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Solutions Manual for Dynamics of Structures Theory and Applications to Earthquake Engineering 6th Edition by Anil K. Chopra

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Solutions Manual for Dynamics of Structures Theory and Applications to Earthquake Engineering 6th Edition by Anil K. Chopra. PART I: SINGLE-DEGREE-OF-FREEDOM SYSTEMS Equations of Motion, Problem Statement, and Solution Methods Free Vibration Response to Harmonic and Periodic Excitations Response to Arbitrary, Step, and Pulse Excitations Numerical Evaluation of Dynamic Response Earthquake Response of Linear Systems Earthquake Response of Inelastic Systems Generalized Single-Degree-of-Freedom Systems PART II: MULTI-DEGREE-OF-FREEDOM SYSTEMS Equations of Motion, Problem Statement, and Solution Methods Free Vibration Damping in Structures Dynamic Analysis and Response of Linear Systems Earthquake Analysis of Linear Systems Analysis of Nonclassically Damped Linear Systems Reduction of Degrees of Freedom Numerical Evaluation of Dynamic Response Systems with Distributed Mass and Elasticity Introduction to the Finite Element Method PART III: EARTHQUAKE RESPONSE, DESIGN, AND EVALUATION OF MULTISTORY BUILDINGS Earthquake Response of Linearly Elastic Buildings Earthquake Analysis and Response of Inelastic Buildings Earthquake Dynamics of Base-Isolated Buildings Earthquake Dynamics of Building–Soil Interaction Structural Dynamics in Building Codes Structural Dynamics in Building Evaluation Guidelines APPENDICES FREQUENCY-DOMAIN METHOD OF RESPONSE ANALYSIS NOTATION ANSWERS TO SELECTED PROBLEMS

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Earthquake Engineering 6th Edition
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Institution
Earthquake Engineering 6th Edition
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Earthquake Engineering 6th Edition

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Uploaded on
October 24, 2024
Number of pages
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Written in
2024/2025
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INSTRUCTOR’S
SOLUTIONS MANUAL




R
DYNAMICS OF STRUCTURES




U
Theory and Applications to




SE
Earthquake Engineering
SIXTH EDITION
IS
O
N

Anil K. Chopra
N


University of California at Berkeley
O
C
ED
M

, CHAPTER 1

Problem 1.1

Starting from the basic definition of stiffness, determine
the effective stiffness of the combined spring and write the
equation of motion for the spring–mass systems shown in
Fig. P1.1.




R
Figure P1.1




U
Solution:
If ke is the effective stiffness,




SE
fS  keu

u
k1


k2
fS
k1 u
k2 u
fS
IS
O
N

Equilibrium of forces: fS  ( k1  k2 ) u
N

Effective stiffness: ke  fS u  k1  k2
Equation of motion: mu  keu  p ( t )
O
C
ED
M




1
Copyright © 2023 Pearson Education, Inc.

,Problem 1.2

Starting from the basic definition of stiffness, determine
the effective stiffness of the combined spring and write the
equation of motion for the spring–mass systems shown in
Fig. P1.2.




Figure P1.2

Solution:




R
If ke is the effective stiffness,




U
fS  keu (a)




SE
u
k1 k2
fS


If the elongations of the two springs are u1 and u2 ,
u  u1  u2 (b) IS
O
Because the force in each spring is fS ,
fS  k1u1 fS  k2u2 (c)
N

Solving for u1 and u2 and substituting in Eq. (b) gives
fS f f 1 1 1
N

 S  S    
ke k1 k2 ke k1 k2
k1 k2
O



ke 
k1  k2
C




Equation of motion: mu  keu  p ( t ) .
ED
M




2
Copyright © 2023 Pearson Education, Inc.

, Problem 1.3

Starting from the basic definition of stiffness, determine
the effective stiffness of the combined spring and write the
equation of motion for the spring–mass systems shown in
Fig. P1.3.




Figure P1.3

Solution:




R
k1 k3
m




U
Figure P1.3a
k2





SE
k 1+ k 2 k3
m
Figure P1.3b




ke
u IS
O
m
Figure P1.3c
N
This problem can be solved either by starting from the
definition of stiffness or by using the results of Problems
N

P1.1 and P1.2. We adopt the latter approach to illustrate
the procedure of reducing a system with several springs to
a single equivalent spring.
O



First, using Problem 1.1, the parallel arrangement of
k1 and k2 is replaced by a single spring, as shown in Fig.
C




1.3b. Second, using the result of Problem 1.2, the series
arrangement of springs in Fig. 1.3b is replaced by a single
ED




spring, as shown in Fig. 1.3c:
1 1 1
 
ke k1  k2 k3
Therefore the effective stiffness is
M




( k1  k2 ) k3
ke 
k1  k2  k3
The equation of motion is mu  keu  p ( t ) .




3
Copyright © 2023 Pearson Education, Inc.

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