WEBVTT 00:00:00.320 --> 00:00:01.880 - [Voiceover] So let's think a little bit about the 00:00:01.880 --> 00:00:04.130 Maxwell-Boltzmann distribution. 00:00:04.130 --> 00:00:05.360 And this right over here, this is 00:00:05.360 --> 00:00:07.540 a picture of James Clerk Maxwell. 00:00:07.540 --> 00:00:09.140 And I really like this picture, it's with his 00:00:09.140 --> 00:00:12.430 wife Katherine Maxwell and I guess this is their dog. 00:00:12.430 --> 00:00:15.800 And James Maxwell, he is a titan of physics 00:00:15.800 --> 00:00:17.550 famous for Maxwell's equations. 00:00:17.550 --> 00:00:19.550 He also did some of the foundational work 00:00:19.550 --> 00:00:22.030 on color photography and he was involved in 00:00:22.030 --> 00:00:23.720 thinking about, "Well, what's the distribution 00:00:23.720 --> 00:00:26.520 of speeds of air particles 00:00:26.520 --> 00:00:29.020 of idealized gas particles?" 00:00:29.020 --> 00:00:32.420 And this gentleman over here, this is Ludwig Boltzmann. 00:00:32.420 --> 00:00:34.960 And he's considered the father or one 00:00:34.960 --> 00:00:37.880 of the founding fathers of statistical mechanics. 00:00:37.880 --> 00:00:41.360 And together, through the Maxwell-Boltzman distribution 00:00:41.360 --> 00:00:42.480 they didn't collaborate, but they 00:00:42.480 --> 00:00:44.530 independently came to the same distribution. 00:00:44.530 --> 00:00:46.490 They were able to describe, "Well, what's the 00:00:46.490 --> 00:00:50.737 distribution of the speeds of air particles?" 00:00:50.737 --> 00:00:52.290 So let's back up a little bit or let's just 00:00:52.290 --> 00:00:54.100 do a little bit of a thought experiment. 00:00:54.100 --> 00:00:56.900 So let's say that I have a container here. 00:00:57.420 --> 00:00:59.240 Let's say that I have a container here. 00:00:59.240 --> 00:01:00.880 And let's say it has air. 00:01:01.290 --> 00:01:03.720 And air is actually made up mostly of nitrogen. 00:01:03.720 --> 00:01:05.350 Let's just say it just has only nitrogen in it 00:01:05.350 --> 00:01:06.778 just to simplify things. 00:01:06.778 --> 00:01:10.844 So let me just draw some nitrogen molecules in there. 00:01:10.844 --> 00:01:13.558 And let's say that I have a thermometer. 00:01:13.558 --> 00:01:15.590 I put a thermometer in there. 00:01:15.590 --> 00:01:19.936 And the thermometer 00:01:20.320 --> 00:01:23.810 reads a temperature of 300 Kelvin. 00:01:24.190 --> 00:01:27.320 What does this temperature of 300 Kelvin mean? 00:01:27.660 --> 00:01:29.510 Well, in our everyday life, we have 00:01:29.510 --> 00:01:31.730 kind of a visceral sense of temperature. 00:01:31.730 --> 00:01:33.200 Hey, I don't wanna touch something that's hot. 00:01:33.200 --> 00:01:34.630 It's going to burn me. 00:01:34.630 --> 00:01:38.650 Or that cold thing, it's gonna make me shiver. 00:01:38.650 --> 00:01:40.080 And that's how our brain 00:01:40.080 --> 00:01:42.300 processes this thing called temperature. 00:01:42.300 --> 00:01:45.760 But what's actually going on at a molecular scale? 00:01:45.760 --> 00:01:47.630 Well, temperature, one way to think 00:01:47.630 --> 00:01:49.420 about temperature, this would be a very 00:01:49.420 --> 00:01:51.530 accurate way to think about temperature 00:01:51.530 --> 00:01:52.750 is that tempera- 00:01:52.750 --> 00:01:54.140 I'm spelling it wrong. 00:01:55.270 --> 00:01:59.480 Temperature is proportional to average kinetic energy 00:01:59.480 --> 00:02:02.919 of the molecules in that system. 00:02:02.919 --> 00:02:03.900 So let me write it this way. 00:02:03.900 --> 00:02:08.636 Temperature is proportional to average kinetic energy. 00:02:08.636 --> 00:02:09.850 Average 00:02:10.430 --> 00:02:13.110 kinetic 00:02:13.110 --> 00:02:15.740 energy 00:02:15.740 --> 00:02:16.720 in the system. 00:02:18.010 --> 00:02:19.600 I'll just write average kinetic energy. 00:02:19.600 --> 00:02:21.952 So let's make that a little bit more concrete. 00:02:21.952 --> 00:02:25.810 So let's say that I have two containers. 00:02:25.810 --> 00:02:27.297 So it's one container. 00:02:27.297 --> 00:02:28.364 Whoops. 00:02:28.364 --> 00:02:31.480 And two containers right over here. 00:02:31.480 --> 00:02:33.240 And let's say they have the same 00:02:33.240 --> 00:02:36.060 number of molecules of nitrogen gas 00:02:36.060 --> 00:02:37.440 And I'm just gonna draw 10 here. 00:02:37.440 --> 00:02:38.830 This obviously is not realistic 00:02:38.830 --> 00:02:40.350 you'd have many, many more molecules. 00:02:40.350 --> 00:02:45.350 One, two, three, four, five, six, seven, eight, nine, ten. 00:02:45.648 --> 00:02:50.640 One, two, three, four, five, six, seven, eight, nine, ten. 00:02:51.030 --> 00:02:52.760 And let's say we know that the 00:02:52.760 --> 00:02:55.210 temperature here is 300 Kelvin. 00:02:56.440 --> 00:02:58.940 So the temperature of this system is 300 Kelvin. 00:02:58.940 --> 00:03:01.500 And the temperature of this system is 200 Kelvin. 00:03:02.040 --> 00:03:05.900 So if I wanted to visualize what these molecules are doing 00:03:05.900 --> 00:03:07.450 they're all moving around, they're bumping 00:03:07.450 --> 00:03:10.200 they don't all move together in unison. 00:03:10.540 --> 00:03:12.810 The average kinetic energy of the molecules 00:03:12.810 --> 00:03:15.010 in this system is going to be higher. 00:03:15.010 --> 00:03:16.440 And so maybe you have 00:03:16.440 --> 00:03:18.965 this molecule is moving in that direction. 00:03:18.965 --> 00:03:20.830 So that's its velocity. 00:03:20.830 --> 00:03:22.610 This one has this velocity. 00:03:22.610 --> 00:03:23.770 This one's going there. 00:03:23.770 --> 00:03:25.800 This one might not be moving much at all. 00:03:25.800 --> 00:03:28.100 This one might be going really fast that way. 00:03:28.100 --> 00:03:30.340 This one might be going super fast that way. 00:03:30.340 --> 00:03:32.040 This is doing that. 00:03:32.270 --> 00:03:33.416 This is doing that. 00:03:33.712 --> 00:03:35.130 This is doing that. 00:03:35.132 --> 00:03:37.200 So if you were to now compare it to this system 00:03:37.200 --> 00:03:40.750 this system, you could still have a molecule 00:03:40.750 --> 00:03:41.800 that is going really fast. 00:03:41.800 --> 00:03:43.060 Maybe this molecule is going faster 00:03:43.060 --> 00:03:44.800 than any of the molecules over here. 00:03:44.800 --> 00:03:46.840 But on average, the molecules here 00:03:46.840 --> 00:03:48.730 have a lower kinetic energy. 00:03:48.730 --> 00:03:50.780 So this one maybe is doing this. 00:03:50.780 --> 00:03:52.750 I'm going to see if I can draw... 00:03:52.750 --> 00:03:56.520 On average, they're going to have a lower kinetic energy. 00:03:56.520 --> 00:03:58.110 That doesn't mean all of these molecules 00:03:58.110 --> 00:04:00.110 are necessarily slower than all of these molecules 00:04:00.110 --> 00:04:02.160 or have lower kinetic energy than all of these molecules. 00:04:02.160 --> 00:04:06.901 But on average they're going to have less kinetic energy. 00:04:06.901 --> 00:04:08.930 And we can actually draw a distribution. 00:04:08.930 --> 00:04:10.600 And this distribution, that is 00:04:10.600 --> 00:04:13.382 the Maxwell-Boltzmann distribution. 00:04:13.382 --> 00:04:15.110 So if we... 00:04:15.110 --> 00:04:18.350 Let me draw a little coordinate plane here. 00:04:18.850 --> 00:04:23.850 So let me draw a coordinate plane. 00:04:24.260 --> 00:04:28.160 So, if on this axis, I were to put speed. 00:04:28.670 --> 00:04:30.140 If I were to put speed. 00:04:30.140 --> 00:04:33.532 And on this axis, I would put number of molecules. 00:04:33.532 --> 00:04:38.340 Number of molecules. 00:04:38.690 --> 00:04:39.931 Right over here. 00:04:39.931 --> 00:04:43.310 For this system, the system that is at 300 Kelvin 00:04:43.310 --> 00:04:46.092 the distribution might look like this. 00:04:46.092 --> 00:04:47.831 So it might look 00:04:47.831 --> 00:04:48.910 the distribution... 00:04:48.910 --> 00:04:50.340 Let me do this in a new color. 00:04:50.690 --> 00:04:53.120 So, the distribution 00:04:53.120 --> 00:04:54.840 this is gonna be all of the molecules. 00:04:54.840 --> 00:04:59.330 The distribution might look like this. 00:04:59.700 --> 00:05:00.890 Might look like this. 00:05:00.890 --> 00:05:02.920 And this would actually be the Maxwell-Boltzmann 00:05:02.920 --> 00:05:05.172 distribution for this system 00:05:05.172 --> 00:05:07.928 For system, let's call this system A. 00:05:07.928 --> 00:05:10.428 System A, right over here. 00:05:10.428 --> 00:05:14.710 And this system, that has a lower temperature 00:05:14.710 --> 00:05:17.238 which means it also has a lower kinetic energy. 00:05:17.238 --> 00:05:19.676 The distribution of its particles... 00:05:19.676 --> 00:05:22.615 So the most likely, the most probable... 00:05:22.615 --> 00:05:24.710 You're going to have the highest number of molecules 00:05:24.710 --> 00:05:25.900 at a slower speed. 00:05:25.900 --> 00:05:27.330 Let's say you're gonna have it at this speed 00:05:27.330 --> 00:05:28.603 right over here. 00:05:28.603 --> 00:05:33.600 So its distribution might look something like this. 00:05:35.000 --> 00:05:37.010 So it might look something like that. 00:05:37.740 --> 00:05:38.980 Now why is this one... 00:05:38.980 --> 00:05:40.310 It might make sense to you that 00:05:40.310 --> 00:05:42.020 okay, the most probable 00:05:42.020 --> 00:05:45.500 the speed at which I have the most molecules 00:05:45.500 --> 00:05:48.460 I get that that's going to be lower than the speed 00:05:48.460 --> 00:05:51.310 at which I have the most molecules in system A 00:05:51.310 --> 00:05:54.280 because I have, because on average 00:05:54.280 --> 00:05:56.050 these things have less kinetic energy. 00:05:56.050 --> 00:05:58.235 They're going to have less speed. 00:05:58.235 --> 00:06:00.184 But why is this peak higher? 00:06:00.184 --> 00:06:01.550 Well, you gotta remember we're talking about 00:06:01.550 --> 00:06:03.080 the same number of molecules. 00:06:03.080 --> 00:06:05.350 So if we have the same number of molecules that means 00:06:05.350 --> 00:06:07.910 that the areas under these curves need to be the same. 00:06:07.910 --> 00:06:10.900 So if this one is narrower, it's going to be taller. 00:06:10.900 --> 00:06:12.760 And if I were gonna, if I were to somehow 00:06:12.760 --> 00:06:15.380 raise the temperature of this system even more. 00:06:15.380 --> 00:06:17.780 Let's say I create a third system or I get this 00:06:17.780 --> 00:06:20.020 or let's say I were to heat it up to 400 Kelvin. 00:06:20.020 --> 00:06:24.120 Well then my distribution would look 00:06:24.120 --> 00:06:27.470 something like this. 00:06:27.470 --> 00:06:29.940 So this is if I heated it up. 00:06:30.270 --> 00:06:32.800 Heated up. 00:06:32.800 --> 00:06:35.620 And so this is all the Maxwell-Boltzmann distribution is. 00:06:35.620 --> 00:06:39.800 I'm not giving you the more involved, hairy equation for it 00:06:39.800 --> 00:06:42.128 but really the idea of what it is. 00:06:42.128 --> 00:06:43.530 It's a pretty neat idea. 00:06:43.530 --> 00:06:46.010 And actually when you actually think about the actual 00:06:46.010 --> 00:06:49.690 speeds of some of these particles, even the air around you 00:06:49.690 --> 00:06:52.060 I'm gonna say, "Oh, it looks pretty stationary to me." 00:06:52.060 --> 00:06:54.700 But it turns out in the air around you is mostly nitrogen. 00:06:54.700 --> 00:06:59.000 That the most probable speed of 00:06:59.000 --> 00:07:00.410 if you picked a random nitrogen 00:07:00.410 --> 00:07:02.618 molecule around you right now. 00:07:02.618 --> 00:07:04.340 So the most probable speed. 00:07:04.340 --> 00:07:05.160 I'm gonna write this down 00:07:05.160 --> 00:07:07.039 'cause this is pretty mindblowing. 00:07:07.039 --> 00:07:10.780 Most probable speed at room temperature. 00:07:10.784 --> 00:07:15.780 Probable speed 00:07:16.197 --> 00:07:20.154 of N2 at room temperature. 00:07:20.154 --> 00:07:23.960 Room temperature. 00:07:25.230 --> 00:07:27.400 So let's say this that this was the Maxwell-Boltzmann 00:07:27.400 --> 00:07:30.960 distribution for nitrogen at room temperature. 00:07:30.960 --> 00:07:32.620 Let's say that that's, let's say we make 00:07:32.620 --> 00:07:35.450 we call room temperature 300 Kelvin. 00:07:35.450 --> 00:07:37.870 This most probable speed right over here 00:07:37.870 --> 00:07:40.030 the one where we have the most molecules 00:07:40.030 --> 00:07:41.400 the one where we're gonna have the most 00:07:41.400 --> 00:07:43.070 molecules at that speed. 00:07:43.630 --> 00:07:45.990 In fact, guess what that is going to be before I tell you 00:07:45.990 --> 00:07:47.635 'cause it's actually mind boggling. 00:07:47.635 --> 00:07:49.930 Well, it turns out that it is approximately 00:07:49.930 --> 00:07:53.690 400, 400 and actually at 300 Kelvin 00:07:53.690 --> 00:07:57.846 it's gonna be 422 meters per second. 00:07:57.846 --> 00:08:00.510 422 meters per second. 00:08:00.510 --> 00:08:04.220 Imagine something traveling 422 meters in a second. 00:08:04.220 --> 00:08:06.700 And if you're used to thinking in terms of miles per hour 00:08:06.700 --> 00:08:09.860 this is approximately 944 00:08:09.860 --> 00:08:12.730 miles per hour. 00:08:12.730 --> 00:08:14.927 So right now, around you 00:08:14.927 --> 00:08:16.850 you have, actually 00:08:16.850 --> 00:08:20.340 the most probable, the highest number 00:08:20.340 --> 00:08:22.300 of the nitrogen molecules around you 00:08:22.300 --> 00:08:24.900 are traveling at roughly this speed 00:08:24.900 --> 00:08:26.280 and they're bumping into you. 00:08:26.280 --> 00:08:27.860 That's actually what's giving you air pressure. 00:08:27.860 --> 00:08:29.480 And not just that speed, there are actually ones 00:08:29.480 --> 00:08:31.190 that are travelling even faster than that. 00:08:31.190 --> 00:08:34.570 Even faster than 422 meters per second. 00:08:34.570 --> 00:08:35.210 Even faster. 00:08:35.210 --> 00:08:37.730 There's particles around you traveling faster 00:08:37.730 --> 00:08:39.210 than a thousand miles per hour 00:08:39.210 --> 00:08:41.980 and they are bumping into your body as we speak. 00:08:41.980 --> 00:08:43.650 And you might say, "Well, why doesn't that hurt?" 00:08:43.650 --> 00:08:47.040 Well, that gives you a sense of how small the mass 00:08:47.040 --> 00:08:48.870 of a nitrogen molecule is, that it can 00:08:48.870 --> 00:08:51.640 bump into you at a thousand miles per hour 00:08:51.640 --> 00:08:52.640 and you really don't feel it. 00:08:52.640 --> 00:08:55.554 It feels just like the ambient air pressure. 00:08:55.554 --> 00:08:57.030 Now, when you first look at this, you're like 00:08:57.030 --> 00:08:59.300 wait, 422 meters per second? 00:08:59.300 --> 00:09:01.510 That's faster than the speed of sound. 00:09:01.510 --> 00:09:04.770 The speed of sound is around 340 meters per second. 00:09:04.770 --> 00:09:06.000 Well, how can this be? 00:09:06.000 --> 00:09:06.860 Well, just think about it. 00:09:06.860 --> 00:09:09.220 Sound is transmitted through the air 00:09:09.220 --> 00:09:10.970 through collisions of particles. 00:09:10.970 --> 00:09:13.420 So the particles themselves have to be moving 00:09:13.420 --> 00:09:15.300 or at least some of them, have to be moving 00:09:15.300 --> 00:09:16.780 faster than the speed of sound. 00:09:16.780 --> 00:09:18.960 So, not all of the things around you 00:09:18.960 --> 00:09:19.910 are moving this fast and they're 00:09:19.910 --> 00:09:20.810 moving in all different directions. 00:09:20.810 --> 00:09:23.298 Some of them might not be moving much at all. 00:09:23.298 --> 00:09:26.520 But some of them are moving quite incredibly fast. 00:09:26.520 --> 00:09:28.800 So, I don't know, I find that a little bit mindblowing.