scholarly journals Optimisation Design and Damping Effect Analysis of Large Mass Ratio Tuned Mass Dampers

2019 ◽  
Vol 2019 ◽  
pp. 1-16 ◽  
Author(s):  
Ying-jie Kang ◽  
Ling-yun Peng

Under harmonic load and random stationary white noise load, the existing fitting formulas are not suitable for calculating the optimal parameters of large mass ratio tuned mass dampers (TMDs). For this reason, the optimal parameters of large mass ratio TMDs are determined by numerical optimisation methods, and a revised fitting formula is proposed herein based on a curve fitting technique. Finally, the dynamic time history analysis method is used to study the control effect of large mass ratio TMDs. The results show that when the mass ratio is large, the error between the existing fitting formula and the actual optimal value is quite large, and the revised fitting formula is applicable to the parameter design of the traditional small mass ratio and large mass ratio (≤1) TMDs. When the ratio of local base soil predominant frequency to structure vibration frequency is greater than 4, the optimal parameters of a TMD under white noise excitation can be calculated according to the revised fitting formula, and the remaining conditions should be determined by numerical optimisation. In addition, a large mass ratio TMD reduces the dynamic response of the main structure effectively compared with a small mass ratio TMD and reduces the relative displacement between the TMD and main structure.

2007 ◽  
Vol 3 (S245) ◽  
pp. 63-66 ◽  
Author(s):  
T. J. Cox ◽  
J. Younger ◽  
L. Hernquist ◽  
P. F. Hopkins

AbstractThe hierarchical formation of structure suggests that dark halos, and the galaxies they host, are shaped by their merging history. While the idea that mergers between galaxies of equal mass, i.e., major merger, produce elliptical galaxies has received considerable attention, he galaxies that result from minor merger, i.e., mergers between galaxies with a large mass ratio, is much less understood. We have performed a large number of numerical simulations of minor mergers, including cooling, star formation, and black hole growth in order to study this process in more detail. This talk will present some preliminary results of this study, and in particular, the morphology and kinematics of minor merger remnants.


1994 ◽  
Vol 422 ◽  
pp. 823 ◽  
Author(s):  
D. R. Gies ◽  
A. W. Fullerton ◽  
C. T. Bolton ◽  
W. G., Jr. Bagnuolo ◽  
M. E. Hahula ◽  
...  

2020 ◽  
Vol 29 (17) ◽  
Author(s):  
Ying‐jie Kang ◽  
Ling‐yun Peng ◽  
Peng Pan ◽  
Hai‐shen Wang ◽  
Gen‐qi Xiao

2016 ◽  
Vol 2016 (0) ◽  
pp. J0910301
Author(s):  
Shotaro ISHIHARA ◽  
Keiichi HIROAKI ◽  
Masahiro WATANABE

2018 ◽  
Vol 155 (6) ◽  
pp. 232 ◽  
Author(s):  
Colin Littlefield ◽  
Peter Garnavich ◽  
Mark Kennedy ◽  
Paula Szkody ◽  
Zhibin Dai

2011 ◽  
Vol 41 (1) ◽  
pp. 41-60 ◽  
Author(s):  
Maurizio De Angelis ◽  
Salvatore Perno ◽  
Anna Reggio

2015 ◽  
Vol 122 (1) ◽  
pp. 27-52 ◽  
Author(s):  
Natasha Bosanac ◽  
Kathleen C. Howell ◽  
Ephraim Fischbach

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