2008
DOI: 10.1007/s00360-008-0264-x
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Physical characteristics of digesta and their influence on flow and mixing in the mammalian intestine: a review

Abstract: The physical properties of digesta may influence mixing, efficiency of digestion, and absorption within the lumen of the intestine. We review how the physical properties of digesta change during transit through the various segments of the intestine, and how their influence on flow and mixing may be modulated by peristaltic activity. We examine how, in more fluid digesta, the solid and liquid phases interact to influence flow and mixing. Similarly, how in viscid digesta, shear strength, plasticity and elasticit… Show more

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Cited by 180 publications
(141 citation statements)
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“…FimH allows E. coli to colonize the mouth where shear stress due to salivary flow is estimated at 0.08 Pa (38), and the intestines where shear stress due to peristalsis is estimated at 1 Pa (39,40). Our data showing the superior binding of wild-type K12 over activated FocH in this flow range (Fig.…”
Section: Discussionsupporting
confidence: 50%
“…FimH allows E. coli to colonize the mouth where shear stress due to salivary flow is estimated at 0.08 Pa (38), and the intestines where shear stress due to peristalsis is estimated at 1 Pa (39,40). Our data showing the superior binding of wild-type K12 over activated FocH in this flow range (Fig.…”
Section: Discussionsupporting
confidence: 50%
“…Cellulose resulted in faster transit than CMC and HG (data not shown); thus, besides the retention time in the small intestine, the accessibility of dietary nutrients appeared to be a critical factor for bacterial growth. Increased digesta viscosity impairs intestinal contractions (21), thereby preventing mixing of digesta and bacteria and thus access of bacteria to new substrate. Low-viscosity CEL, in turn, likely did not impair intestinal contractions and hence digesta mixing.…”
Section: Discussionmentioning
confidence: 99%
“…The absence of both, a distinct gas dome and a distinct sludge layer, could 314 theoretically be explained by a higher viscosity of both the rumen contents and the rumen 315 fluid in the browsing ruminants, which leaves both gas bubbles and fine, high-density 316 particles suspended in the fluid rather than allowing them to rise or sink within the RR. Even though, as discussed above, ingesta from both species separated according to particle 339 size due to its buoyancy characteristics in vitro, the situation in the densely packed suspension 340 of the RR is different (Lentle and Janssen, 2008). Buoyancy and sedimentation will probably 341 occur at much slower rates in this medium.…”
Section: Rr Contents Characteristics 305mentioning
confidence: 99%
“…After thawing, the viscosity of the rumen fluid supernatant was measured at 37 °C using 16 179 ml in a Brookfield LVDVE230 viscosimeter (Serial Number E6536, Brookfield Engineering 180 Laboratories, Middleboro, MA, USA) with a UL/Y adapter and spindle (rotational system 181 with concentric cylinder as recommended by Lentle and Janssen, 2008). With this system, the 182 shear rate is calculated as 1.29 x revolutions s -1 ; the producer recommends not to measure a 183 water-like substance at more than 1.29 s -1 .…”
Section: Introductionmentioning
confidence: 99%