Problems for Chapter 5

 

Analytical Techniques and Solutions for Linear Elastic Solids

 

 

 

5.8.  Energy Methods

 

 

 

5.8.1.      A planet that deforms under its own gravitational force can be idealized as a linear elastic sphere with radius a, Young’s modulus E and Poisson’s ratio ν MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rk0le9 v8qqaqFD0xXdHaVhbbf9v8qqaqFr0xc9pk0xbba9q8WqFfea0=yr0R Yxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9Fve9Ff0dmeaabaqaciGa caGaaeqabaGadeaadaaakeaacqaH9oGBaaa@347E@  that is subjected to a radial gravitational force b=(gR/a) e R MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rk0le9 v8qqaqFD0xXdHaVhbbf9v8qqaqFr0xc9pk0xbba9q8WqFfea0=yr0R Yxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9Fve9Ff0dmeaabaqaciGa caGaaeqabaGadeaadaaakeaacaWHIbGaeyypa0JaeyOeI0Iaaiikai aadEgacaaMc8UaamOuaiaac+cacaWGHbGaaiykaiaahwgadaWgaaWc baGaamOuaaqabaaaaa@3DD5@ , where g is the acceleration due to gravity at the surface of the sphere, and R is the radial coordinate. Use the reciprocal theorem, together with a hydrostatic stress distribution σ ij =p δ ij MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiabeo8aZnaaBaaaleaacaWGPbGaamOAaa qabaGccqGH9aqpcaWGWbGaeqiTdq2aaSbaaSqaaiaadMgacaWGQbaa beaaaaa@39E7@  as the reference solution, to calculate the change in volume of the sphere, and hence deduce the radial displacement of its surface.

 

 

 

 

5.8.2.      Consider an isotropic, linear elastic solid with Young’s modulus E, mass density ρ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rk0le9 v8qqaqFD0xXdHaVhbbf9v8qqaqFr0xc9pk0xbba9q8WqFfea0=yr0R Yxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9Fve9Ff0dmeaabaqaciGa caGaaeqabaGadeaadaaakeaacqaHbpGCaaa@3486@ , and Poisson’s ratio ν MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rk0le9 v8qqaqFD0xXdHaVhbbf9v8qqaqFr0xc9pk0xbba9q8WqFfea0=yr0R Yxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9Fve9Ff0dmeaabaqaciGa caGaaeqabaGadeaadaaakeaacqaH9oGBaaa@347E@ , which is subjected to a body force distribution b i MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rk0le9 v8qqaqFD0xXdHaVhbbf9v8qqaqFr0xc9pk0xbba9q8WqFfea0=yr0R Yxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9Fve9Ff0dmeaabaqaciGa caGaaeqabaGadeaadaaakeaacaWGIbWaaSbaaSqaaiaadMgaaeqaaa aa@34C7@  per unit mass, and tractions t i MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rk0le9 v8qqaqFD0xXdHaVhbbf9v8qqaqFr0xc9pk0xbba9q8WqFfea0=yr0R Yxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9Fve9Ff0dmeaabaqaciGa caGaaeqabaGadeaadaaakeaacaWG0bWaaSbaaSqaaiaadMgaaeqaaa aa@34D9@  on its exterior surface.   By using the reciprocal theorem, together with a state of uniform stress σ ij * MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rk0le9 v8qqaqFD0xXdHaVhbbf9v8qqaqFr0xc9pk0xbba9q8WqFfea0=yr0R Yxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9Fve9Ff0dmeaabaqaciGa caGaaeqabaGadeaadaaakeaacqaHdpWCdaqhaaWcbaGaamyAaiaadQ gaaeaacaGGQaaaaaaa@3741@  as the reference solution, show that the average strains in the solid can be calculated from

1 V V ε ij dV = 1+ν EV A x j t i dA ν EV A δ ij x k t k dA + 1+ν EV V x j ρ b i dV ν EV V δ ij x k ρ b k dV MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rk0le9 v8qqaqFD0xXdHaVhbbf9v8qqaqFr0xc9pk0xbba9q8WqFfea0=yr0R Yxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9Fve9Ff0dmeaabaqaciGa caGaaeqabaGadeaadaaakeaadaWcaaqaaiaaigdaaeaacaWGwbaaam aapefabaGaeqyTdu2aaSbaaSqaaiaadMgacaWGQbaabeaakiaadsga caWGwbaaleaacaWGwbaabeqdcqGHRiI8aOGaeyypa0ZaaSaaaeaaca aIXaGaey4kaSIaeqyVd4gabaGaamyraiaadAfaaaWaa8quaeaacaWG 4bWaaSbaaSqaaiaadQgaaeqaaOGaamiDamaaBaaaleaacaWGPbaabe aakiaadsgacaWGbbGaeyOeI0caleaacaWGbbaabeqdcqGHRiI8aOWa aSaaaeaacqaH9oGBaeaacaWGfbGaamOvaaaadaWdrbqaaiabes7aKn aaBaaaleaacaWGPbGaamOAaaqabaGccaWG4bWaaSbaaSqaaiaadUga aeqaaOGaamiDamaaBaaaleaacaWGRbaabeaakiaadsgacaWGbbaale aacaWGbbaabeqdcqGHRiI8aOGaey4kaSYaaSaaaeaacaaIXaGaey4k aSIaeqyVd4gabaGaamyraiaadAfaaaWaa8quaeaacaWG4bWaaSbaaS qaaiaadQgaaeqaaOGaeqyWdiNaamOyamaaBaaaleaacaWGPbaabeaa kiaadsgacaWGwbGaeyOeI0caleaacaWGwbaabeqdcqGHRiI8aOWaaS aaaeaacqaH9oGBaeaacaWGfbGaamOvaaaadaWdrbqaaiabes7aKnaa BaaaleaacaWGPbGaamOAaaqabaGccaWG4bWaaSbaaSqaaiaadUgaae qaaOGaeqyWdiNaamOyamaaBaaaleaacaWGRbaabeaakiaadsgacaWG wbaaleaacaWGwbaabeqdcqGHRiI8aaaa@8105@

 

 

 

 

5.8.3.      A cylinder with arbitrary cross-section rests on a flat surface, and is subjected to a vertical gravitational body force b=ρg e 3 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rk0le9 v8qqaqFD0xXdHaVhbbf9v8qqaqFr0xc9pk0xbba9q8WqFfea0=yr0R Yxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9Fve9Ff0dmeaabaqaciGa caGaaeqabaGadeaadaaakeaacaWHIbGaeyypa0JaeyOeI0IaeqyWdi Naam4zaiaahwgadaWgaaWcbaGaaG4maaqabaaaaa@3A27@ , where e 3 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rk0le9 v8qqaqFD0xXdHaVhbbf9v8qqaqFr0xc9pk0xbba9q8WqFfea0=yr0R Yxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9Fve9Ff0dmeaabaqaciGa caGaaeqabaGadeaadaaakeaacaWHLbWaaSbaaSqaaiaaiodaaeqaaa aa@349D@  is a unit vector normal to the surface. The cylinder is a linear elastic solid with Young’s modulus E, mass density ρ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rk0le9 v8qqaqFD0xXdHaVhbbf9v8qqaqFr0xc9pk0xbba9q8WqFfea0=yr0R Yxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9Fve9Ff0dmeaabaqaciGa caGaaeqabaGadeaadaaakeaacqaHbpGCaaa@3486@ , and Poisson’s ratio ν MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rk0le9 v8qqaqFD0xXdHaVhbbf9v8qqaqFr0xc9pk0xbba9q8WqFfea0=yr0R Yxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9Fve9Ff0dmeaabaqaciGa caGaaeqabaGadeaadaaakeaacqaH9oGBaaa@347E@ . Define the change in length of the cylinder as

δL= 1 A A u 3 ( x 1 , x 2 ,L)dA MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rk0le9 v8qqaqFD0xXdHaVhbbf9v8qqaqFr0xc9pk0xbba9q8WqFfea0=yr0R Yxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9Fve9Ff0dmeaabaqaciGa caGaaeqabaGadeaadaaakeaacqaH0oazcaWGmbGaeyypa0ZaaSaaae aacaaIXaaabaGaamyqaaaadaWdrbqaaiaadwhadaWgaaWcbaGaaG4m aaqabaGccaGGOaGaamiEamaaBaaaleaacaaIXaaabeaakiaacYcaca WG4bWaaSbaaSqaaiaaikdaaeqaaOGaaiilaiaadYeacaGGPaGaamiz aiaadgeaaSqaaiaadgeaaeqaniabgUIiYdaaaa@45E6@

where u 3 ( x 1 , x 2 ,L) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rk0le9 v8qqaqFD0xXdHaVhbbf9v8qqaqFr0xc9pk0xbba9q8WqFfea0=yr0R Yxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9Fve9Ff0dmeaabaqaciGa caGaaeqabaGadeaadaaakeaacaWG1bWaaSbaaSqaaiaaiodaaeqaaO GaaiikaiaadIhadaWgaaWcbaGaaGymaaqabaGccaGGSaGaamiEamaa BaaaleaacaaIYaaabeaakiaacYcacaWGmbGaaiykaaaa@3C1A@  denotes the displacement of the end x 3 =L MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rk0le9 v8qqaqFD0xXdHaVhbbf9v8qqaqFr0xc9pk0xbba9q8WqFfea0=yr0R Yxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9Fve9Ff0dmeaabaqaciGa caGaaeqabaGadeaadaaakeaacaWG4bWaaSbaaSqaaiaaiodaaeqaaO Gaeyypa0Jaamitaaaa@368D@  of the cylinder.  Show that δL=W/2EA MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rk0le9 v8qqaqFD0xXdHaVhbbf9v8qqaqFr0xc9pk0xbba9q8WqFfea0=yr0R Yxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9Fve9Ff0dmeaabaqaciGa caGaaeqabaGadeaadaaakeaacqaH0oazcaWGmbGaeyypa0Jaam4vai aac+cacaaIYaGaamyraiaadgeaaaa@3A1D@ , where W is the weight of the cylinder, and A its cross-sectional area.

 

 

 

 

5.8.4.      In this problem, you will calculate an expression for the change in potential energy that occurs when an inelastic strain ε ij T MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiabew7aLnaaDaaaleaacaWGPbGaamOAaa qaaiaadsfaaaaaaa@34F2@  is introduced into some part B of an elastic solid.  The inelastic strain can be visualized as a generalized version of the Eshelby inclusion problem MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiFKI8=feu0dXdh9vqqj=hEeeu0xXdbba9frFj0=OqFf ea0dXdd9vqaq=JfrVkFHe9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr 0=vqpWqaaeaabiGaciaacaqabeaadaqaaqaaaOqaaGqaaKqzGfaeaa aaaaaaa8qacaWFtacaaa@37E6@  it could occur as a result of thermal expansion, a phase transformation in the solid, or plastic flow.   Note that B need not be ellipsoidal.

 

The figure illustrates the solid of interest.  Assume that:

The solid has elastic constants C ijkl MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiaadoeadaWgaaWcbaGaamyAaiaadQgaca WGRbGaamiBaaqabaaaaa@351A@

No body forces act on the solid (for simplicity)

Part of the surface of the solid S 1 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiaadofadaWgaaWcbaGaaGymaaqabaaaaa@3227@  is subjected to a prescribed displacement u i * MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiaadwhadaqhaaWcbaGaamyAaaqaaiaacQ caaaaaaa@332B@

The remainder of the surface of the solid  S 2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiaadofadaWgaaWcbaGaaGOmaaqabaaaaa@3228@  is subjected to a prescribed traction t i * MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiaadshadaqhaaWcbaGaamyAaaqaaiaacQ caaaaaaa@332A@

Let u i 0 , ε ij 0 , σ ij 0 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiaadwhadaqhaaWcbaGaamyAaaqaaiaaic daaaGccaGGSaGaeqyTdu2aa0baaSqaaiaadMgacaWGQbaabaGaaGim aaaakiaacYcacqaHdpWCdaqhaaWcbaGaamyAaiaadQgaaeaacaaIWa aaaaaa@3D9D@  denote the displacement, strain, and stress in the solid before the inelastic strain is introduced.  Let V 0 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiaadAfadaWgaaWcbaGaaGimaaqabaaaaa@3229@  denote the potential energy of the solid in this state.

Next, suppose that some external process introduces an inelastic strain ε ij T MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiabew7aLnaaDaaaleaacaWGPbGaamOAaa qaaiaadsfaaaaaaa@34F2@  into part of the solid. Let Δ u i ,Δ ε ij ,Δ σ ij MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiabfs5aejaadwhadaWgaaWcbaGaamyAaa qabaGccaGGSaGaeuiLdqKaeqyTdu2aaSbaaSqaaiaadMgacaWGQbaa beaakiaacYcacqqHuoarcqaHdpWCdaWgaaWcbaGaamyAaiaadQgaae qaaaaa@3F9E@  denote the change in stress in the solid resulting from the inelastic strain.  Note that these fields satisfy

The strain-displacement relation Δ ε ij =(Δ u i / x j +Δ u i / x j )/2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiabfs5aejabew7aLnaaBaaaleaacaWGPb GaamOAaaqabaGccqGH9aqpcaGGOaGaeyOaIyRaeuiLdqKaamyDamaa BaaaleaacaWGPbaabeaakiaac+cacqGHciITcaWG4bWaaSbaaSqaai aadQgaaeqaaOGaey4kaSIaeyOaIyRaeuiLdqKaamyDamaaBaaaleaa caWGPbaabeaakiaac+cacqGHciITcaWG4bWaaSbaaSqaaiaadQgaae qaaOGaaiykaiaac+cacaaIYaaaaa@4C82@

The stress-strain law  Δ σ ij = C ijkl (Δ ε kl ε kl T ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiabfs5aejabeo8aZnaaBaaaleaacaWGPb GaamOAaaqabaGccqGH9aqpcaWGdbWaaSbaaSqaaiaadMgacaWGQbGa am4AaiaadYgaaeqaaOGaaiikaiabfs5aejabew7aLnaaBaaaleaaca WGRbGaamiBaaqabaGccqGHsislcqaH1oqzdaqhaaWcbaGaam4Aaiaa dYgaaeaacaWGubaaaOGaaiykaaaa@4768@  in B, and Δ σ ij = C ijkl Δ ε kl MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiabfs5aejabeo8aZnaaBaaaleaacaWGPb GaamOAaaqabaGccqGH9aqpcaWGdbWaaSbaaSqaaiaadMgacaWGQbGa am4AaiaadYgaaeqaaOGaeuiLdqKaeqyTdu2aaSbaaSqaaiaadUgaca WGSbaabeaaaaa@4080@  outside B

 Boundary conditions Δ u i =0 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiabfs5aejaadwhadaWgaaWcbaGaamyAaa qabaGccqGH9aqpcaaIWaaaaa@35AC@  on S 1 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiaadofadaWgaaWcbaGaaGymaaqabaaaaa@3227@ , and Δ σ ij n j =0 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiabfs5aejabeo8aZnaaBaaaleaacaWGPb GaamOAaaqabaGccaWGUbWaaSbaaSqaaiaadQgaaeqaaOGaeyypa0Ja aGimaaaa@397C@  on S 2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiaadofadaWgaaWcbaGaaGOmaaqabaaaaa@3228@

 

5.8.4.1.            Write down an expressions for V 0 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiaadAfadaWgaaWcbaGaaGimaaqabaaaaa@3229@  in terms of u i 0 , ε ij 0 , σ ij 0 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiaadwhadaqhaaWcbaGaamyAaaqaaiaaic daaaGccaGGSaGaeqyTdu2aa0baaSqaaiaadMgacaWGQbaabaGaaGim aaaakiaacYcacqaHdpWCdaqhaaWcbaGaamyAaiaadQgaaeaacaaIWa aaaaaa@3D9D@

 

5.8.4.2.            Suppose that u i 0 , ε ij 0 , σ ij 0 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiaadwhadaqhaaWcbaGaamyAaaqaaiaaic daaaGccaGGSaGaeqyTdu2aa0baaSqaaiaadMgacaWGQbaabaGaaGim aaaakiaacYcacqaHdpWCdaqhaaWcbaGaamyAaiaadQgaaeaacaaIWa aaaaaa@3D9D@  are all zero (i.e. the solid is initially stress free).  Write down the potential energy V S MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiaadAfadaWgaaWcbaGaam4uaaqabaaaaa@3247@  due to Δ u i ,Δ ε ij ,Δ σ ij MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiabfs5aejaadwhadaWgaaWcbaGaamyAaa qabaGccaGGSaGaeuiLdqKaeqyTdu2aaSbaaSqaaiaadMgacaWGQbaa beaakiaacYcacqqHuoarcqaHdpWCdaWgaaWcbaGaamyAaiaadQgaae qaaaaa@3F9E@ .  This is called the “self energy” of the eigenstrain MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiFKI8=feu0dXdh9vqqj=hEeeu0xXdbba9frFj0=OqFf ea0dXdd9vqaq=JfrVkFHe9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr 0=vqpWqaaeaabiGaciaacaqabeaadaqaaqaaaOqaaGqaaKqzGfaeaa aaaaaaa8qacaWFtacaaa@37E6@  the energy cost of  introducing the eigenstrain ε ij T MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiabew7aLnaaDaaaleaacaWGPbGaamOAaa qaaiaadsfaaaaaaa@34F2@  into a stress-free solid.

 

5.8.4.3.            Show that the expression for the self-energy can be simplified to

V S = 1 2 B Δ σ ij ε ij T dV MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiaadAfadaWgaaWcbaGaam4uaaqabaGccq GH9aqpcqGHsisldaWcaaqaaiaaigdaaeaacaaIYaaaamaapefabaGa euiLdqKaeq4Wdm3aaSbaaSqaaiaadMgacaWGQbaabeaakiabew7aLn aaDaaaleaacaWGPbGaamOAaaqaaiaadsfaaaGccaWGKbGaamOvaaWc baGaamOqaaqab0Gaey4kIipaaaa@4470@

 

5.8.4.4.            Now suppose that u i 0 , ε ij 0 , σ ij 0 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiaadwhadaqhaaWcbaGaamyAaaqaaiaaic daaaGccaGGSaGaeqyTdu2aa0baaSqaaiaadMgacaWGQbaabaGaaGim aaaakiaacYcacqaHdpWCdaqhaaWcbaGaamyAaiaadQgaaeaacaaIWa aaaaaa@3D9D@  are all nonzero.  Write down the total potential energy of the system V TOT MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiaadAfadaWgaaWcbaGaamivaiaad+eaca WGubaabeaaaaa@33F5@ , in terms of u i 0 , ε ij 0 , σ ij 0 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiaadwhadaqhaaWcbaGaamyAaaqaaiaaic daaaGccaGGSaGaeqyTdu2aa0baaSqaaiaadMgacaWGQbaabaGaaGim aaaakiaacYcacqaHdpWCdaqhaaWcbaGaamyAaiaadQgaaeaacaaIWa aaaaaa@3D9D@  and Δ u i ,Δ ε ij ,Δ σ ij MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiabfs5aejaadwhadaWgaaWcbaGaamyAaa qabaGccaGGSaGaeuiLdqKaeqyTdu2aaSbaaSqaaiaadMgacaWGQbaa beaakiaacYcacqqHuoarcqaHdpWCdaWgaaWcbaGaamyAaiaadQgaae qaaaaa@3F9E@ .

 

5.8.4.5.            Finally, show that the total potential energy of the system can be expressed as

V TOT = V 0 + V S B σ ij 0 ε ij T dV MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiaadAfadaWgaaWcbaGaamivaiaad+eaca WGubaabeaakiabg2da9iaadAfadaWgaaWcbaGaaGimaaqabaGccqGH RaWkcaWGwbWaaSbaaSqaaiaadofaaeqaaOGaeyOeI0Yaa8quaeaacq aHdpWCdaqhaaWcbaGaamyAaiaadQgaaeaacaaIWaaaaOGaeqyTdu2a a0baaSqaaiaadMgacaWGQbaabaGaamivaaaakiaadsgacaWGwbaale aacaWGcbaabeqdcqGHRiI8aaaa@4882@

Here, the last term is called the “interaction energy” of the eigenstrain with the applied load. The steps in this derivation are very similar to the derivation of the reciprocal theorem.

 

 

 

 

5.8.5.      An infinite, isotropic, linear elastic solid with Young’s modulus E and Poisson’s ratio ν MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiabe27aUbaa@3220@  is subjected to a uniaxial tensile stress σ 0 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiabeo8aZnaaBaaaleaacaaIWaaabeaaaa a@3311@ .  As a result of a phase transformation, a uniform dilatational strain ε ij T =β δ ij MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiabew7aLnaaDaaaleaacaWGPbGaamOAaa qaaiaadsfaaaGccqGH9aqpcqaHYoGycqaH0oazdaWgaaWcbaGaamyA aiaadQgaaeqaaaaa@3B51@  is then induced in a spherical region of the solid with radius a

5.8.5.1.            Using the solution to problem 1, and the Eshelby solution, find an expression for the change in potential energy of the solid, in terms of β, σ 0 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiabek7aIjaacYcacqaHdpWCdaWgaaWcba GaaGimaaqabaaaaa@3562@  and relevant geometric and material parameters.

5.8.5.2.            Assume that the interface between the transformed material an the matrix has an energy per unit area γ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaebbnrfifHhDYfgasaacH8rkY=vi pgYlH8Gipec8Eeeu0xXdbba9frFj0=OqFfea0dXdd9vqaq=JfrVkFH e9pgea0dXdar=Jb9hs0dXdbPYxe9vr0=vr0=vqpWqaaeaabiGaciaa caqabeaacmqaamaaaOqaaiabeo7aNbaa@320F@ .  Find an expression for the critical stress at which the total energy of the system (elastic potential energy + interface energy) is decreased as a result of the transformation