On the Internal Resonance of a Spinning Disk Under Space-Fixed Pulsating Edge LoadsSource: Journal of Applied Mechanics:;2001:;volume( 068 ):;issue: 006::page 854Author:Jen-San Chen
DOI: 10.1115/1.1408616Publisher: The American Society of Mechanical Engineers (ASME)
Abstract: Internal 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.
keyword(s): Resonance , Stability , Stress , Bifurcation , Rotating Disks , Steady state AND Damping ,
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contributor author | Jen-San Chen | |
date accessioned | 2017-05-09T00:03:56Z | |
date available | 2017-05-09T00:03:56Z | |
date copyright | November, 2001 | |
date issued | 2001 | |
identifier issn | 0021-8936 | |
identifier other | JAMCAV-926184#854_1.pdf | |
identifier uri | http://yetl.yabesh.ir/yetl/handle/yetl/124635 | |
description abstract | Internal 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. | |
publisher | The American Society of Mechanical Engineers (ASME) | |
title | On the Internal Resonance of a Spinning Disk Under Space-Fixed Pulsating Edge Loads | |
type | Journal Paper | |
journal volume | 68 | |
journal issue | 6 | |
journal title | Journal of Applied Mechanics | |
identifier doi | 10.1115/1.1408616 | |
journal fristpage | 854 | |
journal lastpage | 859 | |
identifier eissn | 1528-9036 | |
keywords | Resonance | |
keywords | Stability | |
keywords | Stress | |
keywords | Bifurcation | |
keywords | Rotating Disks | |
keywords | Steady state AND Damping | |
tree | Journal of Applied Mechanics:;2001:;volume( 068 ):;issue: 006 | |
contenttype | Fulltext |