acharya finalreport

46
Creep Analysis of a Thick Walled Spherical Pressure Vessel Considering Large Strain by Tushar Kanti Acharya A Project Submitted to the Graduate Faculty of Rensselaer Polytechnic Institute in Partial Fulfillment of the Requirements for the degree of MASTER OF ENGINEERING IN MECHANICAL ENGINEERING Approved: _________________________________________ Ernesto Gutierrez-Miravete, Project Adviser Rensselaer Polytechnic Institute Hartford, Connecticut April, 2012 (For Graduation May, 2012)

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Page 1: Acharya FinalReport

Creep Analysis of a Thick Walled Spherical Pressure Vessel

Considering Large Strain

by

Tushar Kanti Acharya

A Project Submitted to the Graduate

Faculty of Rensselaer Polytechnic Institute

in Partial Fulfillment of the

Requirements for the degree of

MASTER OF ENGINEERING IN MECHANICAL ENGINEERING

Approved:

_________________________________________ Ernesto Gutierrez-Miravete, Project Adviser

Rensselaer Polytechnic Institute Hartford, Connecticut

April, 2012 (For Graduation May, 2012)

Page 2: Acharya FinalReport

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© Copyright 2012

by

Tushar Kanti Acharya

All Rights Reserved

Page 3: Acharya FinalReport

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CONTENTS

Creep Analysis of a Thick Walled Spherical Pressure Vessel Considering Large

Strain……………………………………………………………...…………………...…..i

LIST OF TABLES ............................................................................................................ iv 

LIST OF FIGURES ........................................................................................................... v 

LIST OF SYMBOLS (WITH UNITS) ............................................................................. vi 

ABSTRACT ................................................................................................................... viii 

1.  Introduction .................................................................................................................. 1 

2.  Theory .......................................................................................................................... 3

2.1. Assumptions………………………………………………………...……3

2.2 Derivation of Creep Strain Rate Equation…………….………….….3

2.3 Stress and Strain Distribution…………………………………………….5

2.4 Norton's Creep Law………………………………………………………5

2.5 Equivalent Stress ……………………………………………………...7

2.6 Radial Stress r and Effective Strain Rate as Functions of Radius……..7

2.7 Small Strain Solution for Radial and Tangential Stresses………………..8

3.  Results of Analytical Formulae ................................................................................. 11 

4.  Finite Element Analysis and Results ......................................................................... 15

4.1 Equations and Input for ANSYS Analysis……………………………...15

4.2 Coarse Mesh Results…………………………………………………….18

4.3 Fine Mesh Results……………………………………………………….23

4.4 Coarse Mesh vs. Fine Mesh……………………………………………..28

5.  Discussion .................................................................................................................. 30 

6.  Conclusions ................................................................................................................ 31 

7.  References .................................................................................................................. 32

Appendix………………………………………………………………………………33

Page 4: Acharya FinalReport

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LIST OF TABLES

Table Description Page

1 Data for Exact Solution 11

2 Data for Analysis 16

3 Coarse and Fine Mesh Comparison 17

4 von Mises Stress Comparison (Coarse Mesh,2300days) 19

5 von Mises Creep Strain Comparison (Coarse Mesh,2300days) 20

6 von Mises Stress Comparison (Coarse Mesh, 2300days) 21

7 von Mises Creep Strain Comparison (Fine Mesh, ε=1.03) 23

8 von Mises Stress Comparison (Fine Mesh,3000days) 24

9 von Mises Creep Strain Comparison (Fine Mesh, ε=0.6) 25

10 von Mises Stress Comparison (Fine Mesh,3000days) 26

11 Percentage Result Deviation of Finite Element model vs. Exact Solution 29

Page 5: Acharya FinalReport

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LIST OF FIGURES

Figure Description Page

1 Creep Rate vs. Strain, both at Internal Radius 11

2 Strain at Internal Radius vs. Time 12

3 Tangential Strain Rate ε't at various Radii of Spherical Vessel 13

4 Stress Distribution at Various Radii of Vessel for εa=0.0 14

5 Stress Distribution at Various Radii of Vessel for εa=0.62 14

6 A Hemispherical part, inner and outer radius are 20in and 100in 17

7 A Hemispherical meshing shown with SOLID187 18

8 Coarse Mesh, von Mises Creep strain at internal radius 19

9 Coarse Mesh, von Mises Creep Stresses at internal radius,

with ε=0.93 and Time=3000days 20

10 Course Mesh, von Mises Creep strain at internal radius

for Time=2300days 21

11 Coarse Mesh, von Mises Creep Stresses at internal radius,

with ε=0.56 and Time=2300days 22

12 Comparison between Coarse Mesh and Exact Solution Results 23

13 Fine Mesh, von Mises Creep strain at internal radius

for Time=3000days 24

14 Fine Mesh, von Mises Creep Stresses at internal radius,

with ε=1.0 and Time=3000days 25

15 Fine, von Mises Creep strain at internal radius

for Time=2300days 26

16 Fine Mesh, von Mises Creep Stresses at internal radius,

with ε=0.6 and Time=2300days 27

17 Comparison between Fine model and Exact Solution 28

18 Comparison between Coarse vs. Fine w.r.t.Exact Solution 29

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LIST OF SYMBOLS (WITH UNITS)

Functions

)'(f function of effective creep strain

Geometry:

a inner radius of sphere (inches)

b outer radius of sphere (inches)

r radius of sphere at random position (inches)

r’ an element at radius r with further very small displacement u

x,y,z coordinate axis

Mechanical Data

E Young’s Modulus (psi)

B,C1,C2,C3,n experimental material constants

c material constant (psi)

Pressure

p internal pressure of spherical vessel (psi)

Strain and Strain Rate

ε effective strain

ε’ effective strain rate

a effective strain at inner radius a

b effective strain at outer radius b

'a strain rate at inner radius a

'b strain rate at outer radius b

εr radial strain

εt tangential strain

Stress

effective stress (psi)

a effective stress at radius a (psi)

b effective stress at radius b (psi)

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r radial stress (psi)

t tangential stress (psi)

FH effective stress per Finnie and Heller (psi)

rFH radial stress per Finnie and Heller (psi)

tFH tangential stress per Finnie and Heller (psi)

Time

t time (seconds)

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ABSTRACT

In this report, the creep analysis of a thick walled spherical pressure vessel made of

a homogeneous and isotropic material and subjected to internal pressure is considered.

Spherical vessels are used as pressure vessels in power plants and in petrochemical

industry. Creep analyses of thick-walled spherical pressure vessels subjected to internal

and or external pressure are important in solid mechanics and in engineering

applications. In engineering design predicting the behavior of creep over the long term is

important. The strains considered are assumed to be large which necessitates the use of

finite strain theory for evaluating the expressions for stresses, creep strains and strain

rates. The general theory developed by N.S. Bhatnagar and V.K. Arya (1973) has been

applied to the solution of a specific problem using Norton’s law of creep. The

infinitesimal (small) strain discussion by Finnie and Heller (1959) was also considered

for comparison. In addition, a finite element approach has been implemented using

ANSYS. The analysis and numerical example will aid the designers in the prediction of

correct creep strains, strain rates and stresses in cases where large creep deformations of

spherical pressure vessels are permissible.

Page 9: Acharya FinalReport

1. Introduction

The problem of creep deformation of thick-walled spherical pressure vessels has

been studied previously (3). Most studies assume that the strains are small and that

deformations can be referred to the original dimensions of the vessels rather than the

instantaneous deformed values. While these assumptions are sufficiently accurate for

small strains, under longer time exposures the deformations may attain a value where

small strains can no longer be assumed. With this in mind an attempt has been made by

Bhatnagar and Arya (1) to solve the problem of creep deformation of thick-walled

spherical vessels under internal pressure considering large strains. This study is based on

a steady state law for creep together with the assumption of a homogeneous,

incompressible, isotropic material.

The finite strain theory, developed in (2), for the case of plastic flow of thick-walled

tubes with large strains, has been extended for application to the creep deformation of a

thick-walled spherical pressure vessel. In this project various expressions for stresses,

strains and creep rates, based both on infinitesimal and finite strain theories are

presented following the descriptions in (1) and (3).

The large amount of previous work has been concerned with the investigation of

stresses and strains in the wall of the vessel assuming the infinitesimal strain theory to be

valid. For the elastic deformations and the early stages of creep, the assumption that the

strains are infinitesimal yields values of stresses and strains which are in good agreement

with the experimental observations. But under longer time creep deformation conditions

the strains keep accumulating and may reach a value so large that the use of infinitesimal

strain theory for the evaluation of stresses and strains is no longer valid.

In finite element analysis, membrane forces and bending moments of the nodes

cannot be easily expressed as due to implicit functions of strain-rate because of the high

nonlinearity of stress-strain relation in creep. These appear to be the main reasons why

the published literature, so far, is directed mainly towards problems of simpler nature

such as hollow hemispherical pressurized vessel. Even in these cases, some

simplifications have been usually introduced.

Page 10: Acharya FinalReport

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In chapter 2 below the large formulation of the problem is first presented and

followed by the small strain formula. Chapter 3 then presents results obtained using the

above formulae. Chapter 4 contains the finite element model results.

Page 11: Acharya FinalReport

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2. Theory

These chapter presents the development of large and small strain theory of creep of

hollow spherical pressure vessel. The large strain formulation follows (1) and small

strain development follows (3).

Consider a spherical vessel of internal and external radii a and b, respectively,

subjected to internal pressure p.

2.1 Assumptions

To investigate the deformation behavior of the vessel at high temperatures, where

creep is dominant the following assumptions are made.

1. The material is homogeneous and isotropic.

2. The volume of the material remains constant (condition of incompressibility).

Creep has no effect on the density of the material as summation of creep rates in

the three principal directions is zero.

3. The ratios of the principal shear strain-rates to the principal shear stresses are equal.

4. The effective stress and effective strain (creep) rate , are related by

σ =f(ε’). [1]

2.2 Derivation of Creep Strain Rate Equation

By symmetry, the principal stresses in the two tangential directions are equal. We

shall denote the stresses and creep rates in radial and tangential directions by subscripts r

and t, respectively.

It may also be concluded from symmetry that the only displacement in this problem

is radial and is such that concentric spherical surfaces remain concentric and spherical

after deformation.

Considering the radial equilibrium in the deformed state, the mechanical

equilibrium equation is

Page 12: Acharya FinalReport

4

)(2'

' rtr

dr

dr

[2]

The equation of compatibility is

1 tre

rr t

[3]

The effective stress σ and effective strain ε equations are

rt [4]

and

)(3

2rt [5]

The condition of incompressibility is

rt 2 [6]

The creep strain rate at any radius r as a function of given creep rate at the inner

radius a, is

'

)2/3(

)2/3(

)1()(1

)('

3

3

aa

a

er

a

er

a

[7]

Relation between creep strain rates and the creep strains is

'

)2/3(

)2/3(

1

1' aae

e

[8]

The equation for internal pressure p in terms of creep rate as

a

b

dp'

'

''3

2

[9]

Where

Page 13: Acharya FinalReport

5

'

)2/3(3

)2/3(3

'

)1()(1

)(

aba

a

eb

a

eb

a

[10]

is the creep rate at the outer radius.

2.3 Stress and Strain Distribution

The effective stress can be obtained as a function of r from Eqn.1, provided the

effective strain a and creep rate'a , both at the inner radius a , are given.

The equation for radial stress r , at any radius r is given as

a

dpr

'

'

''3

2

[11]

And, the tangential stress at any radius r is given as

)'('

'3

2'

'

fdpa

t [12]

The creep rate t' , in the tangential direction, can then be obtained as

'

)2/3(

)2/3(

'

)1()(1

)(

2

13

3

ata

a

er

a

er

a

[13]

2.4 Norton’s Creep Law

Under secondary creep conditions, the effective stress and creep rate ' are

assumed to be related by Norton’s Law

Page 14: Acharya FinalReport

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n

c

B )(' [14]

Where B , n and c are experimental constants and c has the dimensions

of .

Eqn.14 can be rewritten as

)/1(

)/1(' n

nc

B

[15]

From Eqn.9, the equation for internal pressure p in terms of'a ,

'b , c , B and n

is

)(

3

2 )/1(')/1(')/1(

n

b

n

anc

B

np

[16]

From this and Eqn.10, the creep rate 'a at ar as a function of the strain

at ar , a is given as

nnnn

cn

nn

aa

a

eb

a

eb

a

n

Bp

]}

)1()(1

)({1[

2

3' /1

)2/3(

)2/3(

3

3

[17]

Note that the creep rate is function of the creep strain. Integrating Eqn.17 and

simplifying, the strain a can be obtained as a function of time t, given by

a

a

a

tn

Bp

eb

a

eb

a

nnc

n

nnnn

0

/1

)2/3(

)2/3(

2

3]}

)1()(1

)({1[

3

3

[18]

This expression can then be numerically integrated to compute the strain at the inner

radius for any given time.

Page 15: Acharya FinalReport

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2.5 Equivalent Stress

To find an alternate numerical solution for Equivalent stress at various radii of

vessel we use Eqn.7 in Eqn.15, to obtain

'/1

)2/3(

)2/3(

/1]

)1()(1

)([

3

3

an

nc

a

a

er

a

er

a

B

[19]

Inserting the expression for 'a from Eqn.17 in Eqn.19

]})1()(1

)({1[

])1()(1

)([

2

3

/1

)2/3(

)2/3(

/1

)2/3(

)2/3(

3

3

3

3

n

n

a

a

a

a

eb

a

eb

a

er

a

er

a

n

p

[20]

2.6 Radial Stress r and Effective Strain Rate as Functions of Radius

To find an expression for the radial stress at various radii of the vessel we insert

Eqn.15 in Eqn.11, to obtain

'

'

)1

(

)/1(''

3

2 a

dB

p n

n

nc

r

'

'/1

)/1(]'[

3

2an

nc n

Bp

[21]

Page 16: Acharya FinalReport

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However, since this

)/1()/1('

')/1( ']'[

' nn

an a

[22]

Using Eqn.7 in Eqn.22, we get

]})1()(1

)({1[']'[ )/1(

)2/3(3

)2/3(3

)/1('

)/1( ' nna

n

a

a

a

er

a

er

a

.

[23]

Combining Eqn.23, Eqn.17 and Eqn.21, we get

]

]})1()(1

)({1[

]})1()(1

)({1[

1[

/1

)2/3(3

)2/3(3

/1

)2/3(

)2/3(

3

3

n

n

r

a

a

a

a

eb

a

eb

a

er

a

er

a

p

[24]

Eqn.24 is a closed form expression of Eqn.11, which is used below in Fig-4 and 5 to

show the stress distribution at various radii.

2.7 Small Strain Solution for Radial and Tangential Stresses [3]

The expressions obtained for strain elastic and creep deformations are presented

below. The elastic stresses in a hollow sphere under internal pressure are given by the

Lame Equations

)2

1(3

3

33

3

r

b

ab

pat

[25]

Page 17: Acharya FinalReport

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)1(3

3

33

3

r

b

ab

par

[26]

Only two stresses need to be specified, since by symmetry the principal stresses in

the two tangential directions are equal. The condition of incompressibility

becomes drdur /'' and rut /'' , where u’ is the rate at which a radius r

is changing, we have

3'2'

r

Ctr [27]

In which C is a constant.

Now, the corresponding expressions for creep deformation are given.

Finnie & Heller [2] obtained theoretical expressions for creep stresses in spherical

vessel under small strain conditions assuming Norton’s Law. The equilibrium equation

per Finnie and Heller [2, Eqn7-35, p186] is

)(2 rFHtFHrFH

dr

dr

[28]

For a thick-walled creeping sphere under internal pressure prFH at ar

and 0rFH at br ; radial stress rFH [2, Eqn7-36, p187] is

]1)/[(

]1)/[(/3

/3

n

n

rFH ab

rbp [29]

so that

])(

[]1)/[(

)3

(3

/3

/3

n

n

n

nrFH

r

b

ab

p

ndr

d

[30]

Results obtained using Eqn.29 are shown in Fig-4 and Fig-5 for the assumption of

infinitesimal small strains for radial stresses.

Substituting Eqn.29 in Eqn.28, the tangential stress is obtained as

Page 18: Acharya FinalReport

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rr

tFH dr

dr 2 ]1)/[(

1]2

)23([)(

./3

/3

n

n

abn

n

r

b

p [31]

and the equivalent stress can be obtained as

rFHtFHFH [32]

Eqn.31 and Eqn.32 can be used to find the tangential stress in the spherical pressure

vessel for small strain conditions.

Page 19: Acharya FinalReport

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3. Results of Analytical Formulae

Using the formulation in chapter 2 above and the data considered by Bhatnagar and

Arya [1] and Rimrott [4] the creep deformation of a spherical vessel was investigated. The

following values of constants were taken.

Table-1: Data for Exact Solution

Descriptions Data

B 5.E-12 /day

σc 1000psi

n 6

b/a 5

p 40,000 psi

Fig-1 shows the effective creep rate a' at the internal radius a calculated in Excel

from Eqn.17 and plotted against the creep strain a at the internal radius. Note that the

creep strain rate increases with increasing creep strain.

Fig-1: Creep Rate Vs Strain, both at Internal Radius

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Fig-2 shows the computed creep strain as a function of time obtained by numerical

integration of Eqn.18. The graph clearly indicates that the effective creep strain increases

with time. Moreover the figure also shows that the creep strain rate is not constant but

increases with time.

Fig-2: Strain at Internal Radius vs. Time

The tangential creep rate t' at various radii of the vessel was calculated from

Eqn.13 and Eqn.17, and is shown in Fig-3 for three values of the effective creep strain at

the inner radius a viz. 0.24, 0.56 and 0.76. From Fig-3 it is observed that for all radii,

the tangential creep strain rate increases with time. It is also observed that the tangential

creep strain rate decreases first quickly then slowly towards zero with distance from the

inner radius of sphere to the outer radius.

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Fig-3: Tangential Strain Rate ε't at various Radii of Spherical Vessel

Fig-4 shows the distributions of radial tangential and equivalent stresses in the wall

of the vessel as obtained from Eqn.4, 20 and 24 at time zero. Also the radial, tangential

and equivalent stresses for small strain described by Finnie and Heller [2] are shown

(Eqn.29, 31 and 32). As expected, the results are very close since the computed strain

correction is negligible in this case.

The stress distribution in the wall of the vessel for 62.0a is shown in Fig-5.

Here stress distributions are shown following a considerable amount of deformation. The

radial, tangential and equivalent stresses for small strain described by Finnie and Heller

[2] are also plotted in Fig-5 (Eqns.29, 31 and 32). In this case, larger differences exist

between the predictions of small and large strain theories.

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Fig-4: Stress Distribution at Various Radii of Vessel for εa=0.0

Fig-5: Stress Distribution at Various Radii of Vessel for εa=0.62

Page 23: Acharya FinalReport

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4. Finite Element Analysis and Results

In this project a finite element model was developed to compare with the results of

Bhatnagar and Arya. The finite element model was created using ANSYS Student

version 13 and the Norton Creep theory was applied. A hemisphere model was analyzed.

Although the analysis are made for a hemisphere and clamped to annular surface, the

method is quite general and other types of shells boundary conditions and geometries

can be treated similarly.

In ANSYS the vessel was modeled as a hollow hemisphere (Fig-6) and SOLID187

elements were used for meshing (Fig-7). SOLID187 element is a higher order 3-D,

tetrahedral 10-node element. SOLID187 has a quadratic displacement behavior and is

well suited to modeling irregular meshes and non-linear problems.

The element is defined by 10 nodes having three degrees of freedom at each node:

translations in the nodal x, y, and z directions. The element has plasticity, hyper-

elasticity, creep, stress stiffening, large deflection, and large strain capabilities. It also

has a mixed formulation capability for simulating deformations of nearly incompressible

elasto-plastic materials, and fully incompressible hyper-elastic materials. [10] SOLID187

gives better approximation over Axi-symmetric element PLANE182; hence it is used for

the analysis.

4.1 Equations and Input for ANSYS Analysis

For Finite Element Analysis using the program ANSYS, Norton’s Law (Eqn.14

above) is written as (ANSYS Creep Model 10)

)exp()(' 31

2

T

CC C

nnc

B

)( [33]

Where nc

BC

1 , nC 2 and 03 C

The input data included in Table-2 were used in the calculations.

Page 24: Acharya FinalReport

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Table-2: Data for Analysis

Descriptions First Set Analysis Data Second Set Analysis Data

B 5.E-12 /day 5.E-12 /day

c 1000psi 1000psi

n 6 6

C1 (Eqn.45) 5.E-30 5.E-30

C2(Eqn.45) 6 6

C3(Eqn.45) 0 0

Internal Radius, a 20in 20in

Outer Radius, b 100in 100in

Internal Pressure, p 40,000 psi 40,000 psi

Young’s Modulous, E 5.5E6 psi 5.5E6 psi

Poisson’s Ratio 0.3 0.3

Number of Days to be

analyzed

3000 2300

In ANSYS the implicit Norton Creep model (Model 10) was selected in Material

modeling and considered half of a hollow sphere in analysis. A displacement DY=0 was

applied to the circular plane of the hemi-sphere, so that rigid body motion was avoided.

Pressure, p is applied to the inner surface of the sphere. The analysis was done for two

sets of data, 2300 days and 3000 days. The results are shown below.

In Fig-6 the hemispherical part is shown, which was considered for the analysis.

The hemisphere considered is a part of a thick spherical vessel under high internal

pressure of 40,000 psi. The inner radius is 20in and the outer radius of sphere is 100in. A

sample ANSYS input file is included in the Appendix.

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Fig-6: A Hemispherical part, inner and outer radius are 20in and 100in

Fig-7 shows the meshed model. The increase in number of elements increases the

time required for solutions. In this paper results obtained using 4 and 5 subdivisions for

each main line in the geometry are compared. Table-3 shows the resulting discretization

in each case.

Table-3: Coarse and Fine Mesh Comparison

Mesh Type in Model Elements Nodes

4 Line Subdivision

(Coarse Mesh)

643 1144

5 Line Subdivision

(Fine Mesh)

1336 2223

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Fig-7: A hemispherical meshing shown with SOLID187 elements

4.2 Coarse Mesh Results

Results obtained using ANSYS with the coarse mesh consisting of 643 elements are

now presented.

Fig-8 shows that the von Mises creep strain at the internal radius of the sphere

increases with time. The slope approximately matches that of the Exact Solution per

Bhatnagar and Arya’s. The creep strain at 3000days is 0.93 while per Exact Solution the

creep strain is 1.0 for 2984days. Fig-8 also shows that the creep strain rate increases with

time in agreement with the previous result (Fig.-1).

Page 27: Acharya FinalReport

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Fig-8: Coarse Mesh, von Mises Creep strain at internal radius

Fig-9 shows the computed von Mises creep stress in the hemisphere at 3000days.

The stress varies from 22743psi to 13493 from the inner to the outer radius. Per Exact

Solution for creep strain ε =0.93, the equivalent stress varies from 22802 psi to 12802

psi (see Table-4 and Fig-12 below).

Table-4: von Mises Stress Comparison (Coarse Mesh,2300days)

Radius )(exactm )(Ansysm %age Deviation

a = 20in 22802 22743 0.3

b = 100in 12802 13493 5.4

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Fig-9: Coarse Mesh, von Mises Creep Stresses at internal radius,with ε=0.93 and

Time=3000days

Fig-10 shows the von Mises creep strain at the internal radius of the sphere as a

function of time for up to 2300days. Bhatnagar and Arya [1] discussed the results of their

model at effective creep strain ε =0.62. So for comparison we have included this time

line. It is observed that the effective creep strain increases with time. The creep strain at

2300days is 0.56 in ANSYS while per Exact Solution the creep strain is 0.56 for

2191days. The agreement is reasonable but ANSYS seems to under predict the strain

(Table-5).

Table-5: von Mises Creep Strain Comparison (Coarse Mesh,2300days)

Radius )(exact )(Ansys %age Deviation

a = 20in 0.6 0.56 6.7

Page 29: Acharya FinalReport

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Fig-10: Coarse Mesh, von Mises Creep strain at internal radius for Time=2300days

Fig-11 shows the computed von Mises creep stress in the hemisphere for a time

period of 2300days (and effective creep strain ε=0.56). Per analysis it is observed that

the stress varies from 19764psi to 10841 from inner to outer radius. Per Exact Solution

for creep strain ε =0.56 the equivalent stress varies from 20550 psi to 10550psi. This has

been plotted in Fig-12 (see also Table-6).

Table-6: von Mises Stress Comparison (Coarse Mesh, 2300days)

Radius )(exactm )(Ansysm %age Deviation

a = 20in 20550 19764 3.8

b = 100in 10550 10841 2.8

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Fig-11: Coarse Mesh, von Mises Creep Stresses at internal radius,with ε=0.56 and

Time=2300days

Fig-12 plots the von Mises and Equivalent stresses at strains ε=0.93 and 0.56, as

functions of radius obtained from ANSYS and from the Exact solution respectively. The

Equivalent stress at ε=0.56 is aligned approximately with ANSYS calculated von Mises

stress. The same result is observed for ε=0.93. It is also shown that the ANSYS von

Mises stress values are slightly higher than the Exact stress. It seems that the ANSYS

values are more stringent than those obtained from the Exact Solution. So for design

purposes the ANSYS values are preferred.

Page 31: Acharya FinalReport

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Fig-12: Comparison between Coarse Mesh and Exact Solution Results

4.3 Fine Mesh Results

Fig-13 shows how the von Mises creep strain at the internal radius of sphere

increases with time for the Fine mesh model. The effective creep strain is 1.03 at

3000days. The creep strain is 1.03 for 3019 days per Exact Solution. The result is

slightly higher than the Coarse Mesh and Exact Solution results. This is an effect of the

finer mesh used (see Table-7). Table-7 shows von Mises creep strain deviation of

approx.0.60% at the creep strain ε=1.03.

Table-7: von Mises Creep Strain Comparison (Fine Mesh, ε=1.03)

ε )(exactDays )(AnsysDays %age Deviation

1.03 3019 3000 0.6

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Fig-13: Fine Mesh, von Mises Creep strain at internal radius for Time=3000days

Fig-14 shows the von Mises creep stress in the hemisphere obtained from ANSYS

at time 3000 days (and effective creep strain ε=1.03 (approx)). Per analysis it is observed

that the von Mises stress varies from 24171 psi to 14777 psi from the inner to the outer

radius. Per Exact Solution for the creep strain ε =1.03 the equivalent stress varies from

23573 psi to 13573 psi. This has been plotted in Fig-7 and tabulated in Table-8. The

table shows that the ANSYS von Mises stress is more stringent with a 8.9% deviation at

the outer radius and a 2.5% deviation at the inner radius.

Table-8: von Mises Stress Comparison (Fine Mesh,3000days)

Radius )(exactm )(Ansysm %age Deviation

a = 20in 23573 24171 2.5

b = 100in 13573 14777 8.9

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Fig-14: Fine Mesh, von Mises Creep Stresses at internal radius,with ε=1.0 and

Time=3000days

Fig-15 shows the von Mises creep strain at the internal radius of the sphere for time

period up to 2300 days. The creep strain at 2300 days is 0.6 in ANSYS while per Exact

Solution the creep strain is 0.6 for 2291days (Table-9). The ANSYS result seems to

under predict the Exact solution but it is better than the Coarse mesh results. Table-8

shows that the von Misses creep strain %age deviation is 0.4 compare to coarse mesh

with 0.6.

Table-9: von Mises Creep Strain Comparison (Fine Mesh, ε=0.6)

ε )(exactDays )(AnsysDays %age Deviation

0.6 2291 2300 0.4

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Fig-15: Fine, von Mises Creep strain at internal radius for Time=2300days

Fig-16 shows the von Mises creep stress in the hemisphere for a time period of

2300days (and effective creep strain ε=0.6). Per analysis it is observed that the stress

varies from 20488psi to 11257 from inner to outer radius. Per Exact Solution for creep

strain ε =0.6, the equivalent stress varies from 20779 psi to 10779psi. This has been

plotted in Fig-17 (see also Table-10). The von Mises stresses in ANSYS have higher

deviation at the outer radius than at the inner radius.

Table-10: von Mises Stress Comparison (Fine Mesh,3000days)

Radius )(exactm )(Ansysm %age Deviation

a = 20in 20779 20488 1.4

b = 100in 10779 11257 4.4

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Fig-16: Fine Mesh, von Mises Creep Stresses at internal radius,with ε=0.6 and

Time=2300days

Fig-17 shows the Equivalent and von Mises stresses at ε=1.03 and 0.6, calculated

from the Exact Formula and from ANSYS respectively as functions of radius. The

equivalent stress obtained from Exact Formula at ε=0.6 agrees well with the ANSYS von

Mises stress. However, the ANSYS von Mises stress values are slightly higher than the

Exact Solution Equivalent stress values for ε=1.03. It seems that the ANSYS values are

more stringent than those obtained from Exact Solution. So for design purposes the

ANSYS values are preferred.

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Fig-17: Comparison between Fine Mesh Model and Exact Solution

4.4 Coarse Mesh Vs. Fine Mesh

Fig-18 shows a summary of results comparing the Exact Equivalent stress at ε=1.0

and 0.6, the ANSYS von Mises stress at ε=1.03 and 0.6 using the fine mesh and the

ANSYS von Mises stresses at ε=0.93 and 0.56 using the coarse mesh model as functions

of the radius inside the sphere. The equivalent stress at ε=0.6 is aligned approximately

with the ANSYS von Mises stresses both for the coarse and fine mesh models. The

ANSYS result matches Bhatnagar and Arya’s results well up to the creep strain ε=0.6,

but for higher creep strain values the ANSYS von Mises results are higher than the Exact

values.

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Fig-18: Comparison between Coarse vs. Fine Mesh and w.r.t. Exact Solution

In Table-11 we have summarized the deviations between the von Mises and

Effective stress results obtained from ANSYS and from the Exact solution. It is observed

that for the effective creep strain ε=0.6, the percentage deviation is +3.8% to -3.7%.

While for effective creep strain ε=1.0, the percentage deviation is +0.26% to -5.63%.

Table-11: Percentage Result Deviation of Finite Element model vs. Exact Solution

Description of Model Detail Maximum Deviation %

Minimum Deviation %

ANSYS Coarse Mesh 3000day vs. Exact Solution 0.26% -5.63%ANSYS Coarse Mesh 2300day vs. Exact Solution 3.82% -3.70%ANSYS Fine Mesh 3000day vs. Exact Solution -2.54% -9.57%ANSYS Fine Mesh 2300day vs. Exact Solution 1.40% -6.22%

In Table-11, the negative value indicates that the ANSYS results are higher than

those from the Exact Solution.

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5. Discussion

From the analytical results for the large strain creep deformation of a thick walled

hollow spherical vessel shown in Fig-1, it is observed that the creep strain rate at the

inner radius 'a increases with strain. Fig-2 shows that the creep strain increases non-

linearly with time as the deformation under creep continues. Moreover the creep rate is

not constant but increases with time. In Fig-3 the tangential creep rate 't is found to

decrease rapidly with increasing radius for all the three values of a . The significant

results of the present investigations are observed in Fig-4 and Fig-5. The figures show a

negligibly small difference between the two stress distributions based on the

assumptions of finite and infinitesimal strains for 0a i.e. at the outset of the creep

process (i.e. 0a ), as it should be. However, after a considerable deformation under

creep (i.e. for 6.0a ) the difference between the radial and tangential stresses and for

the effective stress for the two assumptions, is quite large. It is to be expected that as the

strain at the inner boundary increases from its initial value, the radial, tangential and

effective stresses all increase continuously and the difference in the predictions from the

two theories goes on increasing.

The Finite Element model results show that the values of von Mises creep strain rate

and von Mises creep stress match those predicted by the Bhatnagar and Arya’s solution.

But when analyzing beyond the creep strain ε=0.6, the ANSYS predicted von Mises

stresses are higher than the Exact Solution values. The analysis results are not

significantly higher, but from design point of view they are noticeable. So for better

accuracy a designer should consider a finite element analysis for worst scenario cases.

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6. Conclusions

In this work, a comparison is made between the Theory by Bhatnagar and Arya and

Finite Element Analysis for the creep analysis of isotropic and homogeneous thick-

walled spherical pressure vessels. Results show that the creep rate of the thick-walled

spherical vessel increases rapidly even though the creep rate of the same material when

subjected to constant true stress in simple tension is constant. This is an important effect

which is overlooked in the analyses making use of the infinitesimal strain theory.

Therefore, the predictions based on the results from small or infinitesimal strain analyses

would be on unsafe side from a design point of view. The results from (1) have been

verified in ANSYS and good agreement has been found.

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7. References

1. Bhatnagar, N.S. and Arya, V.K., Creep of Thick-walled spherical vessels under

internal pressure considering large strains, by. (Department of Mathematics,

University of Roorkee, Roorkee),1973.

2. MacGregor, C. W., Coffin, L. F., and Fisher, J. C. The plastic flow of thick-

walled tubes with large strains. J. appl. Phys., 19, 1948, p. 291.

3. Creep of engineering materials, Finnie, I., Heller, W.R., 1959. McGraw-Hill

Book Co., Inc., New York.

4. Johnson, A.E. and Khan, B., Creep of Metallic Thick-walled spherical vessels

subject to pressure and radial thermal gradient at elevated temperatures, Int. J.

Mech. Sci.,. Vol. 5, 1963, pp. 507-532.

5. Rimrott, F.P.J., Creep of thick-walled tubes under internal pressure considering

large strains, J.Appl.Mech. 26; Trans.ASME.Ser.E.81, 1959, p271.

6. You, L.H. and Ou, H., Steady-state creep analysis of thick-walled spherical

pressure vessel with varying creep properties, Journal of Pressure Vessel

Technology, ASME FEBRUARY 2008, Vol. 130. Issue 1, pp 014501-1-5.

7. Miller, G.K., Stresses in a spherical vessel undergoing creep and dimensional

changes, Int. J. Solids Structures Vol. 32, No. 14, 1995, pp. 2077-2093,

8. Arya, V.K., Debnath, K.K. and Bhatnagar, N.S., The spherical vessel with

anisotropic creep properties considering large strains, Int. J. Nonlinear

Mechanics, Vol. 15, 1980, pp. 185-193.

9. Nejad, M.Z., Hoseini, Z., Niknejad, A., and Ghannad, M., A New Analytical

Solution for Creep Stresses in Thick-walled Spherical Pressure Vessels, Journal

of Basic and Applied Scientific Research, 1 (11), 2011, p2162-2166,

10. Mechanical Behavior of Engineering Materials by Joseph Marin, Prentice Hall

Inc. 1962.

11. ANSYS Mechanical APDL Technical Manual

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Appendix !* /PREP7 !* /NOPR KEYW,PR_SET,1 KEYW,PR_STRUC,1 KEYW,PR_THERM,0 KEYW,PR_FLUID,0 KEYW,PR_ELMAG,0 KEYW,MAGNOD,0 KEYW,MAGEDG,0 KEYW,MAGHFE,0 KEYW,MAGELC,0 KEYW,PR_MULTI,0 KEYW,PR_CFD,0 /GO !* /COM, /COM,Preferences for GUI filtering have been set to display: /COM, Structural !* !* ET,1,SOLID187 !* KEYOPT,1,6,0 !* MPTEMP,,,,,,,, MPTEMP,1,0 MPDATA,EX,1,,5.5e6 MPDATA,PRXY,1,,0.3 TB,CREE,1,1,3,10 TBTEMP,0 TBDATA,,5e-30,6,0,,, SPHERE,100,20,0,180, /VIEW,1,,-1 /ANG,1 /REP,FAST !* LESIZE,ALL, , ,5, ,1, , ,1, MSHKEY,0 MSHAPE,1,3d CM,_Y,VOLU VSEL, , , , 1 CM,_Y1,VOLU CHKMSH,'VOLU' CMSEL,S,_Y !* VMESH,_Y1 !* CMDELE,_Y CMDELE,_Y1 CMDELE,_Y2 !* FLST,2,2,5,ORDE,2 FITEM,2,5

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FITEM,2,-6 !* /GO DA,P51X,UY,0.0 FLST,2,2,5,ORDE,2 FITEM,2,3 FITEM,2,-4 /GO !* SFA,P51X,1,PRES,40000 TUNIF,723, /solu antype,static ! no inertia effects, so transient not needed ... nlgeom,on TUNIF,723, time,1.0e-5 deltim,1.0e-5,1.0e-8,1.0e-5 rate,off solve save time,10 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,20 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,30 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,40 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,50 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve

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save time,100 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,200 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,300 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,400 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,500 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,600 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,700 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,800 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save

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time,900 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,1000 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,1100 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,1200 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,1300 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,1400 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,1500 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,1600 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save

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time,1700 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,1800 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,1900 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,2000 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,2100 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,2200 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,2300 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,2400 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save

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time,2500 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,2600 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,2700 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,2800 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,2900 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save time,3000 deltim,2.0e2,1.0e-1,200 ! largest time step = 200 days ... rate,on,on nlgeom,on ! load drop matches cross section area decrease solve save fini