WEBVTT 00:00:01.400 --> 00:00:02.233 - [Instructor] Collision theory 00:00:02.233 --> 00:00:05.130 can be related to Maxwell-Boltzmann distributions. 00:00:05.130 --> 00:00:07.590 And first we'll start with collision theory. 00:00:07.590 --> 00:00:09.970 Collision theory says that particles must collide 00:00:09.970 --> 00:00:13.860 in the proper orientation and with enough kinetic energy 00:00:13.860 --> 00:00:17.370 to overcome the activation energy barrier. 00:00:17.370 --> 00:00:21.130 So let's look at the reaction where A reacts with B and C 00:00:21.130 --> 00:00:24.420 to form AB plus C. 00:00:24.420 --> 00:00:28.240 On an energy profile, we have the reactants over here 00:00:28.240 --> 00:00:29.580 in the left. 00:00:29.580 --> 00:00:33.660 So A, atom A is colored red, 00:00:33.660 --> 00:00:36.590 and we have molecule BC over here, 00:00:36.590 --> 00:00:39.790 So these two particles must collide 00:00:39.790 --> 00:00:43.150 for the reaction to occur, 00:00:43.150 --> 00:00:45.400 and they must collide with enough energy 00:00:45.400 --> 00:00:48.070 to overcome the activation energy barrier. 00:00:48.070 --> 00:00:51.210 So the activation energy on an energy profile 00:00:51.210 --> 00:00:52.250 is the difference in energy 00:00:52.250 --> 00:00:56.010 between the peak here, which is the transition state 00:00:56.010 --> 00:00:57.610 and the energy of the reactants. 00:00:57.610 --> 00:01:01.810 So this energy here is our activation energy. 00:01:01.810 --> 00:01:04.030 The minimum amount of energy necessary 00:01:04.030 --> 00:01:06.770 for the reaction to occur. 00:01:06.770 --> 00:01:09.830 So if these particles collide with enough energy, 00:01:09.830 --> 00:01:13.920 we can just get over this activation energy barrier 00:01:13.920 --> 00:01:17.653 and the reactions can turn into our two products. 00:01:20.020 --> 00:01:22.090 If our reactant particles don't hit each other 00:01:22.090 --> 00:01:25.340 with enough energy, they simply bounce off of each other 00:01:25.340 --> 00:01:27.070 and our reaction never occurs. 00:01:27.070 --> 00:01:30.820 We never overcome this activation energy barrier. 00:01:30.820 --> 00:01:33.420 As an analogy, let's think about hitting a golf ball. 00:01:33.420 --> 00:01:35.310 So let's imagine we have a hill, 00:01:35.310 --> 00:01:37.150 and on the right side of the hill, 00:01:37.150 --> 00:01:39.050 somewhere is the hole down here, 00:01:39.050 --> 00:01:42.700 and the left side of the hill is our golf ball. 00:01:42.700 --> 00:01:45.720 So we know we have to hit this golf ball with enough force 00:01:45.720 --> 00:01:47.920 to give it enough kinetic energy 00:01:47.920 --> 00:01:49.970 for it to reach the top of the hill 00:01:49.970 --> 00:01:53.050 and to roll over the hill and go into the hole. 00:01:53.050 --> 00:01:55.320 So we can imagine this hill 00:01:55.320 --> 00:01:58.580 as being a hill of potential energy. 00:01:58.580 --> 00:02:02.080 And this golf ball needs to have enough kinetic energy 00:02:02.080 --> 00:02:06.353 to turn into enough potential energy to go over the hill. 00:02:09.390 --> 00:02:11.230 If we don't hit our golf ball hard enough, 00:02:11.230 --> 00:02:13.730 it might not have enough energy to go over the hill. 00:02:13.730 --> 00:02:16.160 So if we hit it softly, it might just roll halfway 00:02:16.160 --> 00:02:18.470 up the hill and roll back down again. 00:02:18.470 --> 00:02:23.470 Kinetic energy is equal to 1/2 MV squared. 00:02:24.770 --> 00:02:26.630 And so M would be the mass of the golf ball 00:02:26.630 --> 00:02:28.790 and V would be the velocity. 00:02:28.790 --> 00:02:30.350 So we have to hit it with enough force 00:02:30.350 --> 00:02:33.770 so it has enough as a high enough velocity 00:02:33.770 --> 00:02:35.190 to have a high enough kinetic energy 00:02:35.190 --> 00:02:37.083 to get over the hill. 00:02:38.740 --> 00:02:40.160 Let's apply collision theory 00:02:40.160 --> 00:02:42.810 to a Maxwell-Boltzmann distribution. 00:02:42.810 --> 00:02:45.370 Usually a Maxwell-Boltzmann distribution 00:02:45.370 --> 00:02:48.400 has fractional particles or relative numbers of particles 00:02:48.400 --> 00:02:52.790 on the y-axis and particle speed on the x-axis. 00:02:52.790 --> 00:02:55.160 And a Maxwell-Boltzmann distribution 00:02:55.160 --> 00:03:00.160 shows us the range of speeds available to the particles 00:03:01.380 --> 00:03:02.840 in a sample of gas. 00:03:02.840 --> 00:03:04.160 So let's say we have, 00:03:04.160 --> 00:03:06.420 here's a particulate diagram over here. 00:03:06.420 --> 00:03:07.820 Let's say we have a sample of gas 00:03:07.820 --> 00:03:10.290 at a particular temperature T. 00:03:10.290 --> 00:03:12.980 These particles aren't traveling at the same speed, 00:03:12.980 --> 00:03:15.790 there's a range of speeds available to them. 00:03:15.790 --> 00:03:19.820 So one particle might be traveling really slowly 00:03:19.820 --> 00:03:22.090 so we'll draw a very short arrow here. 00:03:22.090 --> 00:03:24.450 A few more might be traveling a little faster, 00:03:24.450 --> 00:03:28.190 so we'll draw the arrow longer to indicate a faster speed. 00:03:28.190 --> 00:03:31.310 And maybe one particle is traveling the fastest. 00:03:31.310 --> 00:03:34.293 So we'll give this particle the longest arrow. 00:03:36.130 --> 00:03:38.400 We can think about the area under the curve 00:03:38.400 --> 00:03:40.310 for a Maxwell-Boltzmann distribution 00:03:40.310 --> 00:03:43.850 as representing all of the particles in our sample. 00:03:43.850 --> 00:03:47.920 So we had this one particle here moving very slowly, 00:03:47.920 --> 00:03:50.450 and so if we look at our curve and we think 00:03:50.450 --> 00:03:52.120 about the area under the curve 00:03:52.120 --> 00:03:54.073 that's at a low particle speed, 00:03:54.920 --> 00:03:57.410 this area is smaller than other parts of the curve. 00:03:57.410 --> 00:03:59.640 So that's represented here by only this one particle 00:03:59.640 --> 00:04:01.490 moving very slowly. 00:04:01.490 --> 00:04:03.620 We think about this next part of the curve, 00:04:03.620 --> 00:04:06.610 most, this is a large amount of area in here 00:04:06.610 --> 00:04:09.640 and these particles are traveling at a higher speed. 00:04:09.640 --> 00:04:14.640 So maybe these three particles here would represent 00:04:15.550 --> 00:04:17.870 the particles moving at a higher speed. 00:04:17.870 --> 00:04:21.670 And then finally, we had this one particle here, 00:04:21.670 --> 00:04:23.610 We drew this arrow longer than the others. 00:04:23.610 --> 00:04:26.440 So this particle's traveling faster than the other one. 00:04:26.440 --> 00:04:29.750 So maybe this area under the curve up here 00:04:29.750 --> 00:04:31.853 is represented by that one particle. 00:04:33.520 --> 00:04:34.890 We know from collision theory, 00:04:34.890 --> 00:04:37.760 that particles have to have enough kinetic energy 00:04:37.760 --> 00:04:42.760 to overcome the activation energy for a reaction to occur. 00:04:42.850 --> 00:04:46.610 So we can draw a line representing the activation energy 00:04:46.610 --> 00:04:48.840 on a Maxwell-Boltzmann distribution. 00:04:48.840 --> 00:04:52.722 So if I draw this line, this dotted line right here, 00:04:52.722 --> 00:04:57.060 this represents my activation energy. 00:04:57.060 --> 00:04:59.600 And instead of particle speed, you could think 00:04:59.600 --> 00:05:02.400 about the x-axis as being kinetic energy if you want. 00:05:02.400 --> 00:05:05.480 So the faster a particle is traveling, 00:05:05.480 --> 00:05:07.690 the higher its kinetic energy. 00:05:07.690 --> 00:05:11.390 And so the area under the curve 00:05:11.390 --> 00:05:13.010 to the right of this dash line, 00:05:13.010 --> 00:05:14.640 this represents all of the particles 00:05:14.640 --> 00:05:19.640 that have enough kinetic energy for this reaction to occur. 00:05:21.820 --> 00:05:24.300 Next, let's think about what happens to the particles 00:05:24.300 --> 00:05:27.770 in our sample when we increase the temperature. 00:05:27.770 --> 00:05:29.240 So when we increase the temperature, 00:05:29.240 --> 00:05:32.350 the Maxwell-Boltzmann distribution changes. 00:05:32.350 --> 00:05:36.030 So what happens is the peak height drops 00:05:36.030 --> 00:05:40.360 and our Maxwell-Boltzmann distribution curve gets broader. 00:05:40.360 --> 00:05:43.373 So it looks something like this at a higher temperature. 00:05:45.380 --> 00:05:47.210 So we still have some particles traveling 00:05:47.210 --> 00:05:48.820 at relatively low speeds, right? 00:05:48.820 --> 00:05:50.440 Remember it's the area under the curve. 00:05:50.440 --> 00:05:53.583 So maybe that's represented by this one particle here, 00:05:54.440 --> 00:05:56.520 and next, let's think about the area 00:05:56.520 --> 00:06:00.180 to the left of this dash line for Ea. 00:06:00.180 --> 00:06:02.750 So we want to make these particles green here 00:06:02.750 --> 00:06:05.180 as we have some particles traveling 00:06:05.180 --> 00:06:06.510 a little bit of faster speeds. 00:06:06.510 --> 00:06:09.250 So let me go ahead and draw these arrows a little bit longer 00:06:09.250 --> 00:06:12.330 but notice what happens to the right of this dash line. 00:06:12.330 --> 00:06:14.880 We think about the area under the curve 00:06:14.880 --> 00:06:17.960 for the magenta curve. 00:06:17.960 --> 00:06:21.350 Notice how the area is bigger than in the previous example. 00:06:21.350 --> 00:06:24.450 So maybe this time we have these two particles here 00:06:24.450 --> 00:06:25.900 traveling at a faster speed. 00:06:25.900 --> 00:06:28.150 So I'm gonna draw these arrows longer 00:06:28.150 --> 00:06:30.270 to indicate they're traveling at a faster speed. 00:06:30.270 --> 00:06:33.780 And since they're to the right of this dash line here, 00:06:33.780 --> 00:06:36.690 both of these particles have enough kinetic energy 00:06:36.690 --> 00:06:40.840 to overcome the activation energy for our reaction. 00:06:40.840 --> 00:06:44.530 So we can see when you increase the temperature, 00:06:44.530 --> 00:06:46.730 you increase the number of particles 00:06:46.730 --> 00:06:48.580 that have enough kinetic energy 00:06:48.580 --> 00:06:51.323 to overcome the activation energy. 00:06:52.840 --> 00:06:54.090 It's important to point out 00:06:54.090 --> 00:06:56.770 that since the number of particles hasn't changed, 00:06:56.770 --> 00:06:59.480 all we've done is increase the temperature here, 00:06:59.480 --> 00:07:02.360 the area under the curve remains the same. 00:07:02.360 --> 00:07:06.420 So the area under the curve for the curve in yellow, 00:07:06.420 --> 00:07:08.880 is the same as the area under the curve 00:07:08.880 --> 00:07:12.010 for the one drawn in magenta. 00:07:12.010 --> 00:07:14.640 The difference of course is the one in magenta 00:07:14.640 --> 00:07:15.950 is at a higher temperature, 00:07:15.950 --> 00:07:18.370 and therefore there are more particles with enough energy 00:07:18.370 --> 00:07:20.790 to overcome the activation energy. 00:07:20.790 --> 00:07:23.030 So increasing the temperature 00:07:23.030 --> 00:07:25.783 increases the rate of reaction.