1 00:00:01,400 --> 00:00:02,233 - [Instructor] Collision theory 2 00:00:02,233 --> 00:00:05,130 can be related to Maxwell-Boltzmann distributions. 3 00:00:05,130 --> 00:00:07,590 And first we'll start with collision theory. 4 00:00:07,590 --> 00:00:09,970 Collision theory says that particles must collide 5 00:00:09,970 --> 00:00:13,860 in the proper orientation and with enough kinetic energy 6 00:00:13,860 --> 00:00:17,370 to overcome the activation energy barrier. 7 00:00:17,370 --> 00:00:21,130 So let's look at the reaction where A reacts with B and C 8 00:00:21,130 --> 00:00:24,420 to form AB plus C. 9 00:00:24,420 --> 00:00:28,240 On an energy profile, we have the reactants over here 10 00:00:28,240 --> 00:00:29,580 in the left. 11 00:00:29,580 --> 00:00:33,660 So A, atom A is colored red, 12 00:00:33,660 --> 00:00:36,590 and we have molecule BC over here, 13 00:00:36,590 --> 00:00:39,790 So these two particles must collide 14 00:00:39,790 --> 00:00:43,150 for the reaction to occur, 15 00:00:43,150 --> 00:00:45,400 and they must collide with enough energy 16 00:00:45,400 --> 00:00:48,070 to overcome the activation energy barrier. 17 00:00:48,070 --> 00:00:51,210 So the activation energy on an energy profile 18 00:00:51,210 --> 00:00:52,250 is the difference in energy 19 00:00:52,250 --> 00:00:56,010 between the peak here, which is the transition state 20 00:00:56,010 --> 00:00:57,610 and the energy of the reactants. 21 00:00:57,610 --> 00:01:01,810 So this energy here is our activation energy. 22 00:01:01,810 --> 00:01:04,030 The minimum amount of energy necessary 23 00:01:04,030 --> 00:01:06,770 for the reaction to occur. 24 00:01:06,770 --> 00:01:09,830 So if these particles collide with enough energy, 25 00:01:09,830 --> 00:01:13,920 we can just get over this activation energy barrier 26 00:01:13,920 --> 00:01:17,653 and the reactions can turn into our two products. 27 00:01:20,020 --> 00:01:22,090 If our reactant particles don't hit each other 28 00:01:22,090 --> 00:01:25,340 with enough energy, they simply bounce off of each other 29 00:01:25,340 --> 00:01:27,070 and our reaction never occurs. 30 00:01:27,070 --> 00:01:30,820 We never overcome this activation energy barrier. 31 00:01:30,820 --> 00:01:33,420 As an analogy, let's think about hitting a golf ball. 32 00:01:33,420 --> 00:01:35,310 So let's imagine we have a hill, 33 00:01:35,310 --> 00:01:37,150 and on the right side of the hill, 34 00:01:37,150 --> 00:01:39,050 somewhere is the hole down here, 35 00:01:39,050 --> 00:01:42,700 and the left side of the hill is our golf ball. 36 00:01:42,700 --> 00:01:45,720 So we know we have to hit this golf ball with enough force 37 00:01:45,720 --> 00:01:47,920 to give it enough kinetic energy 38 00:01:47,920 --> 00:01:49,970 for it to reach the top of the hill 39 00:01:49,970 --> 00:01:53,050 and to roll over the hill and go into the hole. 40 00:01:53,050 --> 00:01:55,320 So we can imagine this hill 41 00:01:55,320 --> 00:01:58,580 as being a hill of potential energy. 42 00:01:58,580 --> 00:02:02,080 And this golf ball needs to have enough kinetic energy 43 00:02:02,080 --> 00:02:06,353 to turn into enough potential energy to go over the hill. 44 00:02:09,390 --> 00:02:11,230 If we don't hit our golf ball hard enough, 45 00:02:11,230 --> 00:02:13,730 it might not have enough energy to go over the hill. 46 00:02:13,730 --> 00:02:16,160 So if we hit it softly, it might just roll halfway 47 00:02:16,160 --> 00:02:18,470 up the hill and roll back down again. 48 00:02:18,470 --> 00:02:23,470 Kinetic energy is equal to 1/2 MV squared. 49 00:02:24,770 --> 00:02:26,630 And so M would be the mass of the golf ball 50 00:02:26,630 --> 00:02:28,790 and V would be the velocity. 51 00:02:28,790 --> 00:02:30,350 So we have to hit it with enough force 52 00:02:30,350 --> 00:02:33,770 so it has enough as a high enough velocity 53 00:02:33,770 --> 00:02:35,190 to have a high enough kinetic energy 54 00:02:35,190 --> 00:02:37,083 to get over the hill. 55 00:02:38,740 --> 00:02:40,160 Let's apply collision theory 56 00:02:40,160 --> 00:02:42,810 to a Maxwell-Boltzmann distribution. 57 00:02:42,810 --> 00:02:45,370 Usually a Maxwell-Boltzmann distribution 58 00:02:45,370 --> 00:02:48,400 has fractional particles or relative numbers of particles 59 00:02:48,400 --> 00:02:52,790 on the y-axis and particle speed on the x-axis. 60 00:02:52,790 --> 00:02:55,160 And a Maxwell-Boltzmann distribution 61 00:02:55,160 --> 00:03:00,160 shows us the range of speeds available to the particles 62 00:03:01,380 --> 00:03:02,840 in a sample of gas. 63 00:03:02,840 --> 00:03:04,160 So let's say we have, 64 00:03:04,160 --> 00:03:06,420 here's a particulate diagram over here. 65 00:03:06,420 --> 00:03:07,820 Let's say we have a sample of gas 66 00:03:07,820 --> 00:03:10,290 at a particular temperature T. 67 00:03:10,290 --> 00:03:12,980 These particles aren't traveling at the same speed, 68 00:03:12,980 --> 00:03:15,790 there's a range of speeds available to them. 69 00:03:15,790 --> 00:03:19,820 So one particle might be traveling really slowly 70 00:03:19,820 --> 00:03:22,090 so we'll draw a very short arrow here. 71 00:03:22,090 --> 00:03:24,450 A few more might be traveling a little faster, 72 00:03:24,450 --> 00:03:28,190 so we'll draw the arrow longer to indicate a faster speed. 73 00:03:28,190 --> 00:03:31,310 And maybe one particle is traveling the fastest. 74 00:03:31,310 --> 00:03:34,293 So we'll give this particle the longest arrow. 75 00:03:36,130 --> 00:03:38,400 We can think about the area under the curve 76 00:03:38,400 --> 00:03:40,310 for a Maxwell-Boltzmann distribution 77 00:03:40,310 --> 00:03:43,850 as representing all of the particles in our sample. 78 00:03:43,850 --> 00:03:47,920 So we had this one particle here moving very slowly, 79 00:03:47,920 --> 00:03:50,450 and so if we look at our curve and we think 80 00:03:50,450 --> 00:03:52,120 about the area under the curve 81 00:03:52,120 --> 00:03:54,073 that's at a low particle speed, 82 00:03:54,920 --> 00:03:57,410 this area is smaller than other parts of the curve. 83 00:03:57,410 --> 00:03:59,640 So that's represented here by only this one particle 84 00:03:59,640 --> 00:04:01,490 moving very slowly. 85 00:04:01,490 --> 00:04:03,620 We think about this next part of the curve, 86 00:04:03,620 --> 00:04:06,610 most, this is a large amount of area in here 87 00:04:06,610 --> 00:04:09,640 and these particles are traveling at a higher speed. 88 00:04:09,640 --> 00:04:14,640 So maybe these three particles here would represent 89 00:04:15,550 --> 00:04:17,870 the particles moving at a higher speed. 90 00:04:17,870 --> 00:04:21,670 And then finally, we had this one particle here, 91 00:04:21,670 --> 00:04:23,610 We drew this arrow longer than the others. 92 00:04:23,610 --> 00:04:26,440 So this particle's traveling faster than the other one. 93 00:04:26,440 --> 00:04:29,750 So maybe this area under the curve up here 94 00:04:29,750 --> 00:04:31,853 is represented by that one particle. 95 00:04:33,520 --> 00:04:34,890 We know from collision theory, 96 00:04:34,890 --> 00:04:37,760 that particles have to have enough kinetic energy 97 00:04:37,760 --> 00:04:42,760 to overcome the activation energy for a reaction to occur. 98 00:04:42,850 --> 00:04:46,610 So we can draw a line representing the activation energy 99 00:04:46,610 --> 00:04:48,840 on a Maxwell-Boltzmann distribution. 100 00:04:48,840 --> 00:04:52,722 So if I draw this line, this dotted line right here, 101 00:04:52,722 --> 00:04:57,060 this represents my activation energy. 102 00:04:57,060 --> 00:04:59,600 And instead of particle speed, you could think 103 00:04:59,600 --> 00:05:02,400 about the x-axis as being kinetic energy if you want. 104 00:05:02,400 --> 00:05:05,480 So the faster a particle is traveling, 105 00:05:05,480 --> 00:05:07,690 the higher its kinetic energy. 106 00:05:07,690 --> 00:05:11,390 And so the area under the curve 107 00:05:11,390 --> 00:05:13,010 to the right of this dash line, 108 00:05:13,010 --> 00:05:14,640 this represents all of the particles 109 00:05:14,640 --> 00:05:19,640 that have enough kinetic energy for this reaction to occur. 110 00:05:21,820 --> 00:05:24,300 Next, let's think about what happens to the particles 111 00:05:24,300 --> 00:05:27,770 in our sample when we increase the temperature. 112 00:05:27,770 --> 00:05:29,240 So when we increase the temperature, 113 00:05:29,240 --> 00:05:32,350 the Maxwell-Boltzmann distribution changes. 114 00:05:32,350 --> 00:05:36,030 So what happens is the peak height drops 115 00:05:36,030 --> 00:05:40,360 and our Maxwell-Boltzmann distribution curve gets broader. 116 00:05:40,360 --> 00:05:43,373 So it looks something like this at a higher temperature. 117 00:05:45,380 --> 00:05:47,210 So we still have some particles traveling 118 00:05:47,210 --> 00:05:48,820 at relatively low speeds, right? 119 00:05:48,820 --> 00:05:50,440 Remember it's the area under the curve. 120 00:05:50,440 --> 00:05:53,583 So maybe that's represented by this one particle here, 121 00:05:54,440 --> 00:05:56,520 and next, let's think about the area 122 00:05:56,520 --> 00:06:00,180 to the left of this dash line for Ea. 123 00:06:00,180 --> 00:06:02,750 So we want to make these particles green here 124 00:06:02,750 --> 00:06:05,180 as we have some particles traveling 125 00:06:05,180 --> 00:06:06,510 a little bit of faster speeds. 126 00:06:06,510 --> 00:06:09,250 So let me go ahead and draw these arrows a little bit longer 127 00:06:09,250 --> 00:06:12,330 but notice what happens to the right of this dash line. 128 00:06:12,330 --> 00:06:14,880 We think about the area under the curve 129 00:06:14,880 --> 00:06:17,960 for the magenta curve. 130 00:06:17,960 --> 00:06:21,350 Notice how the area is bigger than in the previous example. 131 00:06:21,350 --> 00:06:24,450 So maybe this time we have these two particles here 132 00:06:24,450 --> 00:06:25,900 traveling at a faster speed. 133 00:06:25,900 --> 00:06:28,150 So I'm gonna draw these arrows longer 134 00:06:28,150 --> 00:06:30,270 to indicate they're traveling at a faster speed. 135 00:06:30,270 --> 00:06:33,780 And since they're to the right of this dash line here, 136 00:06:33,780 --> 00:06:36,690 both of these particles have enough kinetic energy 137 00:06:36,690 --> 00:06:40,840 to overcome the activation energy for our reaction. 138 00:06:40,840 --> 00:06:44,530 So we can see when you increase the temperature, 139 00:06:44,530 --> 00:06:46,730 you increase the number of particles 140 00:06:46,730 --> 00:06:48,580 that have enough kinetic energy 141 00:06:48,580 --> 00:06:51,323 to overcome the activation energy. 142 00:06:52,840 --> 00:06:54,090 It's important to point out 143 00:06:54,090 --> 00:06:56,770 that since the number of particles hasn't changed, 144 00:06:56,770 --> 00:06:59,480 all we've done is increase the temperature here, 145 00:06:59,480 --> 00:07:02,360 the area under the curve remains the same. 146 00:07:02,360 --> 00:07:06,420 So the area under the curve for the curve in yellow, 147 00:07:06,420 --> 00:07:08,880 is the same as the area under the curve 148 00:07:08,880 --> 00:07:12,010 for the one drawn in magenta. 149 00:07:12,010 --> 00:07:14,640 The difference of course is the one in magenta 150 00:07:14,640 --> 00:07:15,950 is at a higher temperature, 151 00:07:15,950 --> 00:07:18,370 and therefore there are more particles with enough energy 152 00:07:18,370 --> 00:07:20,790 to overcome the activation energy. 153 00:07:20,790 --> 00:07:23,030 So increasing the temperature 154 00:07:23,030 --> 00:07:25,783 increases the rate of reaction.