2001
DOI: 10.1016/s0169-5983(00)00018-6
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Flow of a power-law fluid over a rotating disk revisited

Abstract: The von Kà armà an swirling ow due to a rotating disk admits similarity solutions even in the case of a power-law uid. The non-linearities introduced by the rheological model may deteriorate the numerical solutions of the resulting set of ordinary di erential equations with increasing departure from Newtonian behaviour. The reliability of earlier numerical results are nevertheless approved, except for highly shear-thinning uids (the power-law index n ¡ 0:5) for which a severe ambiguity in the solutions is reve… Show more

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Cited by 99 publications
(42 citation statements)
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“…A comparison of the present results corresponding to the values of ffalse(0false) and [θfalse(0false)] with the available published results of Ming et al, Anderson et al, Xun et al, and Hayat et al is made numerically in Table . The results are found in good agreement.…”
Section: Resultsmentioning
confidence: 60%
See 1 more Smart Citation
“…A comparison of the present results corresponding to the values of ffalse(0false) and [θfalse(0false)] with the available published results of Ming et al, Anderson et al, Xun et al, and Hayat et al is made numerically in Table . The results are found in good agreement.…”
Section: Resultsmentioning
confidence: 60%
“…Later, Cochran pointed out errors in von‐Karman's momentum integral solutions and gave more accurate results. Later on, researchers investigated various physical problems …”
Section: Introductionmentioning
confidence: 99%
“…Data most closely aligned with the experiment with respect to statement are cited in [9], where the slow circulation flow of a viscous liquid over a disk rotating in the horizontal plane was investigated; results of visual observations of the eddy structures are not presented here, however, and only an analytical description of the circulation flow observed is given.…”
mentioning
confidence: 88%
“…Erdogan [10] studied the flow which was induced and implemented in a non-torsional fluctuation and a rotation of fluid infinitely by non-coaxial disk revolution. Anderson et al [11] returned power-law fluid flow to a completed spinning disk. Takhar et al [12] worked on unstable flow of MHD and the transfer of heat over a moving disk and the fluid was ambient.…”
Section: Introductionmentioning
confidence: 99%