1 00:00:00,040 --> 00:00:02,470 The following content is provided under a Creative 2 00:00:02,470 --> 00:00:03,880 Commons license. 3 00:00:03,880 --> 00:00:06,920 Your support will help MIT OpenCourseWare continue to 4 00:00:06,920 --> 00:00:10,570 offer high quality educational resources for free. 5 00:00:10,570 --> 00:00:13,470 To make a donation or view additional materials from 6 00:00:13,470 --> 00:00:17,400 hundreds of MIT courses, visit MIT OpenCourseWare at 7 00:00:17,400 --> 00:00:18,650 ocw.mit.edu. 8 00:00:22,240 --> 00:00:23,850 PROFESSOR: Ladies and gentlemen, welcome to this 9 00:00:23,850 --> 00:00:26,370 lecture on Nonlinear Finite Element Analysis of Solids and 10 00:00:26,370 --> 00:00:27,700 Structures. 11 00:00:27,700 --> 00:00:29,770 In the previous lectures, we discussed quite general 12 00:00:29,770 --> 00:00:33,220 kinematic formulations and numerical algorithms that we 13 00:00:33,220 --> 00:00:36,210 use for nonlinear finite element analysis. 14 00:00:36,210 --> 00:00:40,610 We also referred to and used a stress strain matrix C, but we 15 00:00:40,610 --> 00:00:43,580 did not discuss this matrix in any depths. 16 00:00:43,580 --> 00:00:45,990 This is the topic of this lecture and 17 00:00:45,990 --> 00:00:48,420 the following lectures. 18 00:00:48,420 --> 00:00:52,340 The stress strain matrix C is used in the calculation of the 19 00:00:52,340 --> 00:00:56,180 K matrix, and is schematically shown on this graph. 20 00:00:56,180 --> 00:00:58,730 And of course, the stress strain matrix is also used in 21 00:00:58,730 --> 00:01:04,069 the evaluation of the force vector F, as shown here. 22 00:01:04,069 --> 00:01:06,510 The stress strain matrix, of course, will be different for 23 00:01:06,510 --> 00:01:08,180 different material behaviors. 24 00:01:08,180 --> 00:01:09,980 It will be different for different kinematic 25 00:01:09,980 --> 00:01:11,500 formulations that we're using. 26 00:01:11,500 --> 00:01:15,260 And all these aspects we now have to discuss in this and 27 00:01:15,260 --> 00:01:17,650 the following lectures. 28 00:01:17,650 --> 00:01:23,680 We notice that when we do finite element analysis, we 29 00:01:23,680 --> 00:01:26,540 have the choice of different kinds of formulations. 30 00:01:26,540 --> 00:01:30,160 And we talked about the formulation that takes only 31 00:01:30,160 --> 00:01:33,030 into account infinitesimally small displacements. 32 00:01:33,030 --> 00:01:35,920 But of course, material nonlinear behavior, we 33 00:01:35,920 --> 00:01:38,870 actually call that formation a materially nonlinear only 34 00:01:38,870 --> 00:01:41,770 formation, an MNO formulation. 35 00:01:41,770 --> 00:01:44,720 We may have or use a formulation that takes into 36 00:01:44,720 --> 00:01:48,580 account large displacements, large rotations, but only 37 00:01:48,580 --> 00:01:51,350 small strains. 38 00:01:51,350 --> 00:01:55,320 This, for example, would be a total Lagrangian formulation. 39 00:01:55,320 --> 00:02:00,290 And we have also formulations that take into account large 40 00:02:00,290 --> 00:02:03,200 displacements, large locations, and large strains. 41 00:02:03,200 --> 00:02:06,170 And here we use, once again, the total Lagrangian 42 00:02:06,170 --> 00:02:09,750 formulation or an updated Lagrangian formulation. 43 00:02:09,750 --> 00:02:12,020 We discussed these formulations, of course, 44 00:02:12,020 --> 00:02:14,610 earlier in the earlier lectures. 45 00:02:14,610 --> 00:02:18,350 The applicability of material descriptions is also very well 46 00:02:18,350 --> 00:02:21,830 categorized in these three categories. 47 00:02:21,830 --> 00:02:24,400 In other words, there are certain material description 48 00:02:24,400 --> 00:02:28,000 constitutive relations that hold for infinitesimally small 49 00:02:28,000 --> 00:02:31,560 displacements and small strains, and that are not 50 00:02:31,560 --> 00:02:35,020 directly applicable to large strains. 51 00:02:35,020 --> 00:02:37,430 If, however, we have a material description that is 52 00:02:37,430 --> 00:02:41,240 applicable to infinitesimally small displacements and small 53 00:02:41,240 --> 00:02:45,050 strains, then we will see that same material description can 54 00:02:45,050 --> 00:02:48,250 directly be used also in the large displacement, large 55 00:02:48,250 --> 00:02:52,520 rotation, but small strain analysis, provided we use the 56 00:02:52,520 --> 00:02:53,920 proper formulation. 57 00:02:53,920 --> 00:02:56,970 We will discuss this aspect just now. 58 00:02:56,970 --> 00:03:00,740 In fact, the formulation that we are using in this category 59 00:03:00,740 --> 00:03:05,330 of problems is a total Lagrangian formulation. 60 00:03:05,330 --> 00:03:10,010 Let us very briefly once more recall that we have the 61 00:03:10,010 --> 00:03:11,790 materially-nonlinear-only formulation, as I just 62 00:03:11,790 --> 00:03:14,580 mentioned, the total Lagrangian formulation and the 63 00:03:14,580 --> 00:03:16,570 updated Lagrangian formulation, which we 64 00:03:16,570 --> 00:03:20,120 discussed in earlier lectures. 65 00:03:20,120 --> 00:03:25,960 And that really kinematically, these formulations here 66 00:03:25,960 --> 00:03:29,120 kinematically, for the analysis of two dimensional, 67 00:03:29,120 --> 00:03:32,150 three dimensional solids, using isoparametric finite 68 00:03:32,150 --> 00:03:36,690 element formations, we include all large displacement, large 69 00:03:36,690 --> 00:03:39,380 rotation, and large strain effects. 70 00:03:39,380 --> 00:03:42,730 Of course, whether the formulation will actually be 71 00:03:42,730 --> 00:03:47,550 applicable to model a particular problem, will also 72 00:03:47,550 --> 00:03:51,680 depends on whether we use and have the right constitutive 73 00:03:51,680 --> 00:03:53,450 relation for that problem. 74 00:03:53,450 --> 00:03:56,460 And that is an aspect that we will concentrate on now in 75 00:03:56,460 --> 00:03:58,480 this and the following lectures. 76 00:03:58,480 --> 00:04:02,530 But notice that kinematically these formations include all 77 00:04:02,530 --> 00:04:03,780 nonlinearities. 78 00:04:05,920 --> 00:04:10,780 If we look very briefly at various material descriptions, 79 00:04:10,780 --> 00:04:15,340 we have here typical models that I used and examples of 80 00:04:15,340 --> 00:04:20,529 applications, materials, practically all materials 81 00:04:20,529 --> 00:04:24,370 behave elastically as long as the stress and the strains are 82 00:04:24,370 --> 00:04:26,348 small enough. 83 00:04:26,348 --> 00:04:28,620 A hyperelastic material would be, for 84 00:04:28,620 --> 00:04:30,696 example, a rubber material. 85 00:04:30,696 --> 00:04:33,540 A hypoelastic material would be the 86 00:04:33,540 --> 00:04:36,780 concrete material model. 87 00:04:36,780 --> 00:04:40,870 And elasto-plastic material would be applicable to model 88 00:04:40,870 --> 00:04:44,900 metals, soils, rocks under high stresses. 89 00:04:44,900 --> 00:04:48,800 A creep material model would be applicable to model metals 90 00:04:48,800 --> 00:04:50,430 at high temperatures. 91 00:04:50,430 --> 00:04:54,820 When the temperatures are high, then metals are 92 00:04:54,820 --> 00:04:57,110 subjected very easily to creep. 93 00:04:57,110 --> 00:05:01,070 A viscoplastic material model really takes into account the 94 00:05:01,070 --> 00:05:03,670 elasto-plasticity and the creeping effect of the 95 00:05:03,670 --> 00:05:08,720 material and is used frequently to idealize or to 96 00:05:08,720 --> 00:05:12,280 represent polymers and metals. 97 00:05:12,280 --> 00:05:16,140 We will talk about a number of these material models in this 98 00:05:16,140 --> 00:05:17,660 and the following lecture. 99 00:05:17,660 --> 00:05:23,670 We will not go into depths of concrete material models and 100 00:05:23,670 --> 00:05:27,130 rock material models, but still whatever we are talking 101 00:05:27,130 --> 00:05:32,770 about is applicable to a wide range of material models. 102 00:05:32,770 --> 00:05:36,130 Let us first look now, in this lecture, at the elastic 103 00:05:36,130 --> 00:05:39,120 material behavior. 104 00:05:39,120 --> 00:05:44,250 Elasticity means that for a particular strain, you are 105 00:05:44,250 --> 00:05:46,710 given a particular stress. 106 00:05:46,710 --> 00:05:50,010 The history does not enter in the solution. 107 00:05:50,010 --> 00:05:51,770 And a linear elastic stress strain 108 00:05:51,770 --> 00:05:54,380 relationship is shown here. 109 00:05:54,380 --> 00:06:00,450 Notice for the strain, tE, we are given a stress t sigma. 110 00:06:00,450 --> 00:06:02,320 And it's a unique stress. 111 00:06:02,320 --> 00:06:03,840 It is a unique stress. 112 00:06:03,840 --> 00:06:06,520 And of course, the history of the formation does 113 00:06:06,520 --> 00:06:08,920 not enter at all. 114 00:06:08,920 --> 00:06:13,010 Notice that in this particular case, we would have that 115 00:06:13,010 --> 00:06:20,126 typically t sigma here is equal to E times te. 116 00:06:20,126 --> 00:06:24,340 te being of course this value here, t sigma there. 117 00:06:24,340 --> 00:06:27,430 Notice that an increment in stress is given by d sigma 118 00:06:27,430 --> 00:06:29,370 equal to E times de. 119 00:06:29,370 --> 00:06:33,260 Linear elasticity, a linear elastic material description, 120 00:06:33,260 --> 00:06:34,695 means E is constant. 121 00:06:38,200 --> 00:06:42,880 For nonlinear, as a nonlinear elastic material description, 122 00:06:42,880 --> 00:06:46,600 we might have schematically in a one-dimensional analysis, 123 00:06:46,600 --> 00:06:49,440 this relationship here, the red curve. 124 00:06:49,440 --> 00:06:54,560 Notice that, once again, for a particular strain, we pick up 125 00:06:54,560 --> 00:06:57,660 a unique value of stress. 126 00:06:57,660 --> 00:07:03,420 And this relationship here shows that t sigma is 127 00:07:03,420 --> 00:07:05,804 given tC times te. 128 00:07:05,804 --> 00:07:10,320 tC is the slope of this line here. 129 00:07:10,320 --> 00:07:15,020 Now, an increment in stress is obtained by this 130 00:07:15,020 --> 00:07:16,510 relationship here. 131 00:07:16,510 --> 00:07:18,680 d sigma equals C times de. 132 00:07:18,680 --> 00:07:23,220 Notice that C is not the same as tC. 133 00:07:23,220 --> 00:07:26,690 This is here, relating the total stress 134 00:07:26,690 --> 00:07:27,930 to the total strain. 135 00:07:27,930 --> 00:07:30,790 Here we talk about an increment in stress related to 136 00:07:30,790 --> 00:07:32,430 an increment in strain. 137 00:07:32,430 --> 00:07:36,820 It's important to note that C is not the same as tC. 138 00:07:36,820 --> 00:07:40,750 Unless, of course, we have a linear elastic relationship. 139 00:07:43,370 --> 00:07:48,420 In a computer program, we would represent such a curve 140 00:07:48,420 --> 00:07:53,510 typically by a series of straight lines, as shown here. 141 00:07:53,510 --> 00:07:59,330 And the input, of course, would be these points here, 142 00:07:59,330 --> 00:08:03,460 and the corresponding points on the stress curve. 143 00:08:03,460 --> 00:08:07,670 Notice that if you take a large number of such straight 144 00:08:07,670 --> 00:08:11,010 segments, you can really approximate a continuous curve 145 00:08:11,010 --> 00:08:14,620 such as this one here quite well. 146 00:08:14,620 --> 00:08:18,930 We can generalize this elastic material behavior using the 147 00:08:18,930 --> 00:08:23,350 total Lagrangian formulation, as shown here. 148 00:08:23,350 --> 00:08:27,320 Notice that the total stress, second Piola-Kirchhoff 149 00:08:27,320 --> 00:08:29,380 stress-- we talked about this stress measure 150 00:08:29,380 --> 00:08:31,580 in an earlier lecture-- 151 00:08:31,580 --> 00:08:35,679 is given by the stress strain law times the total strain. 152 00:08:35,679 --> 00:08:38,400 Green-Lagrange strain-- once again we talked about this 153 00:08:38,400 --> 00:08:41,610 strain measure in an earlier lecture. 154 00:08:41,610 --> 00:08:44,130 Incrementally, we have this relationship. 155 00:08:44,130 --> 00:08:46,510 The increment in the second Piola-Kirchhoff stress is 156 00:08:46,510 --> 00:08:51,130 related to the increment in the Green-Lagrange strain via 157 00:08:51,130 --> 00:08:52,890 this constitutive law. 158 00:08:52,890 --> 00:08:57,690 Notice that this tensor or the components of this tensor are 159 00:08:57,690 --> 00:09:02,400 not the same as those components in general. 160 00:09:02,400 --> 00:09:06,790 This material description is frequently employed in two 161 00:09:06,790 --> 00:09:12,460 types of analysis, the usual constant material moduli for 162 00:09:12,460 --> 00:09:15,570 infinitesimal displacement analysis. 163 00:09:15,570 --> 00:09:20,120 Or for rubber-type analysis, rubber-type materials, I 164 00:09:20,120 --> 00:09:23,890 should say, where of course this matrix is not constant. 165 00:09:23,890 --> 00:09:27,090 And that matrix is not constant either. 166 00:09:27,090 --> 00:09:29,550 I like to now spend time on discussing 167 00:09:29,550 --> 00:09:33,410 these type of analyses. 168 00:09:33,410 --> 00:09:36,980 The use of the constant material moduli means, for 169 00:09:36,980 --> 00:09:41,500 example, for an isotropic material, that we use these 170 00:09:41,500 --> 00:09:46,610 matrices given via this relationship here. 171 00:09:46,610 --> 00:09:50,750 Notice lambda and mu are the Lame constants, that you're 172 00:09:50,750 --> 00:09:54,780 probably familiar with, and data ij is the Kronecker data, 173 00:09:54,780 --> 00:09:57,570 defined as shown down here. 174 00:09:57,570 --> 00:10:00,430 These are the same constants that are used 175 00:10:00,430 --> 00:10:03,410 also in linear analysis. 176 00:10:03,410 --> 00:10:09,530 So no new parameters are introduced here. 177 00:10:09,530 --> 00:10:15,100 As examples, here we have the stress strain law for the 2-D 178 00:10:15,100 --> 00:10:18,190 plane stress analysis. 179 00:10:18,190 --> 00:10:22,880 I've written it in matrix form, and this zero here means 180 00:10:22,880 --> 00:10:25,640 total Lagrangian formulation. 181 00:10:25,640 --> 00:10:29,550 And notice that there could also be a t up here. 182 00:10:29,550 --> 00:10:35,150 In other words, we use the same matrix for the increment 183 00:10:35,150 --> 00:10:39,440 in the stresses and for the total stresses. 184 00:10:39,440 --> 00:10:45,590 So I could very easily put a t up there, and we notice then 185 00:10:45,590 --> 00:10:51,640 that the last row corresponds to this relationship here. 186 00:10:51,640 --> 00:10:54,770 It's important to recognize that on the right hand side 187 00:10:54,770 --> 00:10:57,970 here, we have the Green-Lagrange strain, t0 zero 188 00:10:57,970 --> 00:11:01,240 epsilon 12 plus t0 21. 189 00:11:01,240 --> 00:11:05,200 In other words, we take the total sharing strain into 190 00:11:05,200 --> 00:11:06,510 account here. 191 00:11:06,510 --> 00:11:09,340 And that gives us then this row and 192 00:11:09,340 --> 00:11:10,590 that column, of course. 193 00:11:13,070 --> 00:11:17,090 For 2-D, access symmetric analysis, we would use this 194 00:11:17,090 --> 00:11:20,180 stress-strain law, once again, for the increments in the 195 00:11:20,180 --> 00:11:22,670 stresses and for the total stresses. 196 00:11:25,480 --> 00:11:29,850 For an orthotropic material, we would typically have this 197 00:11:29,850 --> 00:11:34,316 stress strain law in plane stress, plane strain analysis. 198 00:11:34,316 --> 00:11:37,630 And there you see again, the zero. 199 00:11:37,630 --> 00:11:42,880 Notice Ea, Eb are the material and nu ab are the material 200 00:11:42,880 --> 00:11:46,790 moduli corresponding to the a and b, directions and 201 00:11:46,790 --> 00:11:51,020 similarly the sheer modulis Gab. 202 00:11:51,020 --> 00:11:56,880 The material being orthotropic means Ea is not equal to Eb. 203 00:11:56,880 --> 00:12:00,680 This once again is the material law that we are quite 204 00:12:00,680 --> 00:12:04,610 familiar with from linear analysis. 205 00:12:04,610 --> 00:12:08,240 Now let's look at the sample problem, the sample analysis. 206 00:12:08,240 --> 00:12:11,950 And I would like to choose a very simple problem to just 207 00:12:11,950 --> 00:12:16,050 demonstrate some of the aspects of using a total 208 00:12:16,050 --> 00:12:19,980 Lagrangian formulation with a constant material law. 209 00:12:19,980 --> 00:12:27,230 Here we have a bar, with cross sectional area A bar. 210 00:12:27,230 --> 00:12:31,380 We use the material constants E and nu, the ones that we are 211 00:12:31,380 --> 00:12:35,530 used to you in liner analysis. 212 00:12:35,530 --> 00:12:40,550 And we want to use this stress strain relationship. 213 00:12:40,550 --> 00:12:45,650 We assume that the area A bar remains constant when we pull 214 00:12:45,650 --> 00:12:49,740 the bar out, or when we push it in. 215 00:12:49,740 --> 00:12:54,370 This E curl here is given via this relationship here, E 216 00:12:54,370 --> 00:12:58,750 being the Young's modulis nu being the Poisson ratio. 217 00:12:58,750 --> 00:13:04,090 In tension, the bar would be pulled out as shown here. 218 00:13:04,090 --> 00:13:06,370 Notice the area, the cross sectional 219 00:13:06,370 --> 00:13:08,740 area, remains constant. 220 00:13:08,740 --> 00:13:14,860 And the displacement is measured as t delta. 221 00:13:14,860 --> 00:13:22,050 In compression, the bar would be pushed into, as shown here. 222 00:13:22,050 --> 00:13:27,930 Notice here now t delta and the bar has been pushed in as 223 00:13:27,930 --> 00:13:29,530 shown by the blue outline. 224 00:13:32,470 --> 00:13:39,810 If we now apply this stress strain law, to the problem and 225 00:13:39,810 --> 00:13:45,700 develop a relationship between the force required here to 226 00:13:45,700 --> 00:13:51,190 pull the bar out or push it in, by delta, 227 00:13:51,190 --> 00:13:54,400 we obtain the following. 228 00:13:54,400 --> 00:13:57,330 Here we have the Green-Lagrange strain. 229 00:13:57,330 --> 00:14:00,830 And of course, the right hand side involves derivatives that 230 00:14:00,830 --> 00:14:04,410 we have been discussing in the previous lecture. 231 00:14:04,410 --> 00:14:09,950 Notice t0u1,1 is nothing else than this relationship here. 232 00:14:09,950 --> 00:14:14,070 It's given by the current length and the original length 233 00:14:14,070 --> 00:14:15,630 of the bar. 234 00:14:15,630 --> 00:14:20,470 Substituting into here, we get directly this right hand side. 235 00:14:20,470 --> 00:14:25,340 We also remember that we can calculate or we have a very 236 00:14:25,340 --> 00:14:29,300 clear relationship between the Cauchy stress, which is the 237 00:14:29,300 --> 00:14:31,910 force per unit area, which we are interested 238 00:14:31,910 --> 00:14:33,250 in calculating here. 239 00:14:33,250 --> 00:14:37,560 And the second, Piola-Kirchhoff stress, this 240 00:14:37,560 --> 00:14:40,750 is the inverse of the deformation gradient. 241 00:14:40,750 --> 00:14:46,100 We substitute for here, the Cauchy stress of course being 242 00:14:46,100 --> 00:14:51,490 simply the force divided by A bar, the inverse of the 243 00:14:51,490 --> 00:14:53,440 deformation gradient being given by this 244 00:14:53,440 --> 00:14:55,400 relationship here. 245 00:14:55,400 --> 00:14:58,740 And therefore we can evaluate the second Piola-Kirchhoff 246 00:14:58,740 --> 00:15:02,730 stress in of the externally applied force, the physical 247 00:15:02,730 --> 00:15:07,650 force, divided by the constant area, cross-sectional area, A 248 00:15:07,650 --> 00:15:12,520 bar, and the original length and the current length. 249 00:15:12,520 --> 00:15:15,370 We therefore have now the Green-Lagrange strain and the 250 00:15:15,370 --> 00:15:20,020 second Piola-Kirchhoff stress, in terms of current lengths 251 00:15:20,020 --> 00:15:25,160 and original lengths and force applied-- 252 00:15:25,160 --> 00:15:27,900 and of course the cross section area goes in there. 253 00:15:27,900 --> 00:15:30,950 Substituting these relationship and that 254 00:15:30,950 --> 00:15:34,680 relationship into our stress strain relationship of the 255 00:15:34,680 --> 00:15:43,530 previous view graph and using this fact here, we directly 256 00:15:43,530 --> 00:15:49,600 obtain this red curve in the-- 257 00:15:49,600 --> 00:15:54,750 which gives us the force applied to the bar as a 258 00:15:54,750 --> 00:15:59,240 function of the displacements at the end of the bar. 259 00:15:59,240 --> 00:16:03,340 Now notice that this is a nonlinear curve-- 260 00:16:03,340 --> 00:16:07,190 the expression is actually given here-- 261 00:16:07,190 --> 00:16:11,270 and that it is quite unrealistic, certainly in this 262 00:16:11,270 --> 00:16:12,300 region here. 263 00:16:12,300 --> 00:16:17,340 It's not a realistic material description for large strains. 264 00:16:17,340 --> 00:16:24,070 You see here at this point, we have a 0 force to be applied 265 00:16:24,070 --> 00:16:29,060 when the displacement, the end of the displacement, is minus 266 00:16:29,060 --> 00:16:31,010 the original lengths off the bar. 267 00:16:31,010 --> 00:16:32,920 Quite unrealistic, of course. 268 00:16:32,920 --> 00:16:38,410 And therefore, we recognize that really this use of a 269 00:16:38,410 --> 00:16:43,730 constant E and nu, going in here, constant Young's modulus 270 00:16:43,730 --> 00:16:46,710 and Poisson's ratio, going in here. 271 00:16:46,710 --> 00:16:53,060 It's really not a proper or realistic way to proceed for 272 00:16:53,060 --> 00:16:54,310 large strains. 273 00:16:57,010 --> 00:17:00,260 The usual isotopical and also orthotopic material 274 00:17:00,260 --> 00:17:05,020 relationships, meeting constant E, nu, Ea, et cetera, 275 00:17:05,020 --> 00:17:09,020 the way I just showed it on a few previous view graphs are 276 00:17:09,020 --> 00:17:12,520 really almost exclusively employed in large 277 00:17:12,520 --> 00:17:16,234 displacement, large rotation, but small strain analysis. 278 00:17:18,800 --> 00:17:23,300 We should now recall one very important namely that the 279 00:17:23,300 --> 00:17:26,849 components of the second Piola-Kirchhoff stress tensor, 280 00:17:26,849 --> 00:17:30,470 and of the Green-Lagrange strain tensor are invariant 281 00:17:30,470 --> 00:17:35,610 very under a rigid body motion of the material. 282 00:17:35,610 --> 00:17:41,560 And this is most important because we use this fact to 283 00:17:41,560 --> 00:17:45,770 apply material descriptions that are applicable to small 284 00:17:45,770 --> 00:17:51,090 strain analysis directly also to large displacement, large 285 00:17:51,090 --> 00:17:53,210 rotation analysis. 286 00:17:53,210 --> 00:17:58,350 You see, E nu, Ea are material constant that applicable to 287 00:17:58,350 --> 00:17:59,940 small strain analysis. 288 00:17:59,940 --> 00:18:04,230 And we can directly them some also in large displacement, 289 00:18:04,230 --> 00:18:06,710 large quotation analysis, but small strain 290 00:18:06,710 --> 00:18:09,410 analysis using this fact. 291 00:18:13,930 --> 00:18:16,950 And this means-- 292 00:18:16,950 --> 00:18:21,590 another way of saying it is that the actual straining 293 00:18:21,590 --> 00:18:24,990 increases only the components of the Green-Lagrange strain 294 00:18:24,990 --> 00:18:29,060 tensor through the material relationships. 295 00:18:29,060 --> 00:18:31,610 Let's look at this equation here. 296 00:18:31,610 --> 00:18:35,810 We have here the nodal point force vector being equal to 297 00:18:35,810 --> 00:18:36,980 the stress strain-- 298 00:18:36,980 --> 00:18:42,280 the strain displacement matrix times a stress vector, the 299 00:18:42,280 --> 00:18:45,030 second Piola-Kirchhoff stress vector. 300 00:18:45,030 --> 00:18:49,310 Now this vector is invariant under rigid body rotation. 301 00:18:49,310 --> 00:18:51,670 And of course, this vector is calculated using the 302 00:18:51,670 --> 00:18:53,750 constitutive relation. 303 00:18:53,750 --> 00:18:57,030 This strain displacement matrix takes 304 00:18:57,030 --> 00:18:59,570 into account the rotation. 305 00:18:59,570 --> 00:19:05,690 Let's look at this fact a little bit closer. 306 00:19:05,690 --> 00:19:09,050 Here we have pictorially an element, a four-node element 307 00:19:09,050 --> 00:19:14,050 say, that originally is in this configuration, the black 308 00:19:14,050 --> 00:19:24,110 configuration, and we are pulling it out and sharing it. 309 00:19:24,110 --> 00:19:27,850 If this length here is 1 originally, and that length 310 00:19:27,850 --> 00:19:32,550 here is 1 originally, then this distance here corresponds 311 00:19:32,550 --> 00:19:36,870 to the Green-Lagrange strain in the 1:1 direction, in the 312 00:19:36,870 --> 00:19:38,220 one direction. 313 00:19:38,220 --> 00:19:41,890 In other words, it's equal to 1 0 epsilon 1 1. 314 00:19:41,890 --> 00:19:46,560 Similar, this distance here is equal to 1 0 epsilon 2 2, and 315 00:19:46,560 --> 00:19:50,800 the total sharing is equal to the sum of these two 316 00:19:50,800 --> 00:19:53,790 components here. 317 00:19:53,790 --> 00:19:59,170 This is the deformation that brings the element, say, from 318 00:19:59,170 --> 00:20:03,730 the original configuration to state 1. 319 00:20:03,730 --> 00:20:10,470 Now, going from state 1 to state 2, we rotate the element 320 00:20:10,470 --> 00:20:14,290 rigidly, as shown here. 321 00:20:14,290 --> 00:20:19,740 Then we know that this distance here is still 1 0 322 00:20:19,740 --> 00:20:21,690 epsilon 1 1. 323 00:20:21,690 --> 00:20:24,230 Same as what we have had here. 324 00:20:24,230 --> 00:20:30,010 This distance here is the same as what we have seen here. 325 00:20:30,010 --> 00:20:35,810 And the total sharing is still the same as what the total 326 00:20:35,810 --> 00:20:39,060 sharing was here. 327 00:20:39,060 --> 00:20:44,140 Notice the Green-Lagrange strain components 328 00:20:44,140 --> 00:20:48,480 corresponding to the stationary coordinate axes. 329 00:20:48,480 --> 00:20:52,300 1 and 2 have not changed. 330 00:20:52,300 --> 00:20:59,170 Because here this 1 and that 2 refer still too the stationary 331 00:20:59,170 --> 00:21:00,420 coordinate frame. 332 00:21:04,210 --> 00:21:06,425 On this view graph, we summarize this information 333 00:21:06,425 --> 00:21:10,330 once more for small strains, we have of course this 334 00:21:10,330 --> 00:21:16,570 relationship here, which means that these strain components 335 00:21:16,570 --> 00:21:19,280 are much smaller than 1. 336 00:21:19,280 --> 00:21:23,340 And we can directly say that the second Piola-Kirchhoff 337 00:21:23,340 --> 00:21:26,710 stress in configuration 1 is given by the Green-Lagrange 338 00:21:26,710 --> 00:21:29,030 strains in configuration 1. 339 00:21:29,030 --> 00:21:32,290 Notice the second Piola-Kirchhoff stress is 340 00:21:32,290 --> 00:21:36,860 approximately equal to the Cauchy stress in state 1. 341 00:21:36,860 --> 00:21:41,680 Now since state 2 is reached by just a rigid body motion, 342 00:21:41,680 --> 00:21:47,620 we find that this holds, as I already pointed out on the 343 00:21:47,620 --> 00:21:48,850 earlier view graph. 344 00:21:48,850 --> 00:21:52,290 We also find that this holds. 345 00:21:52,290 --> 00:21:55,575 And of course, the Cauchy stresses in state 2 are 346 00:21:55,575 --> 00:22:01,040 obtained by a rotation of the Cauchy stresses in state 1. 347 00:22:01,040 --> 00:22:04,320 But the second Piola-Kirchhoff stresses and Green-Lagrange 348 00:22:04,320 --> 00:22:07,620 strains, the components of these two tensors are 349 00:22:07,620 --> 00:22:10,790 invariant under the rigid body motion. 350 00:22:10,790 --> 00:22:14,270 And that means that we can directly apply material 351 00:22:14,270 --> 00:22:18,360 relationships that are applicable for small strains 352 00:22:18,360 --> 00:22:20,710 and infinitesimal displacements. 353 00:22:20,710 --> 00:22:24,750 Those that we are, say, already familiar with from an 354 00:22:24,750 --> 00:22:26,660 MNO analysis. 355 00:22:26,660 --> 00:22:30,070 We can directly apply these to large displacement, large 356 00:22:30,070 --> 00:22:34,160 rotation, but small strain analysis, by simply using 357 00:22:34,160 --> 00:22:38,000 Green-Lagrange strains instead of engineering strain 358 00:22:38,000 --> 00:22:40,590 components, and second Piola-Kirchhoff stresses 359 00:22:40,590 --> 00:22:43,950 instead of the engineering stress components. 360 00:22:46,780 --> 00:22:51,270 Applications are really all large displacement, large 361 00:22:51,270 --> 00:22:53,290 rotation, small strain analyses of 362 00:22:53,290 --> 00:22:54,700 beams, plates, and shells. 363 00:22:57,450 --> 00:23:02,565 We can use for this analysis frequently simply the 2D and 364 00:23:02,565 --> 00:23:06,040 3D elements that we discussed earlier. 365 00:23:06,040 --> 00:23:10,070 But we may want to use beam and shell elements, and those 366 00:23:10,070 --> 00:23:14,070 we will discuss in later lectures. 367 00:23:14,070 --> 00:23:18,860 We also have a very large application area here, namely, 368 00:23:18,860 --> 00:23:22,700 the linearized buckling analysis of structures. 369 00:23:22,700 --> 00:23:28,520 We have already performed the analysis of shells, or shown 370 00:23:28,520 --> 00:23:31,250 how we analyze shelves and beams 371 00:23:31,250 --> 00:23:34,670 using continuum elements. 372 00:23:34,670 --> 00:23:36,800 You might recall it from the earlier lectures. 373 00:23:36,800 --> 00:23:41,500 Here you have just schematically how we would 374 00:23:41,500 --> 00:23:45,530 model say a frame using plain stress elements. 375 00:23:45,530 --> 00:23:47,960 And here you should see schematically how we are 376 00:23:47,960 --> 00:23:51,170 modeling using axisymmetric continuum elements and 377 00:23:51,170 --> 00:23:52,420 axisymmetric shell. 378 00:23:55,060 --> 00:24:01,100 Here we use 3D elements to model a general shell. 379 00:24:01,100 --> 00:24:05,590 But as I pointed out, we will talk in later lectures about 380 00:24:05,590 --> 00:24:09,290 actual beam and shell elements that are frequently much more 381 00:24:09,290 --> 00:24:12,135 effective in the analysis of beam and shell structures. 382 00:24:15,050 --> 00:24:18,970 This completes the first large item that I wanted to talk to 383 00:24:18,970 --> 00:24:24,220 you about, namely, the use of constant material moduli, E, 384 00:24:24,220 --> 00:24:31,590 nu, Ea, Eb, et cetera in large displacement, large rotation 385 00:24:31,590 --> 00:24:34,900 analysis, but small strain analysis. 386 00:24:34,900 --> 00:24:39,210 We found that the applicability of constant 387 00:24:39,210 --> 00:24:43,610 material moduli to large strain analysis is really very 388 00:24:43,610 --> 00:24:46,260 questionable. 389 00:24:46,260 --> 00:24:52,340 For large strain analysis, we use frequently a hyperelastic 390 00:24:52,340 --> 00:24:54,210 material model. 391 00:24:54,210 --> 00:24:58,180 And that is very widely used to analyze rubber materials. 392 00:24:58,180 --> 00:25:02,670 Here we have the relationship that is basic to this 393 00:25:02,670 --> 00:25:03,500 description. 394 00:25:03,500 --> 00:25:08,160 We have the Piola-Kirchhoff stress, given in terms of the 395 00:25:08,160 --> 00:25:12,710 partial of the strain energy density function, W, this 396 00:25:12,710 --> 00:25:15,510 respect to the Green-Lagrange strains. 397 00:25:15,510 --> 00:25:20,030 So we get one component here, by taking this t0W and 398 00:25:20,030 --> 00:25:23,460 differentiating it with respect to the corresponding 399 00:25:23,460 --> 00:25:25,930 component of the Green-Lagrange strain. 400 00:25:25,930 --> 00:25:27,810 And of course this right hand side gives 401 00:25:27,810 --> 00:25:29,460 us this tensor t0Cijrs. 402 00:25:32,460 --> 00:25:35,860 Incrementally, then, we have an increment in the second 403 00:25:35,860 --> 00:25:40,010 Piola-Kirchhoff stress is given by this stress strain 404 00:25:40,010 --> 00:25:46,400 law here, involving a tangent material description and an 405 00:25:46,400 --> 00:25:48,140 increment, a differential increment, in the 406 00:25:48,140 --> 00:25:49,960 Green-Lagrange strain. 407 00:25:49,960 --> 00:25:54,720 This 0Cijrs is nothing else but the second partial 408 00:25:54,720 --> 00:25:59,210 derivative of W with respect to these Green-Lagrange strain 409 00:25:59,210 --> 00:26:00,670 components. 410 00:26:00,670 --> 00:26:03,390 W is a strain energy density function per 411 00:26:03,390 --> 00:26:05,170 unit original volume. 412 00:26:05,170 --> 00:26:08,700 And of course that has to be defined for the particular 413 00:26:08,700 --> 00:26:11,200 material that you're looking at and will involve certain 414 00:26:11,200 --> 00:26:13,180 material constants. 415 00:26:13,180 --> 00:26:17,290 For rubber, we generally use this kind of description here, 416 00:26:17,290 --> 00:26:23,140 where W is a function of I1, I2, I3, and the Is are the 417 00:26:23,140 --> 00:26:26,340 invariants of the Cauchy-Green deformation tensor. 418 00:26:26,340 --> 00:26:29,975 We discuss the Cauchy-Green deformation tensor in an 419 00:26:29,975 --> 00:26:31,720 earlier lecture. 420 00:26:31,720 --> 00:26:35,600 Of course, it's given in terms of the deformation gradient. 421 00:26:35,600 --> 00:26:38,280 So I1 is equal to this. 422 00:26:38,280 --> 00:26:40,590 I2 is equal to this relationship here on 423 00:26:40,590 --> 00:26:41,700 the right hand side. 424 00:26:41,700 --> 00:26:44,530 And I3 is simply the determinant of the 425 00:26:44,530 --> 00:26:48,900 Cauchy-Green deformation tensor. 426 00:26:48,900 --> 00:26:52,665 For example, one material law that is quite widely used is 427 00:26:52,665 --> 00:26:56,050 the Mooney-Rivlin material law, where two 428 00:26:56,050 --> 00:26:59,260 constants enter here. 429 00:26:59,260 --> 00:27:02,140 And of course, we have here I1 and 12. 430 00:27:02,140 --> 00:27:05,270 These are material constants that have to be determined 431 00:27:05,270 --> 00:27:07,960 depending on what rubber you're dealing with. 432 00:27:07,960 --> 00:27:12,880 And the incompressibility constraint is imposed onto the 433 00:27:12,880 --> 00:27:16,720 formulation by having I3 equal to 1. 434 00:27:16,720 --> 00:27:20,930 Of course, rubber is an incompressible material, at 435 00:27:20,930 --> 00:27:24,060 least almost an incompressible material, and is modeled as an 436 00:27:24,060 --> 00:27:25,240 incompressible material. 437 00:27:25,240 --> 00:27:28,930 And so we want to have I3 equal to 1. 438 00:27:28,930 --> 00:27:33,100 In general, if you deal with incompressible materials, it 439 00:27:33,100 --> 00:27:38,260 is effective to not use the displacement-based finite 440 00:27:38,260 --> 00:27:40,700 element formulations the way I've been discussing it in the 441 00:27:40,700 --> 00:27:45,210 previous lectures, but to amend that formulation, you 442 00:27:45,210 --> 00:27:48,340 should really extend that formulation to have an 443 00:27:48,340 --> 00:27:50,630 effective formulation to deal with 444 00:27:50,630 --> 00:27:54,120 incompressibility in the analysis. 445 00:27:54,120 --> 00:27:58,430 Except for the plane stress case, we can directly use what 446 00:27:58,430 --> 00:28:00,680 we discussed earlier. 447 00:28:00,680 --> 00:28:05,570 The formation for incompressibility, or for 448 00:28:05,570 --> 00:28:10,840 analysis of incompressible materials, such formulations 449 00:28:10,840 --> 00:28:15,700 of course are very valuable but the discussion of such 450 00:28:15,700 --> 00:28:20,010 formulations really deserves another lecture. 451 00:28:20,010 --> 00:28:26,680 Well, we like to now show how this material law is used in 452 00:28:26,680 --> 00:28:28,400 the plane stress case. 453 00:28:28,400 --> 00:28:32,130 There we can directly employ the formulation that we 454 00:28:32,130 --> 00:28:35,010 discussed in the earlier lectures. 455 00:28:35,010 --> 00:28:39,360 Time 0, for example, we would have a piece of material as 456 00:28:39,360 --> 00:28:40,330 shown here. 457 00:28:40,330 --> 00:28:44,210 At time t, this piece of material has deformed, as 458 00:28:44,210 --> 00:28:46,230 shown here. 459 00:28:46,230 --> 00:28:49,070 Notice plane stress of course means stress is 460 00:28:49,070 --> 00:28:52,300 0 through the thickness. 461 00:28:52,300 --> 00:28:56,630 For this two-dimensional problem, the Cauchy-Green 462 00:28:56,630 --> 00:29:01,100 deformation tensor is as shown here. 463 00:29:01,100 --> 00:29:04,840 0 components here. 464 00:29:04,840 --> 00:29:07,890 And we imposed the incompressibility of the 465 00:29:07,890 --> 00:29:14,980 material by simply setting the determinant of this matrix 466 00:29:14,980 --> 00:29:16,170 equal to 1. 467 00:29:16,170 --> 00:29:20,770 And this gives us then a constraint on T0C33. 468 00:29:20,770 --> 00:29:24,330 Basically, we are saying physically that we constrain 469 00:29:24,330 --> 00:29:30,110 the material to shrink into this 33 direction such that 470 00:29:30,110 --> 00:29:34,000 for the applied stresses in the plane of the material, the 471 00:29:34,000 --> 00:29:37,270 material acts as incompressible. 472 00:29:37,270 --> 00:29:40,770 And that's what's being done here mathematically. 473 00:29:40,770 --> 00:29:45,010 We can now evaluate with this constraint I1 and I2. 474 00:29:45,010 --> 00:29:47,280 Here you see the expressions. 475 00:29:49,950 --> 00:29:53,965 And if we have I1 and I2, we can go back to the material 476 00:29:53,965 --> 00:29:59,070 law, substitute and directly octane obtain our second 477 00:29:59,070 --> 00:30:05,940 Piola-Kirchhoff stresses, in terms of the Cauchy-Green 478 00:30:05,940 --> 00:30:09,160 deformation tensor components. 479 00:30:09,160 --> 00:30:12,290 And of course, we also have a relationship between the 480 00:30:12,290 --> 00:30:15,100 Cauchy-Green deformation tensor components and the 481 00:30:15,100 --> 00:30:17,690 Green-Lagrange strain components. 482 00:30:17,690 --> 00:30:19,380 Those we use. 483 00:30:19,380 --> 00:30:24,370 That relationship we use, and that actually brings into it 484 00:30:24,370 --> 00:30:25,800 this relationship here. 485 00:30:28,500 --> 00:30:31,640 And if you performed then the differentiation, the final 486 00:30:31,640 --> 00:30:36,220 result is shown on this view graph. 487 00:30:36,220 --> 00:30:39,730 This is the stress strain relationship that gives the 488 00:30:39,730 --> 00:30:45,280 total stresses in terms of the Cij components. 489 00:30:50,670 --> 00:30:56,010 You similarly proceed to also calculate the tangent 490 00:30:56,010 --> 00:30:58,850 relationship, the tangent stress strain law. 491 00:30:58,850 --> 00:31:01,780 As I pointed out earlier, you need to now take second 492 00:31:01,780 --> 00:31:05,290 derivatives of W with respect to the Green-Lagrange strain 493 00:31:05,290 --> 00:31:06,740 components. 494 00:31:06,740 --> 00:31:09,310 And if you also use the relationships between the 495 00:31:09,310 --> 00:31:11,530 Green-Lagrange strain components and the components 496 00:31:11,530 --> 00:31:13,590 of the Cauchy-Green deformation tensor, you 497 00:31:13,590 --> 00:31:15,590 directly arrive at this expression. 498 00:31:15,590 --> 00:31:19,090 And of course now, you would have to substitute as we did 499 00:31:19,090 --> 00:31:23,600 earlier for calculating the total stress strain law, in 500 00:31:23,600 --> 00:31:27,580 other words, the stress strain giving us a total stress as a 501 00:31:27,580 --> 00:31:29,930 function of the total deformations. 502 00:31:29,930 --> 00:31:34,110 You proceed in the same way, and obtain the tangent stress 503 00:31:34,110 --> 00:31:35,790 strain law. 504 00:31:35,790 --> 00:31:39,080 Let us now look at an example. 505 00:31:39,080 --> 00:31:43,280 In this example, we are considering the analysis of a 506 00:31:43,280 --> 00:31:45,080 tensile test specimen. 507 00:31:45,080 --> 00:31:46,830 The specimen is shown here. 508 00:31:46,830 --> 00:31:49,490 All dimensions are given in millimeters. 509 00:31:49,490 --> 00:31:53,270 The thickness of the specimen is one millimeter, and the 510 00:31:53,270 --> 00:31:57,540 Mooney-Rivlin constants are given here. 511 00:31:57,540 --> 00:32:00,720 We need to model only one quarter of the specimen 512 00:32:00,720 --> 00:32:02,850 because of symmetry conditions. 513 00:32:02,850 --> 00:32:07,930 And in the analysis, we used 14 eight-node elements to 514 00:32:07,930 --> 00:32:12,370 represent this quarter of the specimen. 515 00:32:12,370 --> 00:32:15,550 Notice that on the right hand side, we constrained all 516 00:32:15,550 --> 00:32:20,370 material particles to move together and only move to the 517 00:32:20,370 --> 00:32:24,840 right, as shown by delta here. 518 00:32:24,840 --> 00:32:27,890 This represents 1/2 the gauge length of the specimen, and 519 00:32:27,890 --> 00:32:31,040 one is particularly interested in seeing the deformations in 520 00:32:31,040 --> 00:32:33,990 that gauge length. 521 00:32:33,990 --> 00:32:37,880 This view graph now shows the calculated response. 522 00:32:37,880 --> 00:32:40,510 The applied node is given here. 523 00:32:40,510 --> 00:32:42,930 The extension is given here. 524 00:32:42,930 --> 00:32:45,240 This is the gauge response. 525 00:32:45,240 --> 00:32:47,330 And that gives us-- 526 00:32:47,330 --> 00:32:50,910 this curve gives us the total response. 527 00:32:50,910 --> 00:32:54,620 Of course, quite nonlinear, because the material is a 528 00:32:54,620 --> 00:32:57,840 nonlinear elastic material. 529 00:32:57,840 --> 00:33:02,900 The deformed mesh is shown on the next view graph here. 530 00:33:02,900 --> 00:33:05,975 At the force 4 Newton, we have this deformed mesh 531 00:33:05,975 --> 00:33:08,110 here shown in red. 532 00:33:08,110 --> 00:33:12,640 And notice here, we have the undeformed mesh in dashed 533 00:33:12,640 --> 00:33:15,090 black line. 534 00:33:15,090 --> 00:33:17,860 Notice that the displacements are large, and the strains 535 00:33:17,860 --> 00:33:23,010 certainly are very large in this problem. 536 00:33:23,010 --> 00:33:26,270 Finally I would like to share with you some analysis results 537 00:33:26,270 --> 00:33:29,400 that we obtained in the analysis of a rubber sheet 538 00:33:29,400 --> 00:33:30,640 with a hole. 539 00:33:30,640 --> 00:33:34,590 And these analysis results are shown on the slides, so let me 540 00:33:34,590 --> 00:33:40,240 walk over here so that we can share that information. 541 00:33:40,240 --> 00:33:43,330 Here, we show the rubber sheet. 542 00:33:43,330 --> 00:33:47,970 It's a square sheet, 20 inch by 20 inch, that contains a 543 00:33:47,970 --> 00:33:51,970 hole of diameter 6-inch. 544 00:33:51,970 --> 00:33:56,460 Notice the sheet is subjected to a force on the left hand 545 00:33:56,460 --> 00:33:59,460 side, the distributed pressure, uniformly 546 00:33:59,460 --> 00:34:01,960 distributed pressure on the left hand side and on the 547 00:34:01,960 --> 00:34:04,330 right hand side. 548 00:34:04,330 --> 00:34:09,590 The mass density is given over here also, and the thickness 549 00:34:09,590 --> 00:34:11,940 off the sheet is given here as well. 550 00:34:11,940 --> 00:34:15,545 We will use the mass density later on when we perform also 551 00:34:15,545 --> 00:34:19,960 or look at the results of a dynamic analysis. 552 00:34:19,960 --> 00:34:22,980 The next slide now shows the finite element mesh that we 553 00:34:22,980 --> 00:34:27,120 used to model one quarter of the sheet. 554 00:34:27,120 --> 00:34:30,590 We only needed to model one quarter because of symmetry 555 00:34:30,590 --> 00:34:31,969 conditions. 556 00:34:31,969 --> 00:34:36,860 Notice we used four-node elements in this mesh, and 557 00:34:36,860 --> 00:34:41,040 that the distributive pressure on this right hand side is 558 00:34:41,040 --> 00:34:47,590 modeled by concentrated loads at these nodes. 559 00:34:47,590 --> 00:34:51,350 The next slide shows now the solution 560 00:34:51,350 --> 00:34:54,050 results that we obtained. 561 00:34:54,050 --> 00:34:58,250 Notice down here, we have a little key for the points that 562 00:34:58,250 --> 00:35:00,070 we want to look at. 563 00:35:00,070 --> 00:35:07,330 Here is point B. Here is point A. And here is point C. The 564 00:35:07,330 --> 00:35:11,500 graphs here shows the displacements at point B, at 565 00:35:11,500 --> 00:35:17,110 point A, and point C. In each case, the W displacement, 566 00:35:17,110 --> 00:35:23,180 which at point B is into this direction, at point A is into 567 00:35:23,180 --> 00:35:28,700 this direction, but at point C is downwards. 568 00:35:28,700 --> 00:35:33,210 Notice the very large displacements, W here, going 569 00:35:33,210 --> 00:35:39,050 up to 10, 11 inches for the load applied. 570 00:35:39,050 --> 00:35:44,500 Remember the sheet is a square sheet of 20 inches, so we have 571 00:35:44,500 --> 00:35:46,215 very large deformations here. 572 00:35:46,215 --> 00:35:50,990 We are computing our solution results obtained in the total 573 00:35:50,990 --> 00:35:55,960 Lagrangian formulation, with the hyperelastic Mooney-Rivlin 574 00:35:55,960 --> 00:36:00,320 material law, with the results obtained by Iding. 575 00:36:00,320 --> 00:36:04,220 In fact, there is almost no difference between our 576 00:36:04,220 --> 00:36:07,020 results, and the results of Iding, so that we could not 577 00:36:07,020 --> 00:36:07,830 plot the difference. 578 00:36:07,830 --> 00:36:11,040 And these curves here refer to our results 579 00:36:11,040 --> 00:36:12,290 and the Iding results. 580 00:36:14,810 --> 00:36:18,150 The next slide now shows the deformations that the sheet 581 00:36:18,150 --> 00:36:21,490 has undergone at maximum load. 582 00:36:21,490 --> 00:36:25,870 Here is the original configuration of the sheet, 583 00:36:25,870 --> 00:36:27,560 the initial configuration. 584 00:36:27,560 --> 00:36:31,670 And here, we show the deformed configuration of the sheet. 585 00:36:34,520 --> 00:36:36,720 Notice that the sheet has undergone very large 586 00:36:36,720 --> 00:36:40,750 displacements and very large strains, particularly of 587 00:36:40,750 --> 00:36:42,620 course here in the region of the hole. 588 00:36:45,900 --> 00:36:50,900 The final slide then shows the dynamic response that the 589 00:36:50,900 --> 00:36:55,740 sheet undergoes when we subject the sheet to a step 590 00:36:55,740 --> 00:37:00,980 loading, where the static loading was applied before. 591 00:37:00,980 --> 00:37:06,340 Notice the step loading is applied over 10 delta-t where 592 00:37:06,340 --> 00:37:10,560 delta-a is 0.0015 seconds. 593 00:37:10,560 --> 00:37:16,850 It goes up linearly to 75 pounds per square inch, and 594 00:37:16,850 --> 00:37:19,440 then it stays constant. 595 00:37:19,440 --> 00:37:23,730 Once again, we're looking at the displacements at point B, 596 00:37:23,730 --> 00:37:29,450 point A, W displacements here, and at point C downward 597 00:37:29,450 --> 00:37:33,860 displacement, again denoted as W. Here you see 598 00:37:33,860 --> 00:37:35,470 the solution response. 599 00:37:35,470 --> 00:37:42,700 Point B, point A, and point C. In this particular analysis, 600 00:37:42,700 --> 00:37:47,640 we used first the Newmark method with data equal to 1/2 601 00:37:47,640 --> 00:37:49,870 and alpha equal to 1/4. 602 00:37:49,870 --> 00:37:52,450 In fact, that is nothing else than the trapezoidal rule, 603 00:37:52,450 --> 00:37:55,090 which we discussed in an earlier lecture. 604 00:37:55,090 --> 00:37:58,430 We also performed the analysis once with the Wilson theta 605 00:37:58,430 --> 00:38:00,680 method, theta being 1.4. 606 00:38:00,680 --> 00:38:03,720 This method we did not discuss in the earlier lecture, but it 607 00:38:03,720 --> 00:38:06,020 is described in the textbook. 608 00:38:06,020 --> 00:38:09,080 Notice that the results obtained using the Newmark 609 00:38:09,080 --> 00:38:12,600 method and the Wilson theta method are really very close 610 00:38:12,600 --> 00:38:15,280 to each other. 611 00:38:15,280 --> 00:38:18,820 It's also interesting to see the static response that the 612 00:38:18,820 --> 00:38:23,130 sheet undergoes for this load level at the points A, B, and 613 00:38:23,130 --> 00:38:28,940 C, and that is given by these horizontal lines. 614 00:38:28,940 --> 00:38:32,790 Once again, you have here a large displacement and very 615 00:38:32,790 --> 00:38:34,890 large strain problem. 616 00:38:34,890 --> 00:38:37,550 This brings me to the end of what I wanted to discuss with 617 00:38:37,550 --> 00:38:38,580 you in this lecture. 618 00:38:38,580 --> 00:38:39,900 Thank you very much for your attention.