Failure Theoriegggs
Failure Theoriegggs
                                   From the available experimental data, brittle failure is governed by one of the
                                   three accepted theories that follow.
σut
                                                                                                                σ1
                                                                σuc                                 σut
σuc
Figure 7.1 The failure envelope according to the maximum principal stress theory when σ3 = 0.
159
                                                                                 σ1            σ2
                                                                First quadrant:         or          = 1,                             (7.1)
                                                                                 σut          σut
                                                                                  σ1             σ2
                                                                Third quadrant:           or         = −1,                           (7.2)
                                                                                  σuc           σuc
                                                                                     σ1       σ2
                                                                Second quadrant:         +        = 1,                               (7.3)
                                                                                     σuc     σut
                                                                                   σ1        σ2
                                                                Fourth quadrant:         +       = 1.                                (7.4)
                                                                                   σut      σuc
                                   As shown in Fig. 7.2, the effect of stress coupling is present in the second and
                                   fourth quadrants.
σ2
σut
                                                                                                                σ1
                                                                σuc                                 σut
σuc
Figure 7.2 The failure envelope according to the Mohr-Coulomb theory when σ3 = 0.
                                                                                       1
                                                                               1   =     [σ1 − νσ2 ],
                                                                                       E
                                                                                       1
                                                                               2   =     [σ2 − νσ1 ].                                (7.5)
                                                                                       E
                                   Then the failure envelope in the stress plane is governed by σ1 − νσ2 = a constant.
                                   This can be sketched as shown in Fig. 7.3.
σ2
σut
                                                                                                                  σ1
                                                                 σuc                               σut
σuc
Figure 7.3 The failure envelope according to the maximum principal strain theory when σ3 = 0.
                                   Our discussion here concerns epoxy matrix composites with glass, boron, or
                                   graphite fibers and with well-defined symmetry axes. Failure in this group of
                                   composites can be characterized as brittle. In intermetallic composites in which
                                   two or more metals form the constituents and, in general, in composites with
                                   metal components, ductile failure through yielding has to be taken into account.
                                   As shown in Fig. 7.4, we denote the fiber direction by x1 and the mutually
                                   orthogonal directions perpendicular to the fiber directions by x2 and x3 .
                                                                     y               x2
                                                                                                             x
x1
                                      Uniaxial tests with a specimen oriented in the fiber direction x1 and in the
                                   perpendicular directions x2 and x3 determine the failure strengths X 1 , X 2 , and X 3 ,
                                   respectively. Additional shearing tests are conducted along the planes tangential
                                   to the fibers to obtain shear strengths S12 and S13 . With these data, the objective
                                   of a failure theory is to predict failure in a multicomponent stress situation.
                                   Table 7.1 shows the elastic and failure properties of glass/epoxy, boron/epoxy, and
                                   graphite/epoxy composites. The subscripts in X 1t and X 1c indicate the values in
                                   tension and compression, respectively. We note the failure stresses in compression
                                   can be quite different from those in tension for some of these materials.
                                           Table 7.1. Elastic and failure properties of selected composites from Jones (1975)
                                             Property          Unit          Glass/epoxy         Boron/epoxy         Graphite/epoxy
                                             E1                (GPa)              53.78               206.84              206.84
                                             E2                (GPa)              17.93                20.68                   5.17
                                             ν12                                   0.25                 0.3                    0.25
                                             G                 (GPa)               8.96                 6.89               52.59
                                             X1t               (MPa)           1034.22               1379.00             1034.21
                                             X1c               (MPa)           1034.22               2757.90              689.48
                                             X2t               (MPa)              27.58                82.74               41.37
                                             Y2c               (MPa)            137.90                275.79              117.21
                                             S12               (MPa)              41.37               124.11               68.95
                                   (G + H )σ11
                                            2
                                               + (H + F)σ22
                                                         2
                                                            + (F + G)σ33
                                                                      2
                                                                         − 2(H σ11 σ22 + Gσ22 σ33 + Fσ33 σ11 ),
                                                                               2                  
                                                                           + 2 Lσ23 + Mσ13
                                                                                        2
                                                                                           + N σ12
                                                                                                2
                                                                                                     = 1.                             (7.8)
                                   The three separate conditions we have seen before are now reduced to a single
                                   condition. This adds one more constant. By applying the stress components one
                                   at a time, we have, when σ12 and σ13 act alone, failure results if
                                                                                    1                     1
                                                                         2N =       2
                                                                                       ,      2M =        2
                                                                                                             .                (7.9)
                                                                                   S12                   S13
                                   Using σ11 , σ22 , and σ33 , one at a time, we find
                                                                        1                       1                   1
                                                        G+H =                ,   H+F=                ,     F +G =        .   (7.10)
                                                                        X 12                    X 22                X 32
                                   We need one more shear test in the 23-direction to find
                                                                            1
                                                                      L= 2 .                                                 (7.11)
                                                                           S23
                                   If we impose the additional condition that the directions 2 and 3 are indistin-
                                   guishable, we have
                                                                           X 2 = X 3,         S12 = S13 .                    (7.12)
                                   This reduces the six constants to four. For the case of plane stress, this failure
                                   criterion reduces to
                                                                     σ11
                                                                      2
                                                                            σ11 σ22   σ22
                                                                                       2
                                                                                             σ12
                                                                                              2
                                                                          −         +      +     = 1.                        (7.13)
                                                                     X 12     X 12    X 12    2
                                                                                             S12
                                   With a single component of stress σx x , we get
                                                                     
                                                cos4 θ      1      1                     sin4 θ   1
                                                       +       −         cos2 θ sin2 θ +        = 2 .                        (7.14)
                                                   2
                                                  X1        2
                                                           S12    X12
                                                                                           X 22  σx x
                                   This one condition replaces the three conditions of the maximum stress or strain
                                   theories. When all the normal stresses are tensile, the Tsai–Hill theory gives
                                   results close to the experimental values. In many cases, the failure strength in
                                   compression is different from that in tension. To account for this, linear terms in
                                   normal stresses are added to the Tsai–HIll criterion to obtain the Tsai-Wu tensor
                                   criterion:
                                            F11 σ11
                                                 2
                                                    + F22 σ22
                                                           2
                                                              + F33 σ33
                                                                     2
                                                                        + 2(F12 σ11 σ22 + F13 σ11 σ33 + F31 σ33 σ11 )
                                                      + F1 σ11 + F2 σ22 + F3 σ22 = 1.                                        (7.15)
                                   This calls for additional compressive failure tests to determine the added three
                                   constants.
                                                                     σ2
                                                                          σy                                       σ2
                                                        σy
                                                                                           σ1
                                                                                      σy          σ3                        σ1
σy
(a) (b)
Figure 7.5 The yield envelope according to the Tresca theory when σ3 = 0.
                                   Eliminating the strain components in terms of stress components, the total energy
                                   density becomes
                                                              1 ! 2                                         "
                                                      U=         σ1 + σ22 + σ32 − 2ν(σ1 σ2 + σ2 σ3 + σ3 σ1 ) .    (7.21)
                                                             2E
dv = 1 + 2 + 3. (7.22)
                                   The work done by the hydrostatic stress due to the volume change is a part of the
                                   total energy, called the dilatational energy. This is obtained as
                                                                     1 σ1 + σ2 + σ3
                                                            Udil =                  ( 1 + 2 + 3 ),
                                                                     2       3
                                                                     σ1 + σ2 + σ3 1 − 2ν
                                                                   =                     (σ1 + σ2 + σ3 ),
                                                                           6         E
                                                                     1 − 2ν
                                                                   =        (σ1 + σ2 + σ3 )2 .                    (7.23)
                                                                       6E
                                   If we subtract Udil from U , what remains is the distortion energy Udis . We may
                                   imagine a unit volume undergoing a volume change with stored energy Udil and
                                   then a distortion, which stores an additional amount of energy Udis .
                                                 Udis = U − Udil ,
                                                         1   2             
                                                      =     3 σ1 + σ22 + σ32 − 6ν(σ1 σ2 + σ2 σ3 + σ3 σ1 )
                                                        6E
                                                          1 − 2ν  2
                                                        −          σ1 + σ22 + σ32 + 2(σ1 σ2 + σ2 σ3 + σ3 σ1 ) ,
                                                            6E
                                                        1+ν 2
                                                      =        σ1 + σ22 + σ32 − (σ1 σ2 + σ2 σ3 + σ3 σ1 ) .        (7.24)
                                                         3E
                                   According to the von Mises theory, a ductile material yields when the distortion
                                   energy Udis reaches a critical value. From a uni-axial test, the critical value for
                                   Udis is
                                                                                            1+ν 2
                                                                               Udis =           σ .               (7.25)
                                                                                             3E y
                                   This is an equation for an ellipse, with its major axis making 45◦ with the σ1 -
                                   direction. Fig. 7.6 shows the von Mises ellipse superposed on the Tresca hexagon.
                                   The ellipse becomes a circle when projected on to the π-plane. The yield behavior
                                   of steel is often modeled using either Tresca or von Mises theory.
σ2
                                                                      σ2
                                                                           σy
                                                                                                    σ3                           σ1
                                                         σy
                                                                                          σ1
                                                                                   σy
σy
Figure 7.6 The yield envelopes according to the Tresca theory and the von Mises theory when σ3 = 0.
7.4 Fatigue
                                   Experiments have shown that the strength of metals under incremental loading
                                   in tension (or compression) is substantially different compared to the case of
                                   cyclic loading. Anyone who has broken a paper clip by bending it back and
                                                                σm
                                                                                                    Δσ
                                   forth knows this. Fig. 7.7 shows an oscillating stress amplitude around a steady
                                   mean stress of σm . The difference between the maximum and minimum stress of
                                   the oscillation is usually denoted by σ . First, let us consider the case of zero
                                   mean stress and the applied stress varying between (+σ/2) and (−σ/2). A
                                   plot, (Fig. 7.8), of the stress difference σ versus log N , called an S − N –plot,
                                   shows the number of load cycles N before a specimen fails for a given σ .
Δσ
Δσe
0 log N
Figure 7.8 A plot of the stress amplitude versus number of cycles to failure for a typical metal.
                                   Most metals (notably, steel) show a threshold for σ called the endurance
                                   limit, σe , below which the specimen can withstand an unlimited number
                                   of cycles without failure. Above this threshold value, we see a linear range,
                                   which can be expressed as
                                   where (−k) is the slope of the S − N curve and σ1 is twice the failure stress in
                                   noncyclic loading.
                                     Typical aluminum alloys do not show an endurance limit.
                                                                Δσ
                                                                Δσ0
                                                                                              p
                                                                                              >
                                                                                                  1
                                                                                       p
                                                                                         =
                                                                                              1
                                                                                   p
                                                                                     <
                                                                                       1
σm /σu
Figure 7.9 The effect of mean stress on the effective stress amplitude according to the Goodman formula.
                                   the fatigue life of a specimen. If σu is the ultimate stress for failure, the Goodman
                                   diagram, shown in Fig. 7.9, shows
                                                                                σ      σm
                                                                                    =1−    ,                                            (7.29)
                                                                                σ0     σu
7.5 Creep
                                                                                   d
                                                                                      = Cσ n ,                 (7.32)
                                                                                   dt
                                   which is called the secondary creep. In the third stage, the strain, again, rapidly
                                   increases resulting in material failure. This stage is called the tertiary creep.
                                   All of the constants listed in the creep formulas are temperature dependent.
                                   Accurate calculation of creep deformation is crucial in applications involving
                                   high temperatures, such as turbine blades in a jet engine.
σ0
                                                                                     A            B     2b
                                                                                           2a
σ0
Figure 7.11 The three modes of loading affecting the crack tip stresses.
                                      Of course, every crack has two surfaces, like the upper and lower surfaces
                                   shown in the figure. In Mode I, the displacements on these surfaces are per-
                                   pendicular to the surfaces and in Mode II and Mode III they are parallel to the
                                   surfaces. As stated earlier, according to the linear elasticity solutions, some stress
                                   components at the tip of a crack may go to infinity. Using a polar coordinate
                                   system with its origin at the crack tip (see Fig. 7.12), the stress components and
                                   displacements very close to the crack tip (when r is small compared to the crack
                                   length) have been found using the theory of elasticity. These are listed in the
                                   following sections for the three modes of loading. The proportionality constants
                                   in these expressions, K I , K I I , and K I I I , are called the stress intensity factors,
                                   which depend on the shape of the body, length of the crack, and the nature of
                                   loading. When there is a single load P as shown in Fig. 7.11, the stress intensity
                                   factors are proportional to P.
                                                                                          y
                                                                                                       r
                                                                                                           θ
                                                                                              2a   x
                                   7.7.1 Mode I
                                                                                             
                                                                   KI      θ          θ    3θ
                                                         σx x   = √    cos     1 − sin sin      ,
                                                                   2πr     2          2     2
                                                                                             
                                                                   KI      θ          θ    3θ
                                                         σ yy   = √    cos     1 + sin sin      ,
                                                                   2πr     2          2     2
                                                                 KI      θ      θ     3θ
                                                         σx y = √    sin cos cos ,
                                                                 2πr     2      2      2
                                                                   *                                            
                                                                KI   r      θ                                  θ
                                                           u=           cos     1 − 2ν + sin2                      ,
                                                                G 2π        2                                  2
                                                                   *                                            
                                                                KI   r      θ                                  θ
                                                           v=           sin     2 − 2ν − cos2                      ,
                                                                G 2π        2                                  2
                                                           w = 0,        σzz = ν(σx x + σ yy ),            σx z = σ yz = 0.   (7.34)
                                                                              KI
                                                                      σ yy = √     , x > a,                                   (7.35)
                                                                              2πr
                                                                                 *
                                                                     2(1 − ν)K I    r
                                                                  v=                  , x < a.                                (7.36)
                                                                           G       2π
                                   An infinite panel with uniform tensile stress σ0 at infinity with a central crack of
                                   length 2a is shown in Fig. 7.13. For this geometry and loading, we have
                                                                              √
                                                                     K I = σ0 πa.                                (7.37)
                                   For a panel with finite width W , with the crack symmetrically located, the approx-
                                   imation
                                                                                √ +
                                                                        K I = σ0 πa sec(πa/W )                                (7.38)
is used.
σ0
2a
σ0
7.7.2 Mode II
                                                                                             
                                                                  KI I     θ          θ    3θ
                                                        σx x = − √     sin     2 + cos cos      ,
                                                                  2πr      2          2     2
                                                                KI I      θ      θ      3θ
                                                        σ yy = √      sin cos cos ,
                                                                 2πr      2      2       2
                                                                                              
                                                                KI I      θ            θ    3θ
                                                        σx y = √      cos      1 − sin sin       ,
                                                                 2πr      2            2     2
                                                                    *                             
                                                               KI I    r      θ                2 θ
                                                           u=             sin      2 − 2ν + cos      ,
                                                               G      2π      2                  2
                                                                    *                               
                                                               KI I    r       θ                   θ
                                                           v=             cos      −1 + 2ν + sin2      ,
                                                               G      2π       2                   2
                                                                                  KI I
                                                                          σx y = √     ,            x > a,                    (7.40)
                                                                                   2πr
                                                                                          *
                                                                        2(1 − ν)K I I           r
                                                                 u=                               ,     x < a.                (7.41)
                                                                             G                 2π
                                     For an infinite plate with a central crack of length 2a (shown in Fig. 7.14)
                                   under a shear stress τ0 , we have
                                                                                           √
                                                                                 K I I = τ0 πa.                               (7.42)
τ0
                                                                                                             τ0
                                                                                        2a
                                                                             KI I I    θ
                                                                    σx z = − √      sin ,
                                                                              2πr      2
                                                                           KI I I      θ
                                                                    σ yz = √       cos ,
                                                                            2πr        2
                                                                                  *
                                                                           KI I I    r    θ
                                                                     w=                sin ,
                                                                            G       2π    2
                                                                    σx y = 0,       σx x = σ yy = σzz = 0,
u=0 v = 0, σx y = 0. (7.43)
                                                                         KI I I
                                                                  σ yz = √      ,         σx z = 0,       x > a,             (7.44)
                                                                           2πr
                                                                                       *
                                                                           KI I I              r
                                                                        w=                       ,   x < a.                  (7.45)
                                                                            G                 2π
                                      All of the preceding expressions for Mode I and Mode II are applicable to
                                   the case of plane strain. By changing Poisson’s ratio ν to ν/(1 + ν), they can be
                                   converted for use in plane stress cases.
                                                               ∂U         ∂U
                                                                    ū +    a − Pū + 2γ a = 0.                                        (7.47)
                                                               ∂ ū       ∂a
                                                                         ∂U                   ∂U
                                                                              = P,               = −2γ t,                                  (7.48)
                                                                         ∂ ū                 ∂a
                                   where the first relation is Castigliano’s second theorem and the second is a
                                   condition to propagate the crack.
                                                                                        a              Δa
                                                                       (a)
σyy
                                                                       (b)
                                                                                        a + Δa             x
Figure 7.15 Stress in front of a crack of length a (a) and the displacement inside a crack of length a + a (b).
                                      Now, to find the rate of change in strain energy with respect to the crack length,
                                   we consider as an example Mode I loading and the state of stress in front of the
                                   original crack of length a and the displacement between x = a and x = a + a.
                                   These are sketched in Fig. 7.15. If we isolate the upper half above the crack and
                                   use a coordinate x starting from the old crack tip, before we had the tensile stress
                                   distribution
                                                                                     KI
                                                                             σ yy = √     ,         x > 0,                                 (7.49)
                                                                                     2π x
                                   between x = 0 and x = a. After the crack has extended, this stress has reduced
                                   to zero and a displacement distribution,
                                                                                                *
                                                                          2(1 − ν)K I               a − x
                                                                       v=                                  ,                               (7.50)
                                                                              G                      2π
                                   represents the opened crack. The transition from “before” to “after” can be viewed
                                   as decreasing the tensile stress to zero while this stress moves by the displacement
                                   v. The work done on the upper and lower half of the material is
                                                                     a
                                                                          1
                                                       U = −2              σ yy vtd x,
                                                                     0    2
                                                                                     √
                                                                  (1 − ν)K I2 a a − x
                                                            =−                          √      td x,
                                                                      2π G        0        x
                                                                                                          
                                                                                              
                                                               ∂U    (1 − ν)K I2                      1       1−x
                                                                  =−             t                                d x,   (7.51)
                                                               ∂a       2π G                      0            x
                                   where we have replaced x/a by x in the last line. Using x = sin2 θ,
                                                         
                                                      1                  π/2
                                                           1−x
                                                                dx = 2         cos2 θdθ = π.                             (7.52)
                                                       0     x            0
                                   Finally,
                                                                             (1 − ν)K I2
                                                                                 γ =     .                     (7.53)
                                                                                 4G
                                   This value of K I , which is responsible for extending the crack, is called the
                                                                                                         √
                                   critical stress intensity factor K I c , which has the dimension of Pa m as can be
                                   verified from the stress expressions. As the applied load P is increased from 0,
                                   there comes a point when K I reaches the critical value K I c and the crack begins
                                   to propagate.
                                                                                              2Gγ
                                                                                  K I2c =         .                      (7.54)
                                                                                              1−ν
                                       Using the energy method we also get
                                                                                 4Gγ
                                                                     K I2I c =       ,         K I2I I c = 4Gγ .         (7.55)
                                                                                 1−ν
                                   When the loading is such that all the three modes are present, by computing
                                                           a
                                                               (σ yy v + σx y u + σ yz w)td x,               (7.56)
                                                                       0
                                   we find
                                                                                     
                                                                  (1 − ν) K I2 + K I2I + K I2I I = 4Gγ .                 (7.57)
                                   The total energy dissipated by creating new surfaces is also known as the energy
                                   release rate. They are denoted by G I , G I I , and G I I I for the three modes. By
                                   multiplying 2γ t by the number of active (where the crack tip is moving) crack tips,
                                   we can find the energy release rate. The energy used for creating the new surfaces
                                   can be regained, in principle, by exerting pressure and by waiting for diffusive
                                   healing of the crack in time. For all practical purposes, the term “dissipated
                                   energy” aptly describes the energy spent in creating the surfaces during the crack
                                   tip motion.
                                                                                 a
                                                                            P
                                     Fig. 7.16 shows a split cantilever beam with Mode I loading. For the loading
                                   shown, the deflection ū of the tip is given by
                                                                  Pa 3          3E I ū
                                                                       , P=
                                                                         ū =           ,                   (7.58)
                                                                  3E I            a3
                                   where I is the second moment of area for one of the beams. The energy stored in
                                   the upper and lower beams totals to
                                                                                              3E I ū 2
                                                                             U = P ū =                 .         (7.59)
                                                                                                a3
                                   Using the energy release rate
                                                                  2(1 − ν)t K I2    ∂U   9E I ū 2   P 2a2
                                                        2γ t =                   =−    =           =       .      (7.60)
                                                                       G            ∂a     a4         EI
                                                                                              Pa
                                                                            KI = +                          .     (7.61)
                                                                                         4(1 − ν 2 )t I
                                   boundaries where crystals with different orientations meet. When these materi-
                                   als are subjected to oscillating loads, the defects could move and coalesce into
                                   microscopic cracks. It takes a number cycles of loading for this microcracks to
                                   grow into visible range. If we denote by a0 the minimum size detectable, we can
                                   predict their further growth using a relation advanced by Paris:
                                                                                da
                                                                                   = C(K )m ,                    (7.63)
                                                                                dN
                                   where C and m are material constants and
                                                                             K = K max − K min .                 (7.64)
                                   Experimental data are often presented in a log–log plot to obtain the constants.
                                                                            √
                                   As an example, with K in the units of MPa m and da/d N in m/cycle, austenitic
                                   steel has C = 5.6 × 10−12 and m = 3.25.
                                   FURTHER READING
                                   Anderson, T. L., Fracture Mechanics: Fundamentals and Applications, CRC
                                   Press (1995).
                                   Bannantine, J., Comer, J., and Handrock, J., Fundamentals of Metal Fatigue
                                   Analysis, Prentice Hall (1990).
                                   Cherepanov, G. P., Mechanics of Brittle Fracture, McGraw-Hill (1979).
                                   Jones, R. M., Mechanics of Composite Materials, McGraw-Hill (1975).
                                   Lubliner, J., Plasticity Theory, Macmillan (1990).
                                   Suresh, S., Fatigue of Materials, Cambridge University Press (1998).
                                   EXERCISES
                                     7.1 A brittle material fails at 80 MPa in a uni-axial test. A plate made of
                                         this material is subjected to a bi-axial tension in the x, y-plane with the
                                         proportional loading σx x = 2α and σ yy = α with α being a load control
                                         parameter. Obtain the value of α at failure, (a) if the material fails according
                                         to the maximum stress criterion, and (b) if it fails under the maximum strain
                                         criterion. Assume the Poisson’s ratio is 1/3.
                                     7.2 The yield stress for a steel alloy is 1.5 GPa. Obtain the internal pressure in
                                         a thin-walled cylindrical pressure vessel with radius 1 m and thickness 0.2
                                         cm for yielding to occur if (a) Tresca yield criterion is used and (b) von
                                         Mises criterion is used.
                                     7.3 A shaft of radius 5 cm carries a torque of 100 Nm and a bending moment
                                         of 50 Nm. Obtain the maximum shear stress and the maximum Mises stress
                                         in the shaft.
                                     7.4 A circular cross-section fuselage is idealized as a thin-walled shell of radius
                                         4 m with 48 booms of radius 2 cm each. The booms are distributed uniformly
                                         around with the first and the 25th booms being located the farthest from the
                                         neutral axis. If the maximum allowable compressive stress in the booms is
                                         1 GPa, what is the allowable bending moment for this structure?