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Effects of Time-Varying Mesh Stiffne...

Mitra, Eeshan.

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Effects of Time-Varying Mesh Stiffness, and its Modifications, on Planetary Gear Dynamics.

Record Type:	Electronic resources : Monograph/item
Title/Author:	Effects of Time-Varying Mesh Stiffness, and its Modifications, on Planetary Gear Dynamics./
Author:	Mitra, Eeshan.
Published:	Ann Arbor : ProQuest Dissertations & Theses, : 2017,
Description:	122 p.
Notes:	Source: Masters Abstracts International, Volume: 56-06.
Contained By:	Masters Abstracts International56-06(E).
Subject:	Mechanical engineering. -
Online resource:	http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=10257335
ISBN:	9780355156409

Effects of Time-Varying Mesh Stiffness, and its Modifications, on Planetary Gear Dynamics.
Mitra, Eeshan.

Effects of Time-Varying Mesh Stiffness, and its Modifications, on Planetary Gear Dynamics. - Ann Arbor : ProQuest Dissertations & Theses, 2017 - 122 p.

Source: Masters Abstracts International, Volume: 56-06.

Thesis (M.S.M.E.)--Purdue University, 2017.

Time-varying mesh stiffness in gears has been found to be the primary cause for vibration in gears. This parametric excitation opens up bands of unstable regions of frequency, rather than just isolated resonances. Despite its many advantages, planetary gears, by virtue of having more components, and therefore more degrees of freedom, add to the complexity in terms of vibrational response.

ISBN: 9780355156409Subjects--Topical Terms:

649730
Mechanical engineering.

Effects of Time-Varying Mesh Stiffness, and its Modifications, on Planetary Gear Dynamics.
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020 $a 9780355156409
035 $a (MiAaPQ)AAI10257335
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100 1 $a Mitra, Eeshan. $3 3348321
245 1 0 $a Effects of Time-Varying Mesh Stiffness, and its Modifications, on Planetary Gear Dynamics.
260 1 $a Ann Arbor : $b ProQuest Dissertations & Theses, $c 2017
300 $a 122 p.
500 $a Source: Masters Abstracts International, Volume: 56-06.
500 $a Adviser: Charles M. Krousgrill.
502 $a Thesis (M.S.M.E.)--Purdue University, 2017.
520 $a Time-varying mesh stiffness in gears has been found to be the primary cause for vibration in gears. This parametric excitation opens up bands of unstable regions of frequency, rather than just isolated resonances. Despite its many advantages, planetary gears, by virtue of having more components, and therefore more degrees of freedom, add to the complexity in terms of vibrational response.
520 $a This research is aimed at carrying out a numerical investigation on the effects of mesh stiffness. To establish this objective, a discretized model of a planetary gear assembly is set up using a lumped parameter approach. Subsequently, its natural frequencies are determined, and categorized based on the structured properties of modal response. A numerical algorithm using the Floquet theory is developed to trace the stability boundaries of a reduced order model. The boundaries for a Rayleigh-damped system are also traced, and compared with the instabilities of the undamped system.
520 $a Qualitative dependence of the external gear mesh stiffness on tooth profile modification is discussed, and stability boundaries are re-computed for different kinds of modifications. Forced response plots for 'relieved' profiles show that while the peak amplitudes of super-harmonic resonances decrease dramatically, amplitudes for primary resonances increase, owing to an increased strength of the fundamental frequency component in a modified stiffness profile.
590 $a School code: 0183.
650 4 $a Mechanical engineering. $3 649730
650 4 $a Mechanics. $3 525881
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690 $a 0346
710 2 $a Purdue University. $b Mechanical Engineering. $3 1019124
773 0 $t Masters Abstracts International $g 56-06(E).
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791 $a M.S.M.E.
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793 $a English
856 4 0 $u http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=10257335