A New Pulley Stress Analysis Method Based on Modified Transfer Matrix

Xiangjun Qiu and Vinit Sethi, USA

Summary

A new pulley stress analysis method is presented. It shall be referred to as the Modified Transfer Matrix (MTM) method. This method is based on a reformulation of transfer matrices for the pulleys cylindindrical shell, end-disk plate with non-uniform thickness and shaft by using finite element concepts. It combines the strength of both classical stress analysis methods and finite element methods. It proves to be an efficient and effective approach in determining the stresses in a pulley. A pulley stress analysis software program named PSTRESS 3.0 has been developed based on this new method. At the end of the paper, a numerical example of the pulley stress analysis, using PSTRESS 3.0, is given. The result is satisfactorily compared with that obtained in a finite element model (ANSYS) solution with a very fine mesh.

Nomenclature

x Cartesian coordinate in horizontal direction
y Cartesian coordinate in vertical direction
z Cartesian coordinate in pulley axial direction
r r cylindrical coordinate in pulley radial direction
cylindrical coordinate in pulley circumferential direction
P shear force acting on shaft cross section
M bending moment acting on shaft cross section
q distributed load acting on shaft axis
Ws transverse displacement of shaft neutral axis
θs rotational angle of shaft cross section
EI shaft bending stiffness
a shaft cross section area
G shear modulus of shaft material
β shaft state variable vector
A matrix containing coefficients of governing ODEs for
shaft bending deformation
B vector representing the non-homogeneous term of the governing ODEs for shaft bending deformation
T transfer matrix for the governing ODEs for shaft
bending deformation
I identity matrix
KBM TMB beam element stiffness matrix
UBM TMB beam element displacement vector
FBMext TMB beam element external force vector
FBMint TMB beam element internal force vector
Qr transverse shear force acting on the disk cross section
perpendicular to radial direction
Q transverse shear force acting on the disk cross section
perpendicular to circumferential direction
Mr bending moment acting on the disk cross section
perpendicular to disk radial direction
M bending moment acting on the disk cross section
perpendicular to disk circumferential direction
Mr twisting moment acting on the disk cross sections perpendicular
to disk radial direction and disk circumferential direction
g external transverse force acting on the neutral surface of the disk
u pulley disk and shell displacements in pulley axial direction
v pulley disk and shell displacements in pulley circumferential direction
w pulley disk and shell displacements in pulley radial direction
E YOUNG'S modulus of disk or cylindrical shell of pulley
POISSON'S ratio of disk or cylindrical shell of pulley
t thickness of disk or cylindrical shell of pulley
c coefficient to describe the geometry of disk variable thickness
p exponential number to describe the geometry of disk variable
thickness
D cross section bending stiffness of disk or cylindrical shell
m FOURIER component number
um FOURIER component of u
vm FOURIER component of v
wm FOURIER component of w
gm FOURIER component of g
Qrm FOURIER component of Qr
Qm FOURIER component of Q
Mrm FOURIER component of Mr
Mm FOURIER component of M
Mrm FOURIER component of Mr
θm rotational angle of disk or cylindrical shell of pulley
γm disk bending state variable vector of FOURIER component m
mrm disk circumferential harmonic resultant bending moment
Vrm disk circumferential harmonic resultant transverse shear force
Am matrix containing coefficients of governing ODEs for disk bending deformation of FOURIER component m
Bm vector representing the non-homogeneous term of the governing ODEs for disk bending deformation of FOURIER component m
UBDm TMB disk bending element displacement vector
KBDextm TMB disk bending element stiffness matrix
FBDextm TMB disk bending element external force vector
FBDintm TMB disk bending element internal force vector
Nr normal force acting on the disk cross section perpendicular to radial direction
N normal force acting on the disk cross section perpendicular to circumferential direction
Nr in-plane shear force acting on the disk cross sections perpendicular to disk radial direction and disk circumferential direction
Nrm FOURIER component of Nr
Nm FOURIER component of N
Nrm FOURIER component of Nr
ηm disk plane-stress state variable vector of FOURIER component m
Cm matrix containing coefficients of governing ODEs for disk In-plane deformation of FOURIER component m
UPNm TMB disk plane-stress element displacement vector
KPNm TMB disk plane-stress element stiffness matrix
FPNextm TMB disk plane-stress element external force vector
FPNintm TMB disk plane-stress element internal force vector 
UDKm TMB disk element displacement vector
KDKm TMB disk element stiffness matrix
FDKextm TMB disk element external force vector 
FDKintm TMB disk element internal force vector
R cylindrical shell radius
N1 normal force acting on the cylindrical shell cross section perpendicular to pulley axial direction
N2 normal force acting on the cylindrical shell cross section perpendicular to pulley circumferential direction
S membrane shear force acting on the cylindrical shell cross sections perpendicular to pulley axial direction and circumferential direction
Q1 transverse shear force acting on the cylindrical shell cross section perpendicular to pulley axial direction
Q2 transverse shear force acting on the cylindrical shell cross section perpendicular to pulley circumferential direction
M1 bending moment acting on the cylindrical shell cross section perpendicular to pulley axial direction
M2 bending moment acting on the cylindrical shell cross section perpendicular to pulley circumferential direction
M12 twisting moment acting on the cylindrical shell cross sections perpendicular to pulley axial direction and circumferential direction
fz external load acting on the neutral surface of shell in pulley axial direction
f external load acting on the neutral surface of shell in pulley circumferential direction
fr external load acting on the neutral surface of shell in pulley radial direction
fzm FOURIER component of fz
fm FOURIER component of f
frm FOURIER component of fr
N1m FOURIER component of N1
N2m FOURIER component of N2
M1m FOURIER component of S
M2m FOURIER component of M1
M12m FOURIER component of M2
V1m FOURIER component of M12
xm FOURIER component of element boundary equivalent transverse shear force
Jm cylindrical shell state variable vector of FOURIER component m
Im matrix containing coefficients of governing ODEs for cylindrical shell of FOURIER component m
M12 vector representing the non-homogeneous term of the governing ODEs for cylindrical shell of FOURIER component m
UCSm TMB cylindrical shell element displacement vector
Kcs m TMB cylindrical shell stiffness matrix
FCSextm TMB cylindrical shell element external force vector
FCSintm TMB cylindrical shell element internal force vector
Ψm state variable vector of FOURIER component m
S axial or radial coordinate
Hm matrix containing coefficients of governing ODEs of a pulley component
Lm vector representing the non-homogeneous term of the governing ODEs of a pulley component
Um generalized displacements of state variable vector of a pulley component
Fm generalized forces of state variable vector of a pulley component
Tm transfer matrix for the governing ODEs of a pulley component
Dm TMB element displacement vector of a pulley component
Km TMB element stiffness matrix of a pulley component
Fint m TMB element internal force vector of a pulley component
Fext m TMB element external force vector of a pulley component

1. Introduction

An engineered class belt conveyor pulley typically consists of a cylindrical shell, two end disks with variable thickness, a shaft, and two locking devices connecting end disks to the shaft as shown in Fig, 1. The pulley is usually subjected to severe bending due to very high belt tensions and locking assembly pressures, In the design of such a pulley, it is necessary to take into account the possibility of fatigue failure. Costly failures in large conveyor pulleys have led designers to seek detailed stress fatigue or endurance analysis. To date, two types of approaches for pulley stress analysis have been reported in the literature. One is the classical mechanics approach developed by LANGE [1] and SCHMOLTZI [2]. The other is the finite element method (FEM) employed by VODSTRICL [3], DANIEL [4] and SETHI et al. [5]. Both types of approaches have advantages and disadvantages.

Fig. 1: Cross-section of pulley assembly

The classical mechanics approach developed by LANGE and SCHMOLTZI is an approximate analytical approach, providing a closed-form solution for stresses in a pulley. The advantages of this method are that it is easy to program and takes a very short execution time to obtain a solution, The disadvantage is that the stress solution is not accurate at the locations near the connection region between the shell and end disks because of its poor approximation in treating the elastic coupling between these components. Specifically, the displacement of the end disk and shell are not coupled at their connection. This leads to significant errors in the stress and strain field about the connectors as will be shown.

The FEM has just the opposite advantages and disadvantages of the LANGE classical method. The major advantage of FEM is its ease of treating complex geometry and boundary conditions. The major disadvantage is its long execution time coupled with its need for an experienced user to generate a proper finite element mesh.

In this paper, a new method called the Modified Transfer Matrix (MTM) method is presented, This method circumvents the disadvantages of both the LANGE classical method and the conventional FEM. The MTM method proves to be a very effective and efficient approach in providing an accurate pulley assembly stress solution for any loading condition pulley.

Historically, the transfer matrix method was developed several decades ago [6] and was very popular in solving one dimensional static and dynamic problems before the advent of the FEM. Even today, this method is still useful in providing dosed form solutions to certain elasticity problems with simple boundary conditions [7]. Although there is a limitation in handling complicated boundary conditions, such as the boundary conditions for a pulley, the solution obtained by using the transfer matrix method is exact. In this paper, it is shown that the limitation of the transfer matrix method can be overcome if the transfer matrix is reformulated by using finite element concepts. The reformulated transfer matrix is essentially a special finite element, The new method using these special finite elements, called transfer matrix based (TMB) finite elements, is capable of solving a class of structural elasticity problems (including the elasticity problem of a pulley), whose governing differential equations can be reduced to a set of ordinary differential equations (ODEs). Regardless of how few of these TMB finite elements are used in a model, the solution obtained by this MTM method is generally very accurate due to the nature of the transfer matrix method.

Based on the MTM method, a computer program for pulley stress analysis named PSTRESS 3,0 has been developed, This program can provide stress solutions and perform fatigue analysis for most pulleys, with the characteristic geometry shown in Fig. 1, The pulley can be subjected to any type of non-uniform surface pressure, sheer loading, and prescribed locking pressure.

In section 2, the general ideas for deriving TMB elements for beam (i.e. shaft), end-disk plate with variable thickness, and cylindrical shell are presented. In section 3, the assembly of these elements to model a pulley in PSTRESS 3.0 is discussed. In section 4, an example of a belt conveyor pulley is numerically solved by PSTRESS 3.0 and the results are compared with those obtained using a finely meshed FEM (ANSYS) solution.

2. TMB Finite Elements for Beam, Disk Plate and Cylindrical Shell

Stresses and displacements in a pulley can be expressed in terms of FOURIER series with respect to the circumferential angle because of the pulley's axisymmetric geometry. Each FOURIER component of the solutions can be determined by solving a set of corresponding governing differential equations, which are uncoupled with the governing equations for other Fourier components. In Appendices A, B and C, it is shown that the governing equations for Fourier components for shaft, end-disk plate with non-uniform thickness, arid cylindrical shell of a pulley can be reduced to a set of ODEs of the first order respectively. The general solutions to these ODEs can be expressed in terms of the transfer matrix. By following the procedure described in Appendix D, the general solutions can be reorganized in a finite element form as below

KmDm = Fint m + Fext m (1)

where Km is the TMB element stiffness matrix, Dm is the element displacement vector, Fint m is the element internal force vector, Fext m is the element external force vector, and the subscript "m" denotes the FOURIER component number, The detailed procedures of developing TMB elements for shaft, end-disk and cylindrical shell are given in Appendices A, B and C, respectively.

Remarks;

As seen in the above discussion, the general solution to the governing differential equations for a pulley can be finally transformed into a finite-element form. This allows us to exploit many finite element analysis (FEA) capabilities to resolve pulley stresses using our MTM method, The most valuable FEA capability to be employed is the way of treating complicated boundary conditions. Therefore, using the MINI method, we can easily take into account the elastic coupling between the rim and the end-disk by following FEA assembly procedures, and implement the locking assembly pressure by using the FEA approach of treating mechanical Interference between two bodies. Both of these problems cannot be easily or precisely handled by most classical methods.

3. Assembly of TMB Elements for a Pulley Model in PSTRESS 3.0

In PSTRESS 3.0, the above derived TMB beam, disk plate and cylindrical shell element stiffness matrices are brought together to font a global stiffness matrix for a pulley in essentially the same way as that in conventional FEM, However, care must be taken at two locations, where special element assembly methods are required.

The first location is the connection region between the shell and the disk shown in Fig, 2a, where the finite dimension of the joint has to be taken into account in the stiffness matrix. The conventional way of treating the whole region as a single node would cause significant error in stress solutions near this region. One of the reasonable ways of providing correct elastic stiffness to connect the rim and the disk is treating the whole region as a special element by applying a substructure method. In PSTRESS 3.0, such a special element shown in Fig. 2b is developed.

Fig. 2: Connecting element between rim and end-disk

The second location is the connection point between the locking device and the shaft, One thing that must be kept in mind when assembling elements in this location is that the final solution consists of many FOURIER components, of which the shaft element only contributes to the FOURIER components of m = 0,1 and -1. In fact, in a pulley structure, the shaft deformation is governed only by these three FOURIER components due to its slender geometry. For the component of m = 0, the corresponding shaft deformation can be exactly modeled by a TMB cylindrical shell element presented in Appendix C. When a TMB beam element described in Appendix A is used, representing the shaft deformation of components of m = -1 and 1 (i.e., bending deformation), the following constraints on the deformation of the connecting point must be imposed:

Wm = -m Vm (2)
Um = rshaftθm (3)
Ws = Wm (4)
θs = θm (5)

Ws and θs are the shaft deflection and rotational angle respectively at the connecting point, where the subscript s denotes shaft deformation. The general definitions of Ws and θs are given in Appendix A.

Um, Vm, Wm and θm are disk plate displacements and rotational angle at the connecting point, where the subscript m denotes the FOURIER component number: m = -1 or 1. The general definitions of Um, Vm, Wm and θm, are given in Appendix B.  rshaft is the shaft radius at The connection point.

Such constraints are easy to implement in a finite element model by using FEA static condensation or penalty methods [10]. In PSTRESS 3.0, the static condensation method is employed. Finally, it must be pointed out that the TMB beam element stiffness matrix and corresponding nodal forces must be multiplied by a factor of 2 before they are assembled into global equations, due to the difference between actual forces and harmonic forces.

4. Numerical Example

Consider the belt conveyor pulley shown in Fig, 1, which is supported on two bearings and subjected to a locking pressure of 115.71 mPa (16,778 psi) at the interface between the locking device and disk hub. The shell circumferential surface pressure and shear loading between circumferential angles of 83 and 254% are developed from unequal belt tensions T1 = 1,017.8 kN (228,800 lb) and T2 = 632.98 kN (142.300 lb) shown in Fig. 3. The material properties and geometrical parameters of the pulley are given in Table 1, This pulley is analyzed by using PSTRESS 3.0, ANSYS 4.4 and CDIs derivation of LANGES classical method, respectively. Because of symmetry, only one quarter of pulley cross section is modeled.

Fig. 3: Load on pulley due to belt tension

In the PSTRESS model, the rim is modeled with 2 TMB elements, the disk is modeled with 6 TMB elements, the shaft is modeled with 3 TMB elements, and 71 FOURIER components are used. The reason for using more TMB elements for the disk is the necessity of taking account of the non-uniform thickness of the disk. In the ANSYS FEA model, 5,000 axisymmetric structural solid elements (with non axis-symmetric loading) are employed in the 2-0 cross-section. The use of the ANSYS FEM package to analyze a pulley is discussed in [5].

Material Property  
Young's modulus, MPSI 30
Poisson's ratio 0.3
Rim Geometry  
Rim length, inches 82
Rim outer diameter, inches 54
Rim thickness, inches 1.5
Belt width, inches 72
Disk Geometry  
Locking device width, inches 3.3
Hub outer diameter, inches 27.6
Hub inner diameter, inches 20.27
Hub width, inches 6.7
Fillet radius at hub, inches 3.67
Filet radius at rim, inches 1.20
Disk thickness between hub and rim, inches             
  Radius Thickness
 1.  15.610 1.740
 2. 16.268 1.487
 3. 19.321 1.409
 4. 22.400 1.217
 5. 22.742 1.199
 
Shaft Geometry  
Diameter, inches 16.535
Shaft length, inches 121
Distance between bearing centers, inches 104
Distance between disk centers, inches 74.13

Table 1: Material properties and geometrical parameters.

Figs. 4-7 show the PSTRESS numerical results compared with the ANSYS results. From these figures, it is seen that at location A of the rim and location D of the disk the agreement between the results Of the MTM method and the results of the conventional FEM is good. At location B of the rim and location C of the disk the agreement is still good, but some inaccuracy is observed, The reason may be that locations B and C are within the connection region between the rim and disk, where the 3-D stress state is more significant and cannot be fully taken into account in 2-D shell and plate theories. According to St. VENANTS principle and our experience, This 3-D stress state has only a very localized effect on pulley stress solution when the thicknesses of rim and disk are relatively small compared with the length and radius of the rim. It must be noted that the MTM method is much more efficient than the conventional FEM. PSTRESS 3.0 takes approximately 30 seconds to obtain a solution on an IBM PC 486, including the fatigue analysis. The FEM (ANSYS) solution takes 12-24 hours on an IBM RISC 6000 workstation.

Fig. 4: Stresses at Location A (inside of rim) PSTRESS 3.0 Analysis

Fig. 5: Stresses at Location B (inside of rim) PSTRESS 3.0 Analysis

Fig. 6: Stresses at Location C (inside of disk) PSTRESS 3.0 Analysis

Fig. 7: Stresses at Location D (inside of disk) PSTRESS 3.0 Analysis

Figs. 8-11 show the comparison of numerical results between LANGES solution and the FEM solution. Except at location A, LANGE's solution does not agree with the FEM solution. The poor agreement is due to the errors in treating the elastic coupling between the rim and the end-disk in LANGEs method.

Fig. 8: Stresses at Location A (Inside of rim) LANGE Analysis

Fig. 9: Stresses at Location B (Inside of rim) LANGE Analysis

Fig. 10: Stresses at Location C (Inside of disk) LANGE Analysis

Fig. 11: Stresses at Location D (Inside of disk) LANGE Analysis

Figs. 12 and 13 show both the PSTRESS and ANSYS results at two corners of the interface between the locking device and the shaft (locations E-E of Fig. 1).At these two locations, 3-D stress state is much more significant than at locations B and C. In order to produce more accurate stress solutions at the two corners, we introduce stress concentration factors in zero and first order FOURIER component solutions by using our empirical formulae built in PSTRESS 3.0. As seen in Figs. 12 and 13, these corrected solutions agree well with ANSYS solutions.

Fig. 12: Stresses at Location E (inside of pulley) PSTRESS 3.0 Analysis

Fig. 13: Stresses at Location E (outside of pulley) PSTRESS 3.0 Analysis

5. Conclusions

A new pulley stress analysis method which is based on reformulated transfer matrix has been developed. An accurate solution can be obtained by using this method. Three transfer-matrix-based elements for the shaft, disk plate and cylindrical shell have been developed. A numerical example has been given, which demonstrates the merits of this new method.

References

  1. LANGE, H.: Investigations on Stress in Belt Conveyor Pul leys; Doctoral thesis, Technical University Hannover, 1963.
  2. SCHMOLTZI, W.: The Design of Conveyor Belt Pulleys with Continuous Shafts; Doctoral thesis, Technical University, Hannover 1974.
  3. V0DSTRCIL, P.: Analysis of Belt Conveyor Pulley Using Finite Element Method; Proc. 4th i nt. Conf. in Australia on Finite Element Methods, University of Melbourne, Aug. 18-20, 1982.
  4. DANIEL, W.J.T.: Development of a Conveyor Pulley Stress Analysis Package; Proc. nt. Conf. on Bulk Material Storage, Handling and Transportation, Newcastle, Aug. 22-24, 1983.
  5. SETHI, V. and NORDELL, L.K.: Modern Pulley Design Techniques and Failure Analysis Methods; Proceedings of SME Annual Meeting & Exhibit, Peno Nevada, USA, Feb. 15-18,1993.
  6. PESTEL, S.C. and LECKIE, F.A.: Matrix Methods in Elastomechanics; New York McGraw-Hill Book Co., 1963.
  7. YEH KAIYUAN: General Solution on Certain Problems of Elasticity with Non-Homogeneity and Variable Thickness, The Advances of Applied Mathematics and Mechanics, Vol. 1; China Academic Publishers, pp 240-273, 1987.
  8. BOYCE, W.E. and DIPRIMA, R.C.: Elementary Differential Equations; Fifth Edition, John Wiley & Sons Inc., New York, 1992.
  9. TIMOSHENKO, S. and WOINOWSKY-KRIEGER. S.: Theory of Plates and Shells; McGraw-Hill Book Co., Second Edition, 1959.
  10. COOK, R.D., MALKUS, D.S. and PLE5HA, M.E.: Concepts and Applications of Finite Element Analysis; Third Edition, John Wiley & Sons Inc., 1969.

Appendix A

TMB Finite Element for Beam

Fig. A1 shows forces that act on a differential beam. Loads P, M, and q are shown in their positive sense. z is the axial coordinate.

Fig. A1: Forces that act on a differential element of beam

The equilibrium equations are

dP/dz = -q                         (A1)
dM/dz = P                          (A2)

By using TIM0SHENKOs beam theory, we have

dWs/dz = -θs + P/kaG    (A3)
s/dz = M/EI                (A4)

where the subscript s denotes the shaft deformation, Ws is the shaft neutral axis displacement, -θs is the slope due to bending, dWs/dz is the slope of the center line of the beam, k is a shape factor equal to 0.75 for circular cross section, EI is the bending stiffness, a is the cross-section area, and G is the shear modulus.

Eqs. (A1)-(A4) can be written in a matrix form

dβ/dz = Aβ + B           (A5)

where

β = (Ws, θs, P, M)T      (A6)
B = (0, 0, -q, 0)T         (A7)

and

A =

[

 0   -1   1/kaG  0 ]     (A8)
 0   0  0  1/EI 
 0   0  0 0
 0  1 0

where β is called state variable vector. 

According to the ODE theory [8], the general solution to Eq. (A5) can be expressed as

β(z) = T(z)β(z0) + T(z) z

z0
T(s)-1B(s)ds     (A9)

where z0 ≤ z ≤ zL, z0 and zL are the coordinates corresponding to two ends of the beam, and T(z) is the transfer matrix satisfying

dT/dz = AT and T(z0) = l              (A10)

where l is the identity matrix. Following the general procedure described in [8]. we can obtain the following closed-form transfer matrix

T(z) = [ 1 z-z0 z-z0 + (z-z0) (z-z0) ]     (A11)
kaG 2EI 2EI
0 1 (z-z0) z-z0
2EI EI
0 0 1 0
0 0 z-z0 1

where z0 ≤ z ≤ zL. Following the procedure described in Appendix D, we can obtain the following finite element equation, which is equivalent to Eq. (A9)

KBMUBM = FBMint + FBMext                 (A12)

where

UBM = (Ws (ZL), θs(ZL), Ws(Z0), θs(Z0))T         (A13)

FBMext is the beam element external force vector, FBMint is the beam element internal force vector, and KBM is the beam element stiffness matrix, which can be expressed:

KBM = [   12EI     Symmetric   ]        (A14)
L(1+α)
   6EI    (4+α)EI    
L(1+α) L(1+α)    
 -12EI    -6EI     12EI    
L(1+α) L(1+α) L(1+α)  
   6EI    (2-α)EI   -6EI   (a+α)EI
L(1+α) L(1+α) L(1+α) L(1+α)

Where

α = 12EI/LkaG and L = ZL - Z0           (A15)

Remarks:

It is not surprising to note that the TMB finite element stiffness matrix for a beam derived as Eq. (A14) is identical to the beam stiffness matrix derived by using conventional finite element method because the polynomial-type trial function used in conventional FEM exactly represents the actual beam displacement. However, for other types of structures such as plate and shell, the TMB element stiffness matrices may not be the same as the conventional finite element stiffness matrices.

Appendix B

TMB Finite Element for Disk Plate with Variable Thickness

B.1 TMB Bending Element

Fig. B1 shows a differential element of plate subjected to bending loads. x, y and z are Cartesian coordinates with z coinciding with pulley axial direction, x horizontal direction, and y vertical direction. r and are disk cylindrical coordinates. Loads Qr, Q, Mr, M and Mr are shown in their positive sense.

Fig. B1: Bending forces that act on a different element of plate

The equilibrium equations are:

Qr = Mr + Mr-M - 1 Mr               (B1)
∂r r r
Q = Mr +2 Mr - 1 M               (B2)
∂r r r
∂Qr + Qr - 1 Q = g(r, )               (B3)
∂r r r

where g is the external transverse force acting on the neutral surface of the plate, and equations representing the force-deformation relationship are:

Mr = -D [ ∂u + ( 1 ∂u + 1 ∂u )]        (B4)
∂r r ∂r r
M = -D [ ∂u + 1 ∂u + 1 ∂u ]        (B5)
∂r r ∂r r

Mr = D(1-)

[ 1 ∂u - 1 u ]        (B6)
r ∂r∂ r

where U is the plate neutral surface transverse displacement (see Fig. B1), is the POISSON's ratio,

D = Et/12(1 - )                   (B7)

E is the YOUNG's modulus, t is the thickness of the plate, which is a function of r, Within the element, we assume

t = crp              (B8)

where a and p are constants. Also, we assume the following FOURIER series for the components of displacement and forces

u =
Σ
m=0
umcosm +
Σ
m=1
u-msinm           (B9)
g =
Σ
m=0
gmcosm +
Σ
m=1
g-msinm         (B10)
Qr =
Σ
m=0
Qrmcosm +
Σ
m=1
Qr,-msinm      (B11)
Q =
Σ
m=1
Qmsinm +
Σ
m=0
Q,-mcosm    (B12)
Mr =
Σ
m=0
Mrmcosm +
Σ
m=1
Mr,-msinm      (B13)
M =
Σ
m=0
Mmcosm +
Σ
m=1
M,-msinm     (B14)
Mr =
Σ
m=1
Mrsinm +
Σ
m=0
Mr,-mcosm  (B15)

where um, Pm, Qrm, Qm, Mrm, Mm, Mrm (m=O.1,2,...) are functions of r only. Substituting Eqs. (89)-(B15) into Eqs. (B1)-(B6), we have the following ordinary differential equations

Qrm = M'rm + 1 (Mrm - Mm) - m Mrm (B16)
r r
Qm = M'rm + 2 Mrm + m

Mm

(B17)
r r

Q'rm +

1 Qrm - m Qm = gm (B18)
r r
Mrm = -D [ u"m + ( 1 u'm - m um )] (B19)
r r
Mm = - D [ u"m + 1 u'm - m um

]

(B20)
r r

Mrm = D(1-)

[

- m u'm + m um

]

(B21)
r r

where m = 0, 1, 2, ..., and the prime represents derivative with respect to r. Introducing the following state variables

γm = (um, θm, rm, Mrm)T      (B22)

Where

θm = u'm (B23)
mrm = -2πr Mrm (B24)
Vrm = 2πr (Qm - m/r Mrm) (B25)

Eliminating five variables, Mrm, Mm, Mrm, Qrm and Qm among Eqs. (B16)-(B21) and (B23)-(B25), we can obtain the following matrix-form equation

m/dr = Am γm + Bm  (m = 0, 1, 2, ...)    (B26)

Where Am =

[ 0 1 0 0 ] (B27)
m _ 0   1  
r   r 2πDr
2πDm(2 - 2 + m - m) -2πDm(3 - 2 - ) _ 1 m
r r   r r
2πDm(-3 + 2 + ) 2πD(1 - + 2m - 2m) -1 (1 - )
r r r

Bm = (0, 0, 2πrgm, 0)T         (B28)

Therefore, following the procedure described in Appendix D, we can obtain the following finite element equation for a circular plate ring (r0 ≤ r ≤ rL) with variable thickness and subjected to harmonic bending load

KBD mUBDm = FBDint m + FBDext m               (B29)

Where

UBDm = (ULm, Lm, Uom, θ0m)T      (B30)

KBD m is the plate element bending stiffness matrix, FBDext m is the element external force vector, FBDint m is the element internal force vector, the subscript L and 0 denote locations at r = rL and r0, respectively, and m denotes the FOURIER component number. Due to the complexity in deriving the transfer matrix for Eq. (B26), it is much more difficult to obtain a closed-form expression for KBD m of Eq. (B29) than for KBM of Eq. (A12). Instead, we can very accurately calculate KBD m by using our computer program of PSTRESS 3.0 mentioned in Remark ii of Appendix D.

B.2 TBM Plane Stress Element

Fig. B2 shows a differential element of plate subjected to in-plane loading. Loads Nr, N, and Nr are shown in their positive sense.

Fig. B2: In-plane forces that act on a differential element of plate

The definitions of x, y, Z, r and are the same as in section B.1. The equilibrium equations are

∂Nr + Nr - N + 1 ∂Nr = 0    (B31)
∂r r r
∂Nr + 2 Nr + 1 ∂N = 0    (B32)
∂r r r

The equations for force-deformation relationship are

Nr =     Et     ( ∂w + 1 ∂v + w ) (B33)
(1 - ) ∂r r r
N =     Et     ( ∂w + 1 ∂v + w ) (B34)
(1 - ) ∂r r r
Nr =     Et     ( ∂v + 1 ∂w - v ) (B35)
2(1 + ) ∂r r ∂θ r

where the definitions of , E and t are the same as in section B.1, arid v and w are the displacements of the neutral surface in circumferential and radial directions, respectively.

We assume the following FOURIER series for the components of displacements and forces

v =
Σ
m=1
vmsinm +
Σ
m=0
v-mcosm    (B36)
w =
Σ
m=0
wmcosm +
Σ
m=1
w-msinm    (B37)
Nr =
Σ
m=0
Nrmcosm +
Σ
m=1
Nr,-msinm    (B38)
N =
Σ
m=0
Nmcosm +
Σ
m=1
N,-msinm    (B39)
Nr =
Σ
m=1
Nrmsinm +
Σ
m=0
Nrmcosm    (B40)

where vmwm, Nrm, Nm and Nrm(m = 0,1,2, ...) are functions of r only. Substituting Eqs. (B36)-(B40) into Eqs. (B31)-(B35), we have the following ordinary differential equations

N'rm + 1 (Nrm - Nrm)+ m Nrm = 0 (B41)
r r
N'rm + 2

Nrm -

m Nm = 0 (B42)
r r
Nrm =     Et     [ w'm + ( m vm + 1 wm )] (B43)
(1 - ) r r
Nm =     Et     [ w'm + m vm + 1 wm ] (B44)
(1 - ) r r
Nrm =     Et     [ v'm - m wm - 1 vm ] (B45)
2(1 + ) r r

where m = 0, 1, 2, 3,.... Introducing the following state variables

ηm = (wm, vm, 2πrNrm , 2πrNrm)T         (B46)

and eliminating Nm among Eqs. (B41)-(B45). we obtain

m/dr = Cm ηm (m = 0, 1, 2, ...)          (B47)

where

Cm = [ _ _ m 1- 0 ]    (B48)
  r   r 2πEtr
m 1 0 1 +
r r 2πEtr
2πEt 2πEtm _ 1 - _ m
r r   r   r
2πEtm 2πEtm m _ 2
r r r   r

Thus, following the similar procedure in deriving Eq. (B29) , we can finally derive the following TMB finite element equation for a circular ring (r0 ≤ r ≤ rL) with variable thickness, subjected to in-plane harmonic loading

KPN m UPNm = FPNint m + FPNext m         (B49)

where

UPNm = (WLm, VLm, W0m, V0m)T             (B50)

KPN m is the element plane-stress stiffness matrix, FPNext m is the element external force vector, FPNint m is the element internal force vector, and the subscript L and C denote locations at r = rL and r0 respectively, and m denotes the FOURIER component number.

Combining Eq. (B29) and Eq. (B49), we can form a TMB shell element for disk plate, which is subjected to both bending and in-plane loading

KDK m UDKm = FDkint m + FDKext m              (B51)

where KDK m is the disk element stiffness matrix, UDKm is the element displacement vector, FDKext m is the element extemal force vector, and FDkint m is the element internal force vector. They can be calculated by the following formulae

UDKm = (ULm, VLm, WLm, θLm, U0m, V0m, W0m, θ0m)T (B52)
KDK m = ST1KBD mS1 + ST2KPN mS2 (B53)
FDKint m = ST1FBDint m + ST2FPNint m (B54)
FDKext m = ST1 FBDext m + ST2 FPNext m (B55)
S1 = [ 1 0 0 0 0 0 0 0 ]   (B56)
0 0 0 1 0 0 0 0
0 0 0 0 1 0 0 0
0 0 0 0 0 0 0 1

Remarks:

  1. Any other state variables than those defined in Eq. (B22) and Eq. (B46) cannot be employed because they may lead to incorrect element stiffness matrices and force vectors due to the violation of MAXWELL'S reciprocal theorem.
  2. Stiffness matrices obtained from transfer matrices must be symmetric. Any mistakes in choosing state variables, in deriving equations, and/or in numerical programming may lead to asymmetric stiffness matrices.
  3. If the stress calculation is desired, we can follow the following steps
    1. calculate values of state variables at element nodes,
    2. use transfer matrix and Eq. (D3) to calculate values of state variables at any interior location of the element, where stress values are desired,
    3. calculate first derivatives of state variables at desired locations by using Eq. (B26) and Eq. (B47),
    4. calculate Mrm, Mm, Mrm, Nrm, Nm and Nrm by using Eqs. (B19)-(B21) and Eqs. (B43)-(B45), and
    5. calculate FOURIER components of stresses by using calculated forces in step d.

Appendix C

TMB Finite Element for Cylindrical Shell

Fig. C1 shows forces acting on a differential element of a cylindrical shell with constant thickness t and radius R, z and are cylindrical coordinates. Loads N1, N2, S, Q1, Q2, M1, M2 and M12 are shown in their positive sense.

Fig. C1: Forces that act on a differential element of cylindrical

The equilibrium equations, according to [9] are

    ∂N1 + ∂S + fz = 0     (C1)
    ∂z R∂
    ∂N2 + ∂S + f = 0     (C2)
    R∂ ∂z
_ N2 + ∂Q1 + ∂Q2 + fr = 0      (C3)
   R ∂z R∂
Q2 = ∂M12 + ∂M2                   (C4)
∂z R∂
Q1 = ∂M1 + ∂M12                   (C5)
∂z R∂

where fz, f and fr are external loads acting on the neutral surface of the shell in axial, circumferential and radial directions respectively, and the equations for force-displacement relationship, according to [9]. are

N1 =    Et      ( ∂u +  ∂v  + w ) (C6)
(1-) ∂z R∂ R
N2 =    Et    ( ∂u +  ∂v  + w ) (C7)
(1-) ∂z R∂ R
    S =    Et    (  ∂u  + ∂v ) (C8)
  (1-2) R∂ ∂z
    M1 = -D ( ∂w +   ∂u   ) (C9)
    ∂z R∂
    M2 = -D ( ∂w +   ∂u   ) (C10)
  ∂z R∂
        M12 = -(1 - )D ∂w   (C11)
        R∂z∂  

where u, v and w are shell neutral surface displacements in axial, circumferential and radial directions, respectively,

D = Et/12(1 - )

the definitions of E and are the same as in section B, and t is the constant shell thickness. We assume the following FOURIER components of displacements and forces

fz =
Σ
m=0
fzmcosm +
Σ
m=1
fz,-msinm  (C12)
f =
Σ
m=1
fmsinm +
Σ
m=0
f,-mcosm  (C13)
fr =
Σ
m=0
frmcosm +
Σ
m=1
fr,-msinm  (C14)
u =
Σ
m=0
umcosm +
Σ
m=1
u-msinm  (C15)
v =
Σ
m=1
vmsinm +
Σ
m=0
v-mcosm  (C16)
w =
Σ
m=0
wmcosm +
Σ
m=1
w-msinm  (C17)
N1 =
Σ
m=0
N1mcosm +
Σ
m=1
N1,-msinm  (C18)
N2 =
Σ
m=0
N2mcosm +
Σ
m=1
N2,-msinm  (C19)
S =
Σ
m=1
Smsinm +
Σ
m=0
S-mcosm  (C20)
M1 =
Σ
m=0
M1mcosm +
Σ
m=1
M1,-msinm  (C21)
M2 =
Σ
m=0
M2mcosm +
Σ
m=1
M2,-msinm  (C22)
M12 =
Σ
m=1
M12msinm +
Σ
m=0
M12,-mcosm  (C23)
Q1 =
Σ
m=0
Q1mcosm +
Σ
m=1
Q1,-msinm  (C24)
Q2 =
Σ
m=1
Q2msinm +
Σ
m=0
Q2,-mcosm  (C25)

where all FOURIER coefficients are functions of z only. Substituting Eqs. (C12)-(C25) into Eqs. (C1)-(C11), introducing the following state variables

ξm = (Um, Vm, Wm, θm, 2πRN1m, 2πRSm, 2πRV1m, 2πRM1m)T       (C26)

Where

θm = -W'm            (C27)

and

V1m = Q1m + m/R M12m       (C28)

and eliminating five variables, N2m, M2m, M12m, Q1m and Q2m we can finally obtain the following matrix-form equation after a long tedious procedure of mathematical derivation

m/dz = Jmξm + Im   (m = 0, 1, 2, ...)     (C29)

Where

Jm = [ 0 _ m _ 0 1 - 0 0 0 ] (C30)
  R   R 2πEtR
m 0 0 0 0 1 + 0 0
R πEtR
0 0 0 -1 0 0 0 0
0 0 _ m 0 0 0 0 6(1 - )
  R πEtR
0 0 0 0 0 _ m 0 0
   R
0 πEtm 2πEtm 0 m 0 0 0
R R R
0 2πEtm 2πEt ( 1 + tm4 ) 0 0 0 m
R R 12R R R
0 0 0   πEtR   0 0 1 0
3(1+)R

and

Im = (0, 0, 0, 0, - 2πRfzm, -2πRfm, 2πRfrm, 0)T       (C31)

Therefore, according to the conclusions of Appendix D, the transfer matrix for Eq. (C29) can be obtained by the computer program developed in PSTRESS 3.0, Based on the transfer matrix, the TMB finite element for cylindrical shell with z0 ≤ z ≤ zL can be derived by following the procedure described in Appendix D, and the result can be expressed by

KCS m UCSm = FCSint m + FCSext m           (C32)

where

UCSm = (ULm, VLm, WLm, θLm, U0m, V0m, W0m, θ0m)T       (C33)

KCS m is the cylindrical-shell stiffness matrix, FCSext m is the element external force vector, FCSint m is the element internal force vector, and the subscripts L and 0 denote locations at z - zL, and z = z0, respectively, and m denotes the FOURIER component number.

If stress calculation for cylindrical shell is desired, we can follow the similar procedure described in Remark vi of section B.

Appendix D

Procedure of Deriving TMB Finite Element

In Appendices A, B and C, it is shown that the governing equations for FOURIER components for shaft, end-disk plate with nonuniform thickness, and cylindrical shell of a pulley can be reduced to a set of ODEs of first order respectively, and these ODEs can be finally unified as the following form

m/ds = Hm(s)ψm + Lm   (m = 0, 1, 2, ...)     (D1)

where the subscript m denotes the ordinary number of FOURIER components, Hm is a 2n x2n matrix. Lm is a 2n x 1 vector containing external loads, ψm is the state variable vector defined as

ψm = (UTm, FTm)T          (D2)

Um is an n x 1 vector containing generalized displacements, Fm an n x 1 vector containing corresponding generalized internal forces, and s is an axial or radial coordinate of the pulley, which is assumed within the range of s0 ≤ s ≤ sL, where s0 and sL are corresponding to two ends of a pulley component section (i,e, element).

Because Eq. (D1) is linear, the general solution is obtainable. By using the theory of ODE [8], the general solution to Eq. (D1) can be written as  

ψm(S) = Tm(S) ψm(s0) + Tm(S) s

s0
Tm(X)-1Lm (x)dx     (D3)

where Tm(s) is a 2n x 2n matrix called transfer matrix satisfying

dTm/ds = HmTm and Tm(s0) = I       (D4)

where I is the identity matrix, For any set of linear ordinary differential equations, which can be expressed in the form of Eq. (D1), there exists a unique 2n x 2n transfer matrix Tm(s) satisfying Eq. (D4). If Eq. (D1) is a set of constant ODEs (i.e., Hm is independent of s) or it can be transformed into a set of constant ODEs, a closed-form transfer matrix Tm(s) is obtainable. The general procedure of deriving Tm(s) is discussed in many textbooks, such as the one by BOYCE and DIPRIMA [8]. In what follows in this section, it is shown that a special finite element (i.e., TMB element) can be developed from Eq. (D3).

Let us consider a section of pulley, which is located in s0 ≤ s ≤ sL, and let

Tm(SL)= [ TUU TUF ] (D5)
TFU TFF
ψm(SL)= [ UL ] (D6)
Fint L
ψm(S0)= [ Uo ]    (D7)
-Fint 0

Pm = Tm(sL

sL

s0

Tm(X)-1 B(x)dx     (D8)

Where

UL = Um(SL)          (D9)
Uo = Um(S0)         (D10)
Fint L = Fm(SL)    (D11)
Fint 0 = -Fm(S0)   (D12)

Then Eq. (D3) can be rewritten as

[ UL ] = [ TUU -TUF ][ Fint L ] + Pm     (D13)
Fint L TFU -TFF Fint 0

Reorganizing Eq. (D13), we have

[ I -TUU ][ UL ] = [ 0 -TUF ][ Fint L ] + Pm     (D14) 
0 -TFU U0 -I -TFF Fint 0

from which we can obtain

KmDm = Fint m + Fext m     (D15)

Where

Km = [ 0 -TUF ]-1[ I -TUU ]   (D16)
-I -TFF o -TFU
Dm = (UTL, UT0)T     (D17)
Fint m = [ Fint L ]        (D18)
Fint 0
Fext m = [ 0 -TUF ]-1 Pm      (D19)
-1 -TFF

It is seen that Eq. (D15) is formulated in a finite-element form, where Km is element stiffness matrix, Dm is the element displacement vector, Fint m is the element internal force vector, and Fext m is the element external force vector, The detailed procedures of developing TMB elements for shaft, end-disk and cylindrical shell are given in Appendices A, B and C, respectively.

Remarks:

  1. It is noted that in developing TMB finite elements the trial function for representing element displacement field is not required. This is the feature that distinguishes the MTM method from the conventional finite element method.
  2. In general, for any type of structures, whose governing differential equations can be reduced to the form of Eq. (D1), which can be further transformed into a set of constant ODEs, the corresponding transfer matrix Tm(s) of Eq. (D3) can be derived following some standard procedure described in [8]. In most cases, the procedure of deriving Tm(S) can be fulfilled by using a computer program, and Pm defined in Eq. (D8) can be evaluated analytically or numerically; and Therefore, a computer program can be made, where the input is the matrix Hm and the external loads, and the output is the TMB element stiffness matrix and element external force vector. In this program, there is no discretization error in computing TMB element stiffness matrix. As a FORTRAN subroutine, such a computer program has been developed in PSTRESS 3.0.