+38.14) describing the relationship between instrumental hardness and starch concentration. When the instrumental hardness (stress) was correlated with the sensory hardness, a linear correlation was observed with a coefficient of determination (R2=0.879). However, the use of logarithmic transformation exhibited the improved correlation of coefficients. A fairly linear correlation (R2>0.96) was thus observed between the instrumental and sensory hardness by a semi-logarithmic relationship known as Weber-Fechner’s law scale. In principal component analysis, two principal components that accounted for 86.71% of the total variance, separated the gel samples in terms of hardness/springiness and moistness, respectively. The categories of the starch gel samples were subdivided into five groups with different stress ranges. As a result, five categories of food texture could be successfully provided with corresponding stress range and consumer languages that can be used as a reference tool to establish the guideline or criteria for developing the elderly foods.
THEORETICAL LINE PROFILES OF THE MAGNETIC COMPACT STARS
KIM YONGGI The Korean Astronomical Society 1996 Journal of The Korean Astronomical Society Vol.29 No.suppl1
Using a phenomenological model for the accretion onto the magnetic white dwarf, we calclliated some optical line profiles from the magnetosphere of such systems. Line profiles of these systems seem to be produced in the magnetosphere of the compact star due to the reemission of X-ray produced near the stellar surface. Some results of our new calculation and the analysis of these results will be presented. Our results show that the model used here can reproduce the observed optical line profiles and open the possiblity to determine the parameters of individual systems.
X-RAY RADIATIONS OF INTERACTING BINARY 44i BOOTIS
KIM YONGGI,KIM MINSU The Korean Astronomical Society 1996 Journal of The Korean Astronomical Society Vol.29 No.suppl1
In order to study the X-ray radiations from solar type strong interacting binary stars, we have collected X-ray data of 44i Bootis (P=0.2678 days, SP=G2+G2) from the EXOSAT data archive. Preliminarly analysis of a part of these data has been already reported by Vilhu & Heise (1986). In this paper, however, we present a more complete light curve in LE region than the previous work, and some unpublished X-ray light curves and spectrums. Using these new materials a new attempt to find the physical explanation about. some observational characteristic figures in the X-ray light curves and spectrums has been made.