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contributor authorJen-San Chen
date accessioned2017-05-09T00:03:56Z
date available2017-05-09T00:03:56Z
date copyrightNovember, 2001
date issued2001
identifier issn0021-8936
identifier otherJAMCAV-926184#854_1.pdf
identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/124635
description abstractInternal resonance between a pair of forward and backward modes of a spinning disk under space-fixed pulsating edge loads is investigated by means of multiple scale method. It is found that internal resonance can occur only at certain rotation speeds at which the natural frequency of the forward mode is close to three times the natural frequency of the backward mode and the excitation frequency is close to twice the frequency of the backward mode. For a light damping case the trivial solution can lose stability via both pitchfork as well as Hopf bifurcations when frequency detuning of the edge load is varied. On the other hand, nontrivial solutions experience both saddle-node and Hopf bifurcations. When the damping is increased, the Hopf bifurcations along the trivial solution path disappear. Furthermore, there exists a certain value of damping beyond which no nontrivial solution is possible. Single-mode resonance is also briefly discussed for comparison.
publisherThe American Society of Mechanical Engineers (ASME)
titleOn the Internal Resonance of a Spinning Disk Under Space-Fixed Pulsating Edge Loads
typeJournal Paper
journal volume68
journal issue6
journal titleJournal of Applied Mechanics
identifier doi10.1115/1.1408616
journal fristpage854
journal lastpage859
identifier eissn1528-9036
keywordsResonance
keywordsStability
keywordsStress
keywordsBifurcation
keywordsRotating Disks
keywordsSteady state AND Damping
treeJournal of Applied Mechanics:;2001:;volume( 068 ):;issue: 006
contenttypeFulltext


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