1 00:00:00,000 --> 00:00:00,030 2 00:00:00,030 --> 00:00:02,470 The following content is provided under a Creative 3 00:00:02,470 --> 00:00:04,000 Commons license. 4 00:00:04,000 --> 00:00:06,320 Your support will help MIT OpenCourseWare 5 00:00:06,320 --> 00:00:10,690 continue to offer high quality educational resources for free. 6 00:00:10,690 --> 00:00:13,300 To make a donation or view additional materials 7 00:00:13,300 --> 00:00:17,025 from hundreds of MIT courses, visit MIT OpenCourseWare 8 00:00:17,025 --> 00:00:17,650 at OCW.MIT.edu. 9 00:00:17,650 --> 00:00:26,140 10 00:00:26,140 --> 00:00:27,860 PROFESSOR: So what I wanted to do today 11 00:00:27,860 --> 00:00:31,540 was talk about thermal properties of foams. 12 00:00:31,540 --> 00:00:34,530 And foams are often used for thermal insulation. 13 00:00:34,530 --> 00:00:36,150 And that's always closed cell foams 14 00:00:36,150 --> 00:00:37,691 that are used for thermal insulation. 15 00:00:37,691 --> 00:00:38,780 And we'll see why. 16 00:00:38,780 --> 00:00:43,290 And the foams tend to have a low thermal conductivity. 17 00:00:43,290 --> 00:00:46,620 And that's largely because gases have lower conductivity 18 00:00:46,620 --> 00:00:47,684 than solids. 19 00:00:47,684 --> 00:00:49,100 And if you have mostly gas, you're 20 00:00:49,100 --> 00:00:50,559 going to have a lower conductivity. 21 00:00:50,559 --> 00:00:53,183 So they have a low conductivity because they have a high volume 22 00:00:53,183 --> 00:00:54,230 fraction of gas. 23 00:00:54,230 --> 00:00:57,640 And they've got a low volume fraction of the solid. 24 00:00:57,640 --> 00:00:59,490 They also have cells. 25 00:00:59,490 --> 00:01:01,480 And the heat is transferred partly 26 00:01:01,480 --> 00:01:03,450 by radiation and convection. 27 00:01:03,450 --> 00:01:06,070 And if you have small cells, you reduce the amount 28 00:01:06,070 --> 00:01:08,070 of convection and radiation. 29 00:01:08,070 --> 00:01:09,360 And we'll see that. 30 00:01:09,360 --> 00:01:12,270 So that, by having a cellular structure, 31 00:01:12,270 --> 00:01:14,230 and in particular, by having small cells, 32 00:01:14,230 --> 00:01:16,740 you can decrease the heat transfer. 33 00:01:16,740 --> 00:01:19,010 OK, so let me write some of the stuff down. 34 00:01:19,010 --> 00:01:30,160 35 00:01:30,160 --> 00:01:36,355 So closed cell foams are widely used for thermal insulation. 36 00:01:36,355 --> 00:01:44,480 37 00:01:44,480 --> 00:01:48,190 And the only materials with lower thermal conductivity 38 00:01:48,190 --> 00:01:50,040 than closed cell foams are aerogels gels. 39 00:01:50,040 --> 00:02:07,355 40 00:02:07,355 --> 00:02:08,729 And I'll I talk a little bit more 41 00:02:08,729 --> 00:02:11,230 about aerogels later on today. 42 00:02:11,230 --> 00:02:12,780 But the difficulty with aerogels is 43 00:02:12,780 --> 00:02:16,600 that they tend to be very weak and brittle, like ridiculously 44 00:02:16,600 --> 00:02:17,580 weak and brittle. 45 00:02:17,580 --> 00:02:21,030 So we had a project on aerogels a couple of years ago. 46 00:02:21,030 --> 00:02:23,530 And the students who I was collaborating with 47 00:02:23,530 --> 00:02:24,410 would make aerogels. 48 00:02:24,410 --> 00:02:26,210 And they'd bring it up to my office. 49 00:02:26,210 --> 00:02:28,390 And I would pick it up and like-- I would pick it up 50 00:02:28,390 --> 00:02:29,640 like this, and it would break. 51 00:02:29,640 --> 00:02:33,010 So they have very low thermal conductivity, 52 00:02:33,010 --> 00:02:34,770 but they're very brittle. 53 00:02:34,770 --> 00:02:37,060 And I brought a few of our samples of aerogels, 54 00:02:37,060 --> 00:02:39,060 just so you can see what they look like. 55 00:02:39,060 --> 00:02:41,000 And I'll pass them around in that little tube, 56 00:02:41,000 --> 00:02:42,980 so you can kind of play with them. 57 00:02:42,980 --> 00:02:46,710 58 00:02:46,710 --> 00:02:49,720 OK, so we're going to focus on foams. 59 00:02:49,720 --> 00:02:57,830 And whoops-- And we can say the low thermal conductivity 60 00:02:57,830 --> 00:03:03,620 of foam arises mostly from the high volume fraction of gas 61 00:03:03,620 --> 00:03:05,200 and that the gas has a low lambda, 62 00:03:05,200 --> 00:03:06,325 a low thermal conductivity. 63 00:03:06,325 --> 00:03:32,384 64 00:03:32,384 --> 00:03:33,800 So lambda is thermal conductivity, 65 00:03:33,800 --> 00:03:35,383 so I'm just going to put lambda there. 66 00:03:35,383 --> 00:03:38,470 67 00:03:38,470 --> 00:03:40,120 Then it has a small volume fraction 68 00:03:40,120 --> 00:03:43,494 of solid, which has a higher thermal conductivity. 69 00:03:43,494 --> 00:03:50,940 70 00:03:50,940 --> 00:03:53,679 And then the foams have a relatively small cell size. 71 00:03:53,679 --> 00:03:55,470 So one of the things we're going to look at 72 00:03:55,470 --> 00:03:58,829 is how does the cell size effect the thermal transfer, 73 00:03:58,829 --> 00:03:59,870 the thermal conductivity. 74 00:03:59,870 --> 00:04:26,771 75 00:04:26,771 --> 00:04:30,980 OK, so there's lots of applications for foams. 76 00:04:30,980 --> 00:04:33,940 And I guess one of the main ones is in buildings, 77 00:04:33,940 --> 00:04:35,690 insulating buildings-- also insulating 78 00:04:35,690 --> 00:04:39,340 refrigerated vehicles, things like LNG tankers. 79 00:04:39,340 --> 00:04:42,577 So there's lots of the applications for using foams 80 00:04:42,577 --> 00:04:43,535 for thermal insulation. 81 00:04:43,535 --> 00:05:05,800 82 00:05:05,800 --> 00:05:08,330 Foams, in addition to having a low thermal conductivity, 83 00:05:08,330 --> 00:05:11,210 they also have good thermal shock resistance. 84 00:05:11,210 --> 00:05:14,250 So thermal shock is if you have a material, you heat it up, 85 00:05:14,250 --> 00:05:16,750 and then you suddenly cool the surface of it, for example. 86 00:05:16,750 --> 00:05:18,958 So say you takes something and you quench it in water 87 00:05:18,958 --> 00:05:22,880 or quench it in some fluid, then the surface, 88 00:05:22,880 --> 00:05:24,922 it wants to shrink because its temperature drops, 89 00:05:24,922 --> 00:05:26,838 but it's connected to everything underneath it 90 00:05:26,838 --> 00:05:28,120 and it can't really shrink. 91 00:05:28,120 --> 00:05:31,230 And so it's constrained and you can get cracking and spalling. 92 00:05:31,230 --> 00:05:34,060 And so, it turns out foams have a good resistance 93 00:05:34,060 --> 00:05:37,600 to that thermal shock kind of loading. 94 00:05:37,600 --> 00:05:38,925 And we'll see why that is, too. 95 00:05:38,925 --> 00:05:57,270 96 00:05:57,270 --> 00:06:00,710 Roughly, you can see if the thermal expansion 97 00:06:00,710 --> 00:06:05,030 strain is the thermal expansion coefficient times the change 98 00:06:05,030 --> 00:06:06,307 in temperature. 99 00:06:06,307 --> 00:06:07,890 And the stress that you might generate 100 00:06:07,890 --> 00:06:11,580 is just going to be related to the modulus times alpha times 101 00:06:11,580 --> 00:06:12,561 delta-t. 102 00:06:12,561 --> 00:06:14,810 And because we're going to see that alpha for the foam 103 00:06:14,810 --> 00:06:16,770 is the same as alpha for the solid, but the E 104 00:06:16,770 --> 00:06:19,670 foam is going to be a lot less that E of a solid would be. 105 00:06:19,670 --> 00:06:21,710 So because the modulus is smaller, 106 00:06:21,710 --> 00:06:26,230 you would get a better thermal shock resistance. 107 00:06:26,230 --> 00:06:31,010 OK, so I wanted to go over a couple of sort 108 00:06:31,010 --> 00:06:32,980 of laws of heat conduction, so we 109 00:06:32,980 --> 00:06:35,860 can talk about what thermal conductivity is 110 00:06:35,860 --> 00:06:37,750 and how we define it. 111 00:06:37,750 --> 00:06:40,526 So the first one here-- 112 00:06:40,526 --> 00:06:49,300 113 00:06:49,300 --> 00:06:52,080 --first one here is for steady state conduction. 114 00:06:52,080 --> 00:06:57,860 115 00:06:57,860 --> 00:07:00,990 So when we say steady state conduction, what we mean 116 00:07:00,990 --> 00:07:03,597 is that the temperature is constant with time, 117 00:07:03,597 --> 00:07:05,305 the temperature doesn't change with time. 118 00:07:05,305 --> 00:07:13,360 119 00:07:13,360 --> 00:07:16,530 So time's not going to come into the equation here. 120 00:07:16,530 --> 00:07:20,570 And heat transfer for steady state conduction, 121 00:07:20,570 --> 00:07:23,480 where there is no change in the temperature with time, 122 00:07:23,480 --> 00:07:24,962 described by Fourier's Law. 123 00:07:24,962 --> 00:07:27,840 124 00:07:27,840 --> 00:07:31,970 And that says that the heat flux q 125 00:07:31,970 --> 00:07:37,720 is equal to minus lambda times the gradient in temperature. 126 00:07:37,720 --> 00:07:41,450 And if you want to think about just a one diversion of that, 127 00:07:41,450 --> 00:07:46,280 it's equal to minus lambda times dt by dx. 128 00:07:46,280 --> 00:07:49,710 So here, q is our heat flux. 129 00:07:49,710 --> 00:07:54,290 130 00:07:54,290 --> 00:07:56,920 So that would have units of joules 131 00:07:56,920 --> 00:07:59,120 per meter squared per second. 132 00:07:59,120 --> 00:08:03,622 So how much heat transfer per unit area per unit time. 133 00:08:03,622 --> 00:08:05,080 Lambda is the thermal conductivity. 134 00:08:05,080 --> 00:08:12,370 135 00:08:12,370 --> 00:08:17,880 And it has units of watts per meter k, so degrees kelvin. 136 00:08:17,880 --> 00:08:22,054 And then delta or-- and then this 137 00:08:22,054 --> 00:08:23,220 is our temperature gradient. 138 00:08:23,220 --> 00:08:31,320 139 00:08:31,320 --> 00:08:32,919 OK, so that's Fourier's Law, and we're 140 00:08:32,919 --> 00:08:37,340 going to use that later on when we talk about the foams. 141 00:08:37,340 --> 00:08:39,940 And then, just so that we have things a little more complete, 142 00:08:39,940 --> 00:08:42,770 if you have a non-steady heat conduction, if the temperature 143 00:08:42,770 --> 00:08:44,987 varies with time, then there's a difference equation 144 00:08:44,987 --> 00:08:46,570 that involves the thermal diffusivity. 145 00:08:46,570 --> 00:08:50,570 146 00:08:50,570 --> 00:09:00,190 So if we have non-steady heat conduction-- so t 147 00:09:00,190 --> 00:09:03,170 varies with time. 148 00:09:03,170 --> 00:09:04,610 I'm going to call a time tau. 149 00:09:04,610 --> 00:09:08,830 150 00:09:08,830 --> 00:09:12,810 Then a partial differentiation, the partial derivative 151 00:09:12,810 --> 00:09:16,290 of temperature with respect to time 152 00:09:16,290 --> 00:09:17,970 is equal to the diffusivity, that's 153 00:09:17,970 --> 00:09:21,220 given the symbol a, times the second derivative 154 00:09:21,220 --> 00:09:24,020 of temperature with respect of distance, 155 00:09:24,020 --> 00:09:25,870 so with respect x squared. 156 00:09:25,870 --> 00:09:27,836 So here a is the thermal diffusivity. 157 00:09:27,836 --> 00:09:36,760 158 00:09:36,760 --> 00:09:40,420 And it is equal to the thermal conductivity 159 00:09:40,420 --> 00:09:44,740 divided by the density and divided by the specific heat. 160 00:09:44,740 --> 00:09:50,600 So here, rho is the density and cp is the specific heat. 161 00:09:50,600 --> 00:09:54,700 162 00:09:54,700 --> 00:09:57,250 The specific heat is the heat required 163 00:09:57,250 --> 00:09:59,570 to raise the temperature of a unit mass 164 00:09:59,570 --> 00:10:03,220 by the unit temperature. 165 00:10:03,220 --> 00:10:07,700 And so, the density times cp is the volumetric heat capacity. 166 00:10:07,700 --> 00:10:09,570 It's how much energy you would need 167 00:10:09,570 --> 00:10:13,410 to raise a certain volume by, say, 1 degree 168 00:10:13,410 --> 00:10:14,750 k instead of a certain mass. 169 00:10:14,750 --> 00:10:33,090 170 00:10:33,090 --> 00:10:38,110 OK, so on the table here, on the screen, 171 00:10:38,110 --> 00:10:39,810 we have different materials. 172 00:10:39,810 --> 00:10:42,350 And we have the thermal conductivity lambda. 173 00:10:42,350 --> 00:10:44,820 And we have the thermal diffusivity, a. 174 00:10:44,820 --> 00:10:48,320 And I guess I should also say a has units 175 00:10:48,320 --> 00:10:51,510 of meters squared per second. 176 00:10:51,510 --> 00:10:56,240 177 00:10:56,240 --> 00:11:00,230 So this table is arranged in order of decreasing 178 00:11:00,230 --> 00:11:01,280 thermal conductivity. 179 00:11:01,280 --> 00:11:08,010 So here's copper at the top, 384, watts per meter k. 180 00:11:08,010 --> 00:11:09,880 Here's, you know, different metals. 181 00:11:09,880 --> 00:11:11,020 You've got aluminum. 182 00:11:11,020 --> 00:11:12,420 Here's a couple of ceramics. 183 00:11:12,420 --> 00:11:15,230 They're about a factor of 10 less than the metals. 184 00:11:15,230 --> 00:11:18,580 Here's the polymers, another factor of 10 less than that. 185 00:11:18,580 --> 00:11:20,540 And here's some gases. 186 00:11:20,540 --> 00:11:23,030 Air is about 0.025. 187 00:11:23,030 --> 00:11:25,220 Carbon dioxide is less than that. 188 00:11:25,220 --> 00:11:27,410 Triclorofluoromethane, which used 189 00:11:27,410 --> 00:11:30,390 to be used as a gas in foams because it's 190 00:11:30,390 --> 00:11:33,470 got such low thermal conductivity, is 0.008. 191 00:11:33,470 --> 00:11:36,830 But it's no longer used because it's a-- what you call it? 192 00:11:36,830 --> 00:11:39,210 A fluorocarbon. 193 00:11:39,210 --> 00:11:41,590 Anyway, it decreases our ozone layer. 194 00:11:41,590 --> 00:11:43,100 So they don't use that anymore. 195 00:11:43,100 --> 00:11:44,220 Now here's some wood. 196 00:11:44,220 --> 00:11:46,040 So that's one sort of cellular solid. 197 00:11:46,040 --> 00:11:48,430 And they're around 0.04-- something like that. 198 00:11:48,430 --> 00:11:51,150 And here's a group of polymer foams. 199 00:11:51,150 --> 00:11:53,940 And they're a little over 0.025. 200 00:11:53,940 --> 00:11:56,030 So if you think of-- if you had the gas, 201 00:11:56,030 --> 00:11:58,680 air-- if the air was the gas inside the foam, 202 00:11:58,680 --> 00:12:00,905 0.025 is lambda for the gas. 203 00:12:00,905 --> 00:12:02,850 So you're not going to get lower than that. 204 00:12:02,850 --> 00:12:06,440 And you have to use a low conductivity gas to get these 205 00:12:06,440 --> 00:12:10,690 values, like 0.025 here, 0.020, 0.017. 206 00:12:10,690 --> 00:12:13,360 And then, hear some other sorts of sort of mineral fibers, 207 00:12:13,360 --> 00:12:15,140 glass foams, glass wools. 208 00:12:15,140 --> 00:12:19,280 OK, so that's just a table so that you have some data there. 209 00:12:19,280 --> 00:12:19,780 All right? 210 00:12:19,780 --> 00:12:20,720 Yes? 211 00:12:20,720 --> 00:12:30,310 STUDENT: [INAUDIBLE] --foams, if they are closed cell, 212 00:12:30,310 --> 00:12:31,540 with a different gas rate. 213 00:12:31,540 --> 00:12:32,480 Because if they're open cell-- 214 00:12:32,480 --> 00:12:32,530 PROFESSOR: --Right. 215 00:12:32,530 --> 00:12:32,660 The gas is going to-- 216 00:12:32,660 --> 00:12:33,680 STUDENT: --it would just always be air. 217 00:12:33,680 --> 00:12:34,846 PROFESSOR: It's going to go. 218 00:12:34,846 --> 00:12:37,420 And in fact, one of the difficulties 219 00:12:37,420 --> 00:12:39,950 with using the lower conductivity of any gases 220 00:12:39,950 --> 00:12:42,500 is there's a phenomenon called aging, that if, you know, 221 00:12:42,500 --> 00:12:44,720 you've got your gas inside your foam, 222 00:12:44,720 --> 00:12:46,480 it's going to diffuse out into the air. 223 00:12:46,480 --> 00:12:47,900 And air's going to diffuse in. 224 00:12:47,900 --> 00:12:49,980 So over time, the thermal conductivity 225 00:12:49,980 --> 00:12:51,850 tends to increase because you're getting 226 00:12:51,850 --> 00:12:56,440 air coming and the local-- conductivity gas going out. 227 00:12:56,440 --> 00:12:58,410 But I think, typically, that process 228 00:12:58,410 --> 00:13:00,104 takes a number of years. 229 00:13:00,104 --> 00:13:01,270 It doesn't happen in a week. 230 00:13:01,270 --> 00:13:02,530 But if you're designing a building 231 00:13:02,530 --> 00:13:04,488 and want the building to be there for 50 years, 232 00:13:04,488 --> 00:13:05,990 it occurs faster than that. 233 00:13:05,990 --> 00:13:08,385 So it's not ideal from that point of view. 234 00:13:08,385 --> 00:13:10,900 235 00:13:10,900 --> 00:13:12,820 All right. 236 00:13:12,820 --> 00:13:15,600 So let me talk a little bit more about thermal diffusivity. 237 00:13:15,600 --> 00:13:17,991 Let me scoot over here. 238 00:13:17,991 --> 00:13:49,970 239 00:13:49,970 --> 00:13:54,260 So materials with a high value of that thermal diffusivity, a. 240 00:13:54,260 --> 00:13:56,180 They rapidly adjust their temperature 241 00:13:56,180 --> 00:13:57,680 to their surroundings. 242 00:13:57,680 --> 00:14:00,190 So if they have a high value of a, what it really 243 00:14:00,190 --> 00:14:02,220 means they've got a, say, a high value 244 00:14:02,220 --> 00:14:04,570 of lamda-- so high thermal conductivity. 245 00:14:04,570 --> 00:14:07,480 And, say, a low value of this volumetric heat capacity. 246 00:14:07,480 --> 00:14:10,160 So it doesn't take much energy to change their temperature. 247 00:14:10,160 --> 00:14:11,570 And they also conduct heat well. 248 00:14:11,570 --> 00:14:13,940 So they tend to adjust their temperature 249 00:14:13,940 --> 00:14:15,288 to their surroundings quickly. 250 00:14:15,288 --> 00:15:01,570 251 00:15:01,570 --> 00:15:05,110 OK, so then, let's talk about the thermal conductivity 252 00:15:05,110 --> 00:15:05,730 of a foam. 253 00:15:05,730 --> 00:15:13,620 254 00:15:13,620 --> 00:15:15,630 So I'm going to call that lambda star. 255 00:15:15,630 --> 00:15:16,870 So the star is the foam. 256 00:15:16,870 --> 00:15:19,700 And then we'll talk about-- lambda 257 00:15:19,700 --> 00:15:23,410 s will be the lambda for the solid that it's made from. 258 00:15:23,410 --> 00:15:26,730 So if you think of the thermal conductivity of the foam, 259 00:15:26,730 --> 00:15:28,720 there's contributions from different types 260 00:15:28,720 --> 00:15:30,370 of heat transfer. 261 00:15:30,370 --> 00:15:33,610 So you could have conduction through the solid. 262 00:15:33,610 --> 00:15:35,380 I'm going to call that lambda s. 263 00:15:35,380 --> 00:15:38,440 You could have conduction through the gas. 264 00:15:38,440 --> 00:15:40,420 You could have convection within the cell. 265 00:15:40,420 --> 00:15:44,550 So convection has to do with having, say, within the cell, 266 00:15:44,550 --> 00:15:46,390 it might be a different temperature on one 267 00:15:46,390 --> 00:15:48,390 side of the cell to the other side of the cell. 268 00:15:48,390 --> 00:15:50,100 And the warmer side of the cell, the gas 269 00:15:50,100 --> 00:15:52,060 is going to tend to rise to the warmer side 270 00:15:52,060 --> 00:15:54,160 and fall to the cooler side. 271 00:15:54,160 --> 00:15:56,536 And you get a convection current set up. 272 00:15:56,536 --> 00:15:58,160 So you can get heat transfer from that. 273 00:15:58,160 --> 00:16:00,530 And you can also get heat transfer by radiation. 274 00:16:00,530 --> 00:16:03,750 So radiation can cause heat transfer, as well. 275 00:16:03,750 --> 00:16:11,570 So we're going to have contributions from conduction 276 00:16:11,570 --> 00:16:12,342 through the solid. 277 00:16:12,342 --> 00:16:18,850 278 00:16:18,850 --> 00:16:22,780 So the amount of conduction in the foam from the solid-- I'm 279 00:16:22,780 --> 00:16:25,510 going to call lambda star s. 280 00:16:25,510 --> 00:16:28,670 So lambda s would be the conductivity of the solid. 281 00:16:28,670 --> 00:16:32,530 And lambda star s is the thermal conductivity contribution 282 00:16:32,530 --> 00:16:35,490 from the solid in the foam. 283 00:16:35,490 --> 00:16:38,830 So we get kind of-- through the solid. 284 00:16:38,830 --> 00:16:42,490 We have conductivity through the gas. 285 00:16:42,490 --> 00:16:45,230 So it's lambda star g for gas. 286 00:16:45,230 --> 00:16:47,372 And then we could have convection within the cells. 287 00:16:47,372 --> 00:16:55,530 288 00:16:55,530 --> 00:16:58,450 We'll call that lambda star c. 289 00:16:58,450 --> 00:17:04,590 And then we could get radiation through the cell walls 290 00:17:04,590 --> 00:17:05,465 and across the voids. 291 00:17:05,465 --> 00:17:18,609 292 00:17:18,609 --> 00:17:21,890 We'll call that lambda star r. 293 00:17:21,890 --> 00:17:24,069 And so, the thermal conductivity of the foam 294 00:17:24,069 --> 00:17:25,908 is just the sum of those four contributions. 295 00:17:25,908 --> 00:17:40,447 296 00:17:40,447 --> 00:17:42,030 So we're just going to go through each 297 00:17:42,030 --> 00:17:45,880 of those contributions, in turn, and work out 298 00:17:45,880 --> 00:17:48,759 how much thermal conductivity you get from each of them. 299 00:17:48,759 --> 00:17:50,800 And it turns out most of the thermal conductivity 300 00:17:50,800 --> 00:17:53,280 comes through the gas. 301 00:17:53,280 --> 00:18:04,740 So if we first look at just conduction through the solid, 302 00:18:04,740 --> 00:18:10,250 we've got that contribution to the conductivity of the foam 303 00:18:10,250 --> 00:18:14,730 from the solid, it's just equal to some efficiency factor 304 00:18:14,730 --> 00:18:17,650 times the thermal conductivity of the solid times 305 00:18:17,650 --> 00:18:21,710 the volume fraction of the solid or the relative density. 306 00:18:21,710 --> 00:18:24,323 And here, eta is an efficiency factor. 307 00:18:24,323 --> 00:18:30,570 308 00:18:30,570 --> 00:18:33,320 And it accounts for that tortuosity in the foam. 309 00:18:33,320 --> 00:18:35,704 So if you think of the solid in the foam, 310 00:18:35,704 --> 00:18:37,370 it's not like we have little fibers that 311 00:18:37,370 --> 00:18:39,203 just go from one side to the other like this 312 00:18:39,203 --> 00:18:41,460 and the heat just moves along those fibers. 313 00:18:41,460 --> 00:18:44,320 You know, the foam cells have some complicated geometry 314 00:18:44,320 --> 00:18:46,020 and the heat has to kind of run along 315 00:18:46,020 --> 00:18:48,390 that complicated geometry. 316 00:18:48,390 --> 00:18:52,040 And people have made estimates of what this is. 317 00:18:52,040 --> 00:18:54,540 And it's roughly a factor of 2/3. 318 00:18:54,540 --> 00:18:58,610 So I guess it would depend on exactly the foam cell geometry. 319 00:18:58,610 --> 00:19:00,408 But typically it's around 2/3. 320 00:19:00,408 --> 00:19:06,990 321 00:19:06,990 --> 00:19:08,590 So that's conduction through a solid. 322 00:19:08,590 --> 00:19:11,600 That's straight forward. 323 00:19:11,600 --> 00:19:15,900 Conduction through gas is similarly straightforward. 324 00:19:15,900 --> 00:19:18,460 It's just the conductivity of the gas 325 00:19:18,460 --> 00:19:21,220 times the amount of the gas. 326 00:19:21,220 --> 00:19:23,550 And the volume fraction of the gas is just 1 327 00:19:23,550 --> 00:19:25,440 minus the volume fraction of the solid. 328 00:19:25,440 --> 00:19:27,805 So it's just 1 minus the relative density. 329 00:19:27,805 --> 00:19:29,180 So the conduction through the gas 330 00:19:29,180 --> 00:19:32,760 is just lambda g times 1 minus the relative density. 331 00:19:32,760 --> 00:20:07,822 332 00:20:07,822 --> 00:20:09,280 So we can do a little example here. 333 00:20:09,280 --> 00:20:11,030 And you can see how much of the conduction 334 00:20:11,030 --> 00:20:12,517 comes from the solid in the gas. 335 00:20:12,517 --> 00:20:17,900 336 00:20:17,900 --> 00:20:24,230 So for example, if we look at a foam that's 2.5% dense and say 337 00:20:24,230 --> 00:20:28,670 it's a closed cell poly-- what are we doing-- polystyrene. 338 00:20:28,670 --> 00:20:39,320 339 00:20:39,320 --> 00:20:43,380 So the total thermal conductivity of the foam 340 00:20:43,380 --> 00:20:50,410 is about 0.04 watts per meter k. 341 00:20:50,410 --> 00:20:53,640 And the thermal conductivity of polystyrene 342 00:20:53,640 --> 00:20:59,010 is 0.15 watts per meter k. 343 00:20:59,010 --> 00:21:07,500 And the thermal conductivity of air is 0.025. 344 00:21:07,500 --> 00:21:10,900 So let's assume it's just blown with air. 345 00:21:10,900 --> 00:21:12,510 And then if I just add up, what's 346 00:21:12,510 --> 00:21:16,315 the contribution of conduction through the solid 347 00:21:16,315 --> 00:21:18,999 and conduction through the gas-- so I just 348 00:21:18,999 --> 00:21:20,790 use those two little equations-- conduction 349 00:21:20,790 --> 00:21:23,720 through the solid-- it's going to be 2/3 350 00:21:23,720 --> 00:21:28,300 of this value of lambda s times the amount of the solids-- 351 00:21:28,300 --> 00:21:34,077 that's 0.025 and then plus lambda g, which 352 00:21:34,077 --> 00:21:41,850 is 0.025 times the amount of the gas, which is 0.975. 353 00:21:41,850 --> 00:21:46,360 And if I work those two things out, this is 0.003 354 00:21:46,360 --> 00:21:52,160 and this is 0.024. 355 00:21:52,160 --> 00:21:54,730 So that total is 0.027 watts per meter k. 356 00:21:54,730 --> 00:21:58,240 357 00:21:58,240 --> 00:22:02,010 So you can see if the total is 0.04, most of it's 358 00:22:02,010 --> 00:22:02,800 come from the gas. 359 00:22:02,800 --> 00:22:04,330 A little bit's come from the solid. 360 00:22:04,330 --> 00:22:06,900 And the rest is going to be from convection and radiation. 361 00:22:06,900 --> 00:22:09,519 362 00:22:09,519 --> 00:22:10,310 And that's typical. 363 00:22:10,310 --> 00:22:27,560 364 00:22:27,560 --> 00:22:29,810 And that's the reason that they sometimes 365 00:22:29,810 --> 00:22:32,940 use low thermal conductivity gases to blow foams 366 00:22:32,940 --> 00:22:35,020 for thermal insulation because the gas makes up 367 00:22:35,020 --> 00:22:39,034 such a big fraction of the total conductivity. 368 00:22:39,034 --> 00:22:40,450 If you can reduce that, you reduce 369 00:22:40,450 --> 00:22:41,491 the overall conductivity. 370 00:22:41,491 --> 00:22:46,790 371 00:22:46,790 --> 00:22:49,220 So, we'll say foams for insulation are blown 372 00:22:49,220 --> 00:22:53,247 with low conductivity gases. 373 00:22:53,247 --> 00:22:58,100 374 00:22:58,100 --> 00:23:00,350 But as I mentioned, you have this problem with aging 375 00:23:00,350 --> 00:23:02,750 that, over time, that gas is going to diffuse out 376 00:23:02,750 --> 00:23:04,090 and air is going to diffuse in. 377 00:23:04,090 --> 00:23:21,810 378 00:23:21,810 --> 00:23:26,135 Then the overall thermal conductivity of the foam 379 00:23:26,135 --> 00:23:27,010 is going to increase. 380 00:23:27,010 --> 00:23:46,570 381 00:23:46,570 --> 00:23:50,190 So that's the conduction. 382 00:23:50,190 --> 00:23:54,580 And then the next contribution is from convection. 383 00:23:54,580 --> 00:23:59,150 So imagine we have one of our little cells here. 384 00:23:59,150 --> 00:24:03,260 And it's hotter on that side than it is on that side. 385 00:24:03,260 --> 00:24:06,050 And hot air is going to rise. 386 00:24:06,050 --> 00:24:07,430 Cold air is going to fall. 387 00:24:07,430 --> 00:24:10,380 So you get a convection current set up. 388 00:24:10,380 --> 00:24:13,160 And because of the density changes, 389 00:24:13,160 --> 00:24:16,320 you get a buoyancy force in the air. 390 00:24:16,320 --> 00:24:18,600 So that's kind of driving the convection. 391 00:24:18,600 --> 00:24:20,520 But you also have a viscous drag. 392 00:24:20,520 --> 00:24:24,580 So the air is moving past the wall of the foam. 393 00:24:24,580 --> 00:24:27,580 And there's going to be some viscous drag associated. 394 00:24:27,580 --> 00:24:29,320 And how much convection you can get 395 00:24:29,320 --> 00:24:31,740 depends on the balance between this buoyancy force 396 00:24:31,740 --> 00:24:32,815 and the viscous drag. 397 00:24:32,815 --> 00:24:37,700 398 00:24:37,700 --> 00:24:44,300 So we'll say the gas rises and falls 399 00:24:44,300 --> 00:24:46,080 due to density changes with temperature. 400 00:24:46,080 --> 00:24:54,871 401 00:24:54,871 --> 00:24:57,850 And the density changes give rise to buoyancy forces. 402 00:24:57,850 --> 00:25:08,750 403 00:25:08,750 --> 00:25:18,490 But we also have these viscous forces 404 00:25:18,490 --> 00:25:22,590 from the drag of the air against the walls of the cell. 405 00:25:22,590 --> 00:25:33,070 406 00:25:33,070 --> 00:25:35,700 So air moving past the walls-- this 407 00:25:35,700 --> 00:25:39,220 is kind of a fluid mechanics thing-- so that air is a fluid. 408 00:25:39,220 --> 00:25:41,340 And in fluid mechanics, they often 409 00:25:41,340 --> 00:25:42,894 use dimensionless numbers. 410 00:25:42,894 --> 00:25:44,310 And there's a dimensionless number 411 00:25:44,310 --> 00:25:45,524 called the Rayleigh number. 412 00:25:45,524 --> 00:25:47,440 And the Rayleigh number, you can think of it-- 413 00:25:47,440 --> 00:25:50,570 it's not quite the balance of the buoyancy force 414 00:25:50,570 --> 00:25:52,370 against the viscous forces. 415 00:25:52,370 --> 00:25:54,310 But it involves those forces. 416 00:25:54,310 --> 00:25:56,530 And convection is important if this Raleigh number's 417 00:25:56,530 --> 00:25:57,215 over 1,000. 418 00:25:57,215 --> 00:26:17,400 419 00:26:17,400 --> 00:26:19,211 And here's what the Rayleigh number is. 420 00:26:19,211 --> 00:26:22,150 421 00:26:22,150 --> 00:26:26,120 It's the density of the fluid times the acceleration 422 00:26:26,120 --> 00:26:28,810 of gravity times beta. 423 00:26:28,810 --> 00:26:30,880 Beta's the volume expansion coefficient 424 00:26:30,880 --> 00:26:34,284 for the gas-- times the temperature change. 425 00:26:34,284 --> 00:26:35,950 And we're going to look at a temperature 426 00:26:35,950 --> 00:26:38,200 change across a cell. 427 00:26:38,200 --> 00:26:39,480 And then, times the length. 428 00:26:39,480 --> 00:26:42,790 That's going to be the cell size. 429 00:26:42,790 --> 00:26:46,730 And we divide that by the fluid viscosity 430 00:26:46,730 --> 00:26:50,380 and the thermal diffusivity. 431 00:26:50,380 --> 00:26:52,910 So let me write down what all these things are. 432 00:26:52,910 --> 00:26:54,608 So rho is the density of the gas. 433 00:26:54,608 --> 00:26:58,910 434 00:26:58,910 --> 00:27:01,820 So the g's gravitational acceleration. 435 00:27:01,820 --> 00:27:09,170 436 00:27:09,170 --> 00:27:11,945 Beta is the volume expansion of the gas. 437 00:27:11,945 --> 00:27:23,010 438 00:27:23,010 --> 00:27:24,682 And for a constant pressure that's 439 00:27:24,682 --> 00:27:26,015 equal to 1 over the temperature. 440 00:27:26,015 --> 00:27:31,390 441 00:27:31,390 --> 00:27:35,460 Then delta tc is the temperature difference across a cell. 442 00:27:35,460 --> 00:27:43,090 443 00:27:43,090 --> 00:27:44,410 And l is the cell size. 444 00:27:44,410 --> 00:27:46,990 445 00:27:46,990 --> 00:27:51,815 Mu is the dynamics viscosity the fluid. 446 00:27:51,815 --> 00:27:55,610 447 00:27:55,610 --> 00:27:57,270 And a is our thermal diffusivity. 448 00:27:57,270 --> 00:28:06,680 449 00:28:06,680 --> 00:28:09,300 So what I'm going to do is just work out, 450 00:28:09,300 --> 00:28:16,450 for a typical example, how big of a cell size 451 00:28:16,450 --> 00:28:19,420 do you need to get this Rayleigh number to be 1,000. 452 00:28:19,420 --> 00:28:22,060 And we're going to see that, typically, 453 00:28:22,060 --> 00:28:23,830 that cell size is big. 454 00:28:23,830 --> 00:28:24,970 It's like 20 millimeters. 455 00:28:24,970 --> 00:28:26,660 So in most foams, the convection really 456 00:28:26,660 --> 00:28:27,970 isn't very important at all. 457 00:28:27,970 --> 00:28:30,510 So it's typically-- people don't worry about convection. 458 00:28:30,510 --> 00:28:32,500 And let me just show you how that works. 459 00:28:32,500 --> 00:28:53,540 460 00:28:53,540 --> 00:28:56,165 So for our Rayleigh number, which 461 00:28:56,165 --> 00:28:59,030 is ra-- for the Rayleigh number to be 1,000-- 462 00:28:59,030 --> 00:29:01,760 say we had air in the cells. 463 00:29:01,760 --> 00:29:04,095 And say the temperature was room temperature. 464 00:29:04,095 --> 00:29:07,670 465 00:29:07,670 --> 00:29:13,170 Then the volume coefficient of expansion is just 1 over t. 466 00:29:13,170 --> 00:29:16,150 So it's 1 over 300, say. 467 00:29:16,150 --> 00:29:18,670 degrees k to the minus 1. 468 00:29:18,670 --> 00:29:22,700 Let's say our change in temperature across one cell 469 00:29:22,700 --> 00:29:25,480 was 1 degree k. 470 00:29:25,480 --> 00:29:26,980 Bless you. 471 00:29:26,980 --> 00:29:32,400 The viscosity of air is 2 times 10 to the minus 5, 472 00:29:32,400 --> 00:29:34,280 pascal seconds. 473 00:29:34,280 --> 00:29:41,850 The density of air is 1.2 kilograms per cubic meter. 474 00:29:41,850 --> 00:29:45,680 475 00:29:45,680 --> 00:29:47,960 And the thermal diffusivity for air 476 00:29:47,960 --> 00:29:53,840 is 2 times 10 to the minus 5 meters squared per second. 477 00:29:53,840 --> 00:29:56,220 And if you plug all of these into that equation 478 00:29:56,220 --> 00:29:59,470 for the Rayleigh number and you solve for the cell size, 479 00:29:59,470 --> 00:30:04,280 you find that the cell size, l, is 20 millimeters. 480 00:30:04,280 --> 00:30:06,740 So that says convection is only important if the cell 481 00:30:06,740 --> 00:30:08,010 size is bigger than that. 482 00:30:08,010 --> 00:30:21,200 483 00:30:21,200 --> 00:30:23,752 And so most foams have cells much smaller than that. 484 00:30:23,752 --> 00:30:24,960 And convection is negligible. 485 00:30:24,960 --> 00:30:46,000 486 00:30:46,000 --> 00:30:48,420 So I have enclosed cells and the heat's 487 00:30:48,420 --> 00:30:50,770 not transferred so easily from one cell to another 488 00:30:50,770 --> 00:30:52,230 by the gas moving. 489 00:30:52,230 --> 00:30:55,280 And by having small cells the convection drops out. 490 00:30:55,280 --> 00:30:56,930 So you don't have to worry about that. 491 00:30:56,930 --> 00:31:00,705 So the last contribution to heat transfer is from radiation. 492 00:31:00,705 --> 00:31:10,960 493 00:31:10,960 --> 00:31:12,830 And there's something called Stefan's law 494 00:31:12,830 --> 00:31:16,490 that describes the heat flux for radiated heat 495 00:31:16,490 --> 00:31:18,920 transfer from a surface at one temperature 496 00:31:18,920 --> 00:31:21,110 to another surface at a different temperature 497 00:31:21,110 --> 00:31:22,990 across a vacuum. 498 00:31:22,990 --> 00:31:29,350 So we can say we have a heat flux 499 00:31:29,350 --> 00:31:34,484 qr not from a surface of one temperature. 500 00:31:34,484 --> 00:31:37,310 501 00:31:37,310 --> 00:31:41,180 So I'm going to call that t1-- to one at a lower temperature. 502 00:31:41,180 --> 00:31:47,090 503 00:31:47,090 --> 00:31:51,730 I'm going to call tnot-- with a vacuum in between them. 504 00:31:51,730 --> 00:32:03,340 505 00:32:03,340 --> 00:32:08,060 So this is [? Stefan's ?] law so this is the radiative heat 506 00:32:08,060 --> 00:32:13,850 flux is equal to the emissivity of the surfaces, which 507 00:32:13,850 --> 00:32:16,130 is beta 1 times a constant called 508 00:32:16,130 --> 00:32:21,460 Stefan's constant-- sigma times the fourth power 509 00:32:21,460 --> 00:32:24,800 of temperatures. 510 00:32:24,800 --> 00:32:32,830 I'm taking the difference of the temperatures 511 00:32:32,830 --> 00:32:37,874 so here are the Stefan's Constant-- is sigma. 512 00:32:37,874 --> 00:32:41,750 513 00:32:41,750 --> 00:32:48,760 And that's equal to 5.67 times the 10 to the minus 8. 514 00:32:48,760 --> 00:32:54,740 And that's in watts per meter squared per k to the fourth. 515 00:32:54,740 --> 00:32:58,770 And beta is a constant describing 516 00:32:58,770 --> 00:33:00,260 the emissivity of the surfaces. 517 00:33:00,260 --> 00:33:18,980 518 00:33:18,980 --> 00:33:21,480 So it gives the radiant heat flux 519 00:33:21,480 --> 00:33:24,244 per unit area of the sample relative to a black body. 520 00:33:24,244 --> 00:33:26,160 And that's a characteristic of the emissivity. 521 00:33:26,160 --> 00:33:29,830 522 00:33:29,830 --> 00:33:33,599 All right, so then, so if we-- yes? 523 00:33:33,599 --> 00:33:34,432 STUDENT: [INAUDIBLE] 524 00:33:34,432 --> 00:33:37,932 525 00:33:37,932 --> 00:33:39,890 PROFESSOR: Now-- so right now, forget the foam. 526 00:33:39,890 --> 00:33:40,540 We have no foam. 527 00:33:40,540 --> 00:33:42,748 We just have two surfaces with a vacuum between them. 528 00:33:42,748 --> 00:33:45,140 And now I'm going to stick a foam between the surfaces. 529 00:33:45,140 --> 00:33:48,320 And we're going to see how that changes the heat flux, OK? 530 00:33:48,320 --> 00:33:50,680 So the next step is we put the foam between those two 531 00:33:50,680 --> 00:33:51,604 surfaces. 532 00:33:51,604 --> 00:33:53,270 And the heat flux is going to be reduced 533 00:33:53,270 --> 00:33:55,686 because the radiation is going to be absorbed by the solid 534 00:33:55,686 --> 00:33:57,560 and reflected by the cell walls. 535 00:33:57,560 --> 00:33:59,040 And so we're going to characterize 536 00:33:59,040 --> 00:34:00,090 how much it's reduced. 537 00:34:00,090 --> 00:34:03,440 So there's another law called Beer's Law, which characterizes 538 00:34:03,440 --> 00:34:07,736 the reduction in the heat flux. 539 00:34:07,736 --> 00:34:39,239 540 00:34:39,239 --> 00:34:41,480 Piece of chalk's getting to small 541 00:34:41,480 --> 00:35:34,550 542 00:35:34,550 --> 00:35:38,810 OK, so Beer's Law gives us the attenuation, so the sort 543 00:35:38,810 --> 00:35:42,510 of reduction in the heat flow. 544 00:35:42,510 --> 00:35:45,990 So qr is equal to qr not. 545 00:35:45,990 --> 00:35:49,100 That would be the heat flux, if we just had the vacuum. 546 00:35:49,100 --> 00:35:51,530 And then there's an exponential law. 547 00:35:51,530 --> 00:35:56,630 And it's the exponential of minus k star t star. 548 00:35:56,630 --> 00:35:59,050 And here, k stars in an extinction coefficient 549 00:35:59,050 --> 00:36:00,254 for the foam. 550 00:36:00,254 --> 00:36:02,170 Talk a little bit more about that in a minute. 551 00:36:02,170 --> 00:36:10,090 552 00:36:10,090 --> 00:36:12,200 and t star is just the thickness of the foam. 553 00:36:12,200 --> 00:36:18,970 554 00:36:18,970 --> 00:36:20,758 And then this thing is called Beer's Law. 555 00:36:20,758 --> 00:36:28,800 556 00:36:28,800 --> 00:36:31,120 So we have very thin walls and struts. 557 00:36:31,120 --> 00:36:33,890 And we're just going to consider optically thin walls and struts 558 00:36:33,890 --> 00:36:35,070 to make life easy. 559 00:36:35,070 --> 00:36:37,070 Then we can say that, if they're optically thin, 560 00:36:37,070 --> 00:36:38,906 they're transparent to radiation. 561 00:36:38,906 --> 00:36:40,280 They're optically thin if they're 562 00:36:40,280 --> 00:36:42,170 less than about 10 microns. 563 00:36:42,170 --> 00:36:44,950 Then this extinction coefficient is just the amount 564 00:36:44,950 --> 00:36:47,420 of solid times the extension coefficient for the solids. 565 00:36:47,420 --> 00:36:49,670 So it's just the relative density times the extinction 566 00:36:49,670 --> 00:36:50,936 coefficient for the solid. 567 00:36:50,936 --> 00:37:20,500 568 00:37:20,500 --> 00:37:25,390 OK, and then I can say, the heat flux by radiation. 569 00:37:25,390 --> 00:37:28,320 570 00:37:28,320 --> 00:37:31,148 I can use two equations to write that down now. 571 00:37:31,148 --> 00:37:34,890 572 00:37:34,890 --> 00:37:37,060 And then I'm going to let them be equal to get 573 00:37:37,060 --> 00:37:38,870 the thermal conductivity. 574 00:37:38,870 --> 00:37:44,920 I can say qr is going equal to lambda r times dt by dx. 575 00:37:44,920 --> 00:37:49,800 So that's the Fourier's Law that we started out with. 576 00:37:49,800 --> 00:37:52,160 And then I've also got the qr that I'm 577 00:37:52,160 --> 00:37:55,780 going to get by combining the Stefan's Law with the Beer's 578 00:37:55,780 --> 00:37:57,440 Law up there. 579 00:37:57,440 --> 00:38:00,130 So if I do that, I get that qr is beta 580 00:38:00,130 --> 00:38:09,630 1 times sigma times t1 to the fourth minus t not the fourth. 581 00:38:09,630 --> 00:38:14,730 So that's the qr not up there from down there. 582 00:38:14,730 --> 00:38:18,370 And then I've got an exponential for the attenuation. 583 00:38:18,370 --> 00:38:21,500 And instead of k star, I'm going to put the relative density 584 00:38:21,500 --> 00:38:22,268 of times ks. 585 00:38:22,268 --> 00:38:27,610 586 00:38:27,610 --> 00:38:32,330 and then I've got the thickness of the foam, t star, as well. 587 00:38:32,330 --> 00:38:39,900 OK, so that's qr, but that has to equal lambda times dt by dx. 588 00:38:39,900 --> 00:38:44,700 589 00:38:44,700 --> 00:38:46,402 So I'm going to use some approximations. 590 00:38:46,402 --> 00:38:48,360 Here and I'm going to end up with an expression 591 00:38:48,360 --> 00:38:51,162 for the contribution from radiation 592 00:38:51,162 --> 00:38:52,370 to heat transfer in the foam. 593 00:38:52,370 --> 00:38:53,134 Yeah? 594 00:38:53,134 --> 00:38:55,300 STUDENT: So when you say optically thin walls, where 595 00:38:55,300 --> 00:38:57,050 t is less than 10 microns, you mean 596 00:38:57,050 --> 00:38:59,585 like the walls of the foam? 597 00:38:59,585 --> 00:39:00,460 PROFESSOR: Yeah, yea. 598 00:39:00,460 --> 00:39:02,774 STUDENT: So it's different t than the-- 599 00:39:02,774 --> 00:39:04,190 PROFESSOR: t star is the thickness 600 00:39:04,190 --> 00:39:05,850 of the whole thing, yeah. 601 00:39:05,850 --> 00:39:07,800 So imagine we had our two surfaces. 602 00:39:07,800 --> 00:39:10,320 And they might be like 100 millimeters apart 603 00:39:10,320 --> 00:39:12,650 or something. t star is the sort of thickness 604 00:39:12,650 --> 00:39:15,170 of the foam in between the two surfaces. 605 00:39:15,170 --> 00:39:18,250 And the optically thin is the cell walls, which 606 00:39:18,250 --> 00:39:21,687 are microns kind of thickness. 607 00:39:21,687 --> 00:39:22,186 OK. 608 00:39:22,186 --> 00:39:30,570 609 00:39:30,570 --> 00:39:32,840 So I'm going to make some approximations here. 610 00:39:32,840 --> 00:39:36,560 611 00:39:36,560 --> 00:39:39,140 And that's going to allow me to solve for t star. 612 00:39:39,140 --> 00:39:43,060 So I'm going to say that dt by dx 613 00:39:43,060 --> 00:39:47,100 x is approximately equal to just t1 minus t 614 00:39:47,100 --> 00:39:51,570 not over the thickness of the foam 615 00:39:51,570 --> 00:39:58,220 or I'll call that delta t over t star. 616 00:39:58,220 --> 00:40:00,440 And then, the other approximation I'm going to use 617 00:40:00,440 --> 00:40:05,420 is that t1 to the 4th minus t not to the fourth 618 00:40:05,420 --> 00:40:10,860 is equal to 4 times delta t times 619 00:40:10,860 --> 00:40:13,240 the average temperature cubed. 620 00:40:13,240 --> 00:40:18,350 So here t bar is the average temperature, t1 plus t 621 00:40:18,350 --> 00:40:19,090 not over 2. 622 00:40:19,090 --> 00:40:44,070 623 00:40:44,070 --> 00:40:47,220 So then, if I use those two approximations, 624 00:40:47,220 --> 00:40:52,470 I can write that qr, our heat flux from radiative transfer. 625 00:40:52,470 --> 00:40:53,500 I got the beta 1. 626 00:40:53,500 --> 00:40:54,710 I've got the sigma. 627 00:40:54,710 --> 00:40:59,280 And instead of the difference of the fourth power, 628 00:40:59,280 --> 00:41:05,250 I'm going to write 4 delta t t bar cubed. 629 00:41:05,250 --> 00:41:06,675 And then I've got my exponential. 630 00:41:06,675 --> 00:41:09,780 631 00:41:09,780 --> 00:41:12,130 Blah, blah, blah, blah, blah. 632 00:41:12,130 --> 00:41:17,990 So then, here's the relative density times ks times 633 00:41:17,990 --> 00:41:20,780 t star, the overall thickness. 634 00:41:20,780 --> 00:41:23,720 That's going to equal the radiative contribution 635 00:41:23,720 --> 00:41:26,300 to the thermal conductivity of the foam. 636 00:41:26,300 --> 00:41:29,230 And instead of dt by dx, I'm going 637 00:41:29,230 --> 00:41:34,160 to have delta t over t star here. 638 00:41:34,160 --> 00:41:35,940 So part of the reason for doing these 639 00:41:35,940 --> 00:41:40,490 approximations I end up with a delta t term on both sides. 640 00:41:40,490 --> 00:41:42,150 Now I can cancel that out. 641 00:41:42,150 --> 00:41:45,540 And if I just take this mess here and multiply it by t star, 642 00:41:45,540 --> 00:41:47,670 then I've got lambda r star. 643 00:41:47,670 --> 00:42:03,560 644 00:42:03,560 --> 00:42:08,790 That's our thermal conductivity contribution from radiation. 645 00:42:08,790 --> 00:42:10,840 So one of the things to notice here 646 00:42:10,840 --> 00:42:15,820 is that, as the relative density goes down, 647 00:42:15,820 --> 00:42:19,690 then the contribution from radiation 648 00:42:19,690 --> 00:42:22,802 to the thermal conductivity of the foam goes up. 649 00:42:22,802 --> 00:42:49,920 650 00:42:49,920 --> 00:42:53,900 OK, so this chart here shows thermal conductivity 651 00:42:53,900 --> 00:42:55,330 as a function of relative density. 652 00:42:55,330 --> 00:42:56,830 And it breaks down the contributions 653 00:42:56,830 --> 00:43:00,770 from the gas, g, the solid, s, and the radiation, r. 654 00:43:00,770 --> 00:43:03,070 And you kind of see the gas contribution 655 00:43:03,070 --> 00:43:04,230 doesn't change that much. 656 00:43:04,230 --> 00:43:06,790 These are relative densities between a little over 2 657 00:43:06,790 --> 00:43:08,330 and a little less than 5%. 658 00:43:08,330 --> 00:43:10,570 So the amount of gas-- it's mostly 659 00:43:10,570 --> 00:43:14,050 gas in all of these things. 660 00:43:14,050 --> 00:43:18,670 The solid contribution increases as the relative density 661 00:43:18,670 --> 00:43:19,260 increases. 662 00:43:19,260 --> 00:43:21,670 So you'd expect that. 663 00:43:21,670 --> 00:43:26,030 And then, as I just said, as the relative density goes down, 664 00:43:26,030 --> 00:43:30,030 the amount of radiation contribution goes up. 665 00:43:30,030 --> 00:43:32,800 And so you can kind of see how that all fits together. 666 00:43:32,800 --> 00:43:35,654 Another plot that shows the thermal conductivity 667 00:43:35,654 --> 00:43:36,820 versus the relative density. 668 00:43:36,820 --> 00:43:39,590 These are for a few different types of foams. 669 00:43:39,590 --> 00:43:42,450 You can see for this plot here, you 670 00:43:42,450 --> 00:43:45,067 reach a minimum in the thermal conductivity. 671 00:43:45,067 --> 00:43:46,900 And that's because you've got this trade off 672 00:43:46,900 --> 00:43:49,399 between the contribution from the solid and the contribution 673 00:43:49,399 --> 00:43:50,760 from the radiation. 674 00:43:50,760 --> 00:43:54,750 And those two kind of trade off and you get to a minimum. 675 00:43:54,750 --> 00:43:56,545 So let me write some of this down. 676 00:43:56,545 --> 00:43:59,950 677 00:43:59,950 --> 00:44:03,968 So I'll just say that-- hang on. 678 00:44:03,968 --> 00:44:05,610 Write this over again. 679 00:44:05,610 --> 00:44:13,897 680 00:44:13,897 --> 00:44:16,063 This is looking at the overall thermal conductivity. 681 00:44:16,063 --> 00:44:19,600 682 00:44:19,600 --> 00:44:24,650 And we can see the relative contributions 683 00:44:24,650 --> 00:44:30,180 of lambda, solid, lambda, gas, lambda, radiation. 684 00:44:30,180 --> 00:44:31,942 I'll just say this shown in the figure. 685 00:44:31,942 --> 00:44:38,490 686 00:44:38,490 --> 00:44:49,389 I'm going to say the next figure shows a minimum 687 00:44:49,389 --> 00:44:50,555 in the thermal conductivity. 688 00:44:50,555 --> 00:44:53,990 689 00:44:53,990 --> 00:45:00,630 Then I'll just say there's a trade off 690 00:45:00,630 --> 00:45:03,300 between the conduction through the solid 691 00:45:03,300 --> 00:45:05,593 and I can direction from the radiation. 692 00:45:05,593 --> 00:45:10,610 693 00:45:10,610 --> 00:45:12,640 And then we also have a plot here 694 00:45:12,640 --> 00:45:16,637 that shows the conductivity versus the cell size. 695 00:45:16,637 --> 00:45:27,620 696 00:45:27,620 --> 00:45:30,710 And you can see that the conductivity increases 697 00:45:30,710 --> 00:45:31,775 with cell size. 698 00:45:31,775 --> 00:45:39,580 699 00:45:39,580 --> 00:45:41,960 And the reason for that is the bigger the cells get, 700 00:45:41,960 --> 00:45:45,040 the radiation is reflected less often. 701 00:45:45,040 --> 00:45:58,120 702 00:45:58,120 --> 00:46:04,800 And one thing I wanted to mention with the cell size 703 00:46:04,800 --> 00:46:08,920 is that if you look at aerogels, the way aerogels shells work 704 00:46:08,920 --> 00:46:11,790 is that they have a very small cell size, a very small pore 705 00:46:11,790 --> 00:46:12,610 size. 706 00:46:12,610 --> 00:46:15,200 So typically, it's less than 100 nanometers. 707 00:46:15,200 --> 00:46:20,230 And the mean free path of air is 68 nanometers. 708 00:46:20,230 --> 00:46:22,140 So the mean free path is the average distance 709 00:46:22,140 --> 00:46:25,400 the molecules move before they collide with another molecule. 710 00:46:25,400 --> 00:46:29,130 And if your pore size is less than the mean free path, 711 00:46:29,130 --> 00:46:32,360 then that reduces the thermal conductivity. 712 00:46:32,360 --> 00:46:34,200 It reduces the ability of the atoms 713 00:46:34,200 --> 00:46:37,810 to pass the heat along between one another. 714 00:46:37,810 --> 00:46:39,310 So the way the aerogels work is they 715 00:46:39,310 --> 00:46:40,830 have a very small pore size. 716 00:46:40,830 --> 00:46:46,690 717 00:46:46,690 --> 00:46:49,120 And what's important is how big the pores 718 00:46:49,120 --> 00:46:50,900 are relative to the mean free path of air. 719 00:46:50,900 --> 00:48:04,380 720 00:48:04,380 --> 00:48:06,790 OK, so that's the thermal conductivity. 721 00:48:06,790 --> 00:48:09,820 I wanted to talk about a few other thermal properties 722 00:48:09,820 --> 00:48:11,205 of foams, as well, today. 723 00:48:11,205 --> 00:48:43,100 724 00:48:43,100 --> 00:48:45,100 So one is the specific heat. 725 00:48:45,100 --> 00:48:47,760 And since the specific heat is the energy required 726 00:48:47,760 --> 00:48:51,990 to raise the temperature by a unit mass, 727 00:48:51,990 --> 00:48:57,794 then the mass is the same-- you know, 728 00:48:57,794 --> 00:48:59,210 if you have a certain mass of foam 729 00:48:59,210 --> 00:49:01,440 or a certain mass of solid-- the specific heat from the foam 730 00:49:01,440 --> 00:49:02,481 is the same as the solid. 731 00:49:02,481 --> 00:49:32,390 732 00:49:32,390 --> 00:49:36,030 So the specific heat for the foam 733 00:49:36,030 --> 00:49:40,080 is the same as the specific heat for the solid. 734 00:49:40,080 --> 00:49:41,680 So that would have units of joules 735 00:49:41,680 --> 00:49:43,610 per kilogram per degree k. 736 00:49:43,610 --> 00:49:48,560 737 00:49:48,560 --> 00:49:51,490 And the next property is the thermal expansion coefficient. 738 00:49:51,490 --> 00:50:02,380 739 00:50:02,380 --> 00:50:03,460 And it's a similar thing. 740 00:50:03,460 --> 00:50:06,150 The thermal expansion coefficient for the foam 741 00:50:06,150 --> 00:50:07,850 is equal to the thermal coefficient 742 00:50:07,850 --> 00:50:10,840 of expansion for the solid. 743 00:50:10,840 --> 00:50:14,250 So imagine you have-- say you had something like a honeycomb. 744 00:50:14,250 --> 00:50:15,910 If you heat it up a certain amount, 745 00:50:15,910 --> 00:50:17,879 every member is going to expand by alpha. 746 00:50:17,879 --> 00:50:19,420 And if every member expands by alpha, 747 00:50:19,420 --> 00:50:20,794 the whole thing expands by alpha. 748 00:50:20,794 --> 00:50:22,460 And this is the same. 749 00:50:22,460 --> 00:50:24,090 And it's the same idea with the foam. 750 00:50:24,090 --> 00:50:26,590 So if every member just gets longer by alpha, 751 00:50:26,590 --> 00:50:28,340 then the whole thing gets bigger by alpha. 752 00:50:28,340 --> 00:50:44,010 753 00:50:44,010 --> 00:50:46,730 OK, so the last topic I wanted to talk about 754 00:50:46,730 --> 00:50:48,612 was the thermal shock resistance. 755 00:50:48,612 --> 00:50:51,070 And thermal shock is the idea is that if you have something 756 00:50:51,070 --> 00:50:54,140 that's hot, and say you quench it in a liquid-- 757 00:50:54,140 --> 00:50:56,220 so you put it suddenly in a liquid-- 758 00:50:56,220 --> 00:50:57,630 the surface is going to cool down 759 00:50:57,630 --> 00:50:59,560 faster than the bulk of it. 760 00:50:59,560 --> 00:51:00,970 And because the surface is trying 761 00:51:00,970 --> 00:51:02,785 to contract because it's cooling down, 762 00:51:02,785 --> 00:51:05,160 but it's attached to the bulk of it and it's constrained, 763 00:51:05,160 --> 00:51:08,692 it can't really cool down, then you generate stresses. 764 00:51:08,692 --> 00:51:10,150 And if the stresses are big enough, 765 00:51:10,150 --> 00:51:12,566 you can cause fracture and have the thing crack and spall. 766 00:51:12,566 --> 00:51:17,530 767 00:51:17,530 --> 00:51:20,340 So we'll say if the materials is subjected 768 00:51:20,340 --> 00:51:34,880 to a sudden change in the surface temperature, that 769 00:51:34,880 --> 00:51:37,060 induces thermal stresses at the surface 770 00:51:37,060 --> 00:51:39,080 and can induce spalling and cracking. 771 00:51:39,080 --> 00:52:00,642 772 00:52:00,642 --> 00:52:03,100 So we're going to think about a material at one temperature 773 00:52:03,100 --> 00:52:04,570 that's dropped into, say, a liquid 774 00:52:04,570 --> 00:52:05,695 at a different temperature. 775 00:52:05,695 --> 00:52:27,912 776 00:52:27,912 --> 00:52:29,370 So the surface temperature is going 777 00:52:29,370 --> 00:52:31,564 to drop to the cooler liquid temperature 778 00:52:31,564 --> 00:52:33,480 and it's going to contract the surface layers. 779 00:52:33,480 --> 00:52:52,560 780 00:52:52,560 --> 00:52:55,510 And the fact that they're bound to the layers underneath that 781 00:52:55,510 --> 00:52:57,710 are not contracting as quickly, it 782 00:52:57,710 --> 00:53:00,860 means that you generate a thermal strain. 783 00:53:00,860 --> 00:53:11,821 784 00:53:11,821 --> 00:53:13,320 So the thermal strain is going to be 785 00:53:13,320 --> 00:53:15,904 the coefficient of thermal expansion times the change 786 00:53:15,904 --> 00:53:16,528 in temperature. 787 00:53:16,528 --> 00:53:52,300 788 00:53:52,300 --> 00:53:54,560 So you're going to constrain the surface 789 00:53:54,560 --> 00:53:56,300 to the original dimensions. 790 00:53:56,300 --> 00:53:58,105 And then you're going to induce the stress. 791 00:53:58,105 --> 00:54:19,450 792 00:54:19,450 --> 00:54:23,310 So if it's a plane or thing, it's e alpha delta t. 793 00:54:23,310 --> 00:54:25,970 And then, there's a factor of 1 minus nu, 794 00:54:25,970 --> 00:54:29,850 just because it's a plane, in a plane. 795 00:54:29,850 --> 00:54:31,590 And then you'll get cracking or spalling 796 00:54:31,590 --> 00:54:34,210 when that stress equals some failure, stress. 797 00:54:34,210 --> 00:54:43,120 798 00:54:43,120 --> 00:54:47,490 So I can rearrange this and solve for the critical delta t 799 00:54:47,490 --> 00:54:50,580 that you can withstand without getting cracking. 800 00:54:50,580 --> 00:54:54,106 So I just rearranged this and say sigma's equal to sigma f. 801 00:54:54,106 --> 00:55:00,600 That would be sigma f times 1 minus nu over e and over alpha. 802 00:55:00,600 --> 00:55:02,450 So that's the critical change in temperature 803 00:55:02,450 --> 00:55:03,660 to just cause cracking. 804 00:55:03,660 --> 00:55:13,210 805 00:55:13,210 --> 00:55:15,864 So now what I can do is I can substitute in there for what 806 00:55:15,864 --> 00:55:17,030 you would have for the foam. 807 00:55:17,030 --> 00:55:20,294 808 00:55:20,294 --> 00:55:22,210 And I'm going to do it just for the open cells 809 00:55:22,210 --> 00:55:24,210 just because it's easier to write the equations. 810 00:55:24,210 --> 00:55:27,580 811 00:55:27,580 --> 00:55:32,230 So for the foam, I would have some sort of fracture strength. 812 00:55:32,230 --> 00:55:34,180 So when we did the modeling of the foams, 813 00:55:34,180 --> 00:55:37,140 we said that was equal to about 0.2 times the modulus 814 00:55:37,140 --> 00:55:42,980 of rupture times the relative density to the 3/2's power 815 00:55:42,980 --> 00:55:46,730 and 1 minus nu. 816 00:55:46,730 --> 00:55:49,460 And if I divide by the modulus of the foam, 817 00:55:49,460 --> 00:55:54,460 that's es times the relative density squared. 818 00:55:54,460 --> 00:55:57,150 And then we just had alpha for the foam 819 00:55:57,150 --> 00:55:58,575 was the same as alpha s. 820 00:55:58,575 --> 00:56:01,130 821 00:56:01,130 --> 00:56:03,760 So then, I can rearrange this slightly 822 00:56:03,760 --> 00:56:07,640 and say it's equal to 0.2 over the relative density 823 00:56:07,640 --> 00:56:09,240 to the 1/2 power. 824 00:56:09,240 --> 00:56:12,950 So I'm canceling out these relative densities here. 825 00:56:12,950 --> 00:56:17,431 And then I can combine all the solid properties together. 826 00:56:17,431 --> 00:56:19,180 And I'm going to say that nu for the solid 827 00:56:19,180 --> 00:56:21,263 is about equal to the same as nu for the foam. 828 00:56:21,263 --> 00:56:34,650 829 00:56:34,650 --> 00:56:37,951 So what I can do here is I can group all the solid properties 830 00:56:37,951 --> 00:56:38,450 together. 831 00:56:38,450 --> 00:56:41,880 And this just is delta t critical for the solid, right? 832 00:56:41,880 --> 00:56:45,930 So this is saying that the critical temperature range 833 00:56:45,930 --> 00:56:48,890 before you get cracking in the foam 834 00:56:48,890 --> 00:56:52,050 is equal to the range for the solid, 835 00:56:52,050 --> 00:56:54,879 but multiplied by this factor of 0.2 836 00:56:54,879 --> 00:56:57,170 and divided by the square root of the relative density. 837 00:56:57,170 --> 00:56:58,919 So if the square of-- the relative density 838 00:56:58,919 --> 00:56:59,959 is going to less than 1. 839 00:56:59,959 --> 00:57:02,000 So this number here is going to be bigger than 1. 840 00:57:02,000 --> 00:57:04,830 So it's saying that the temperature range that 841 00:57:04,830 --> 00:57:06,700 will give you spalling in the foam 842 00:57:06,700 --> 00:57:09,780 is going to be bigger than the temperature range in the solid. 843 00:57:09,780 --> 00:57:14,440 So the foam's going to be better than the solid, OK? 844 00:57:14,440 --> 00:57:16,420 And that uses our little models from before. 845 00:57:16,420 --> 00:57:21,217 846 00:57:21,217 --> 00:57:23,050 So I think I'm going to stop there, probably 847 00:57:23,050 --> 00:57:27,030 cause my throat is starting to get too sore. 848 00:57:27,030 --> 00:57:29,370 There's a little case study in the notes. 849 00:57:29,370 --> 00:57:31,770 And I'll just put that on the notes on the Stellar site. 850 00:57:31,770 --> 00:57:34,130 It's like one page and it's really straightforward. 851 00:57:34,130 --> 00:57:36,171 You can just read that, OK? 852 00:57:36,171 --> 00:57:38,420 So this is the end of the bit on thermal conductivity. 853 00:57:38,420 --> 00:57:40,530 That's just this one lecture. 854 00:57:40,530 --> 00:57:43,200 And this is really the end of the whole section 855 00:57:43,200 --> 00:57:45,300 on modeling of the honey combs and the foams. 856 00:57:45,300 --> 00:57:47,633 So that's kind of the first half of the term is modeling 857 00:57:47,633 --> 00:57:49,317 the honey combs and the foams. 858 00:57:49,317 --> 00:57:50,900 And the second half of the term, we're 859 00:57:50,900 --> 00:57:53,850 kind of applying those models to different situations. 860 00:57:53,850 --> 00:57:56,720 So next week, we'll have the review on Monday, 861 00:57:56,720 --> 00:57:59,730 have a test on Wednesday, week after that is Spring break. 862 00:57:59,730 --> 00:58:02,339 I can't believe we're at Spring break already. 863 00:58:02,339 --> 00:58:04,630 And then after that we'll start we'll do the trabecular 864 00:58:04,630 --> 00:58:05,850 bone for a week. 865 00:58:05,850 --> 00:58:08,670 We'll do tissue engineering scaffolds and cell mechanics 866 00:58:08,670 --> 00:58:10,490 for two or three lectures. 867 00:58:10,490 --> 00:58:12,830 We'll look at some other applications 868 00:58:12,830 --> 00:58:15,910 to engineering design, look at energy absorption and sandwich 869 00:58:15,910 --> 00:58:16,880 panels. 870 00:58:16,880 --> 00:58:19,088 And then, I'm going to talk about plants a little bit 871 00:58:19,088 --> 00:58:19,970 at the very end, OK? 872 00:58:19,970 --> 00:58:23,200 So we've already covered a lot of the kind of deriving 873 00:58:23,200 --> 00:58:24,910 equations part of the course. 874 00:58:24,910 --> 00:58:27,340 The rest of the course is more applying the equations 875 00:58:27,340 --> 00:58:29,894 to lots of different situations, OK? 876 00:58:29,894 --> 00:58:32,060 So I'm going to stop there just because my throat is 877 00:58:32,060 --> 00:58:33,860 giving out. 878 00:58:33,860 --> 00:58:37,706