1 00:00:00,090 --> 00:00:02,490 The following content is provided under a Creative 2 00:00:02,490 --> 00:00:04,059 Commons license. 3 00:00:04,059 --> 00:00:06,330 Your support will help MIT OpenCourseWare 4 00:00:06,330 --> 00:00:10,690 continue to offer high quality educational resources for free. 5 00:00:10,690 --> 00:00:13,320 To make a donation or view additional materials 6 00:00:13,320 --> 00:00:15,810 from hundreds of MIT courses, visit 7 00:00:15,810 --> 00:00:20,656 MIT you OpenCourseWare at ocw.mit.edu. 8 00:00:20,656 --> 00:00:23,040 SHAOUL EZEKIEL: As we have already learned, 9 00:00:23,040 --> 00:00:26,730 the most important component in a laser, 10 00:00:26,730 --> 00:00:31,080 or the heart of the laser, is the gain medium 11 00:00:31,080 --> 00:00:33,990 or the optical amplifier. 12 00:00:33,990 --> 00:00:35,670 This is no ordinary amplifier. 13 00:00:35,670 --> 00:00:38,940 This is an amplifier for light. 14 00:00:38,940 --> 00:00:41,250 And in this demonstration, we're going 15 00:00:41,250 --> 00:00:44,250 to show you, and hopefully convince you, that, indeed, 16 00:00:44,250 --> 00:00:47,790 light can be amplified. 17 00:00:47,790 --> 00:00:50,490 The amount of amplification is not so huge. 18 00:00:50,490 --> 00:00:54,780 But I'm sure we'll make it convincing enough so that you 19 00:00:54,780 --> 00:00:59,640 get the feel that, indeed, that light can be amplified. 20 00:00:59,640 --> 00:01:02,100 The setup we're going to use is here. 21 00:01:02,100 --> 00:01:06,300 We're going to have a laser, which is 22 00:01:06,300 --> 00:01:08,740 going to be our light source. 23 00:01:08,740 --> 00:01:12,330 Here's the output of the laser. 24 00:01:12,330 --> 00:01:15,060 We're going to reflect it by this mirror here 25 00:01:15,060 --> 00:01:18,120 and then this mirror over here. 26 00:01:18,120 --> 00:01:23,730 Now, the laser beam then enters this optical amplifier. 27 00:01:23,730 --> 00:01:30,190 Now, this optical amplifier is essentially this. 28 00:01:30,190 --> 00:01:34,830 It's a discharge tube, helium neon gas mixture 29 00:01:34,830 --> 00:01:39,990 that will give gain amplification or gain at 6328 30 00:01:39,990 --> 00:01:41,070 Angstroms. 31 00:01:41,070 --> 00:01:44,040 In fact, the light enters this window here and then 32 00:01:44,040 --> 00:01:46,760 comes out at the other end. 33 00:01:46,760 --> 00:01:50,430 And that's what we have essentially 34 00:01:50,430 --> 00:01:53,580 mounted here right below. 35 00:01:53,580 --> 00:02:00,900 So then the output through this amplifier-- 36 00:02:00,900 --> 00:02:03,030 and the amplifier right now is turned off-- 37 00:02:03,030 --> 00:02:06,630 then goes onto a detector over here. 38 00:02:06,630 --> 00:02:08,759 And then the output of the detector 39 00:02:08,759 --> 00:02:13,980 then goes onto an oscilloscope over here. 40 00:02:13,980 --> 00:02:22,200 And also we look at the output on a digital meter. 41 00:02:22,200 --> 00:02:28,130 All right, so we have two ways of looking at the same output. 42 00:02:28,130 --> 00:02:32,580 All right, now we are ready to set zero. 43 00:02:32,580 --> 00:02:35,040 So first, what I'm going to do is then 44 00:02:35,040 --> 00:02:38,530 block the beam of light over here. 45 00:02:38,530 --> 00:02:42,810 And let's look at the zero on the scope and the zero 46 00:02:42,810 --> 00:02:46,080 on the meter. 47 00:02:46,080 --> 00:02:50,490 Now, the meter says 008, which is not quite zero. 48 00:02:50,490 --> 00:02:55,020 And the reason for that is because we have room light 49 00:02:55,020 --> 00:02:56,190 hitting the detector. 50 00:02:56,190 --> 00:02:58,120 So what I'm going to do to get rid of that, 51 00:02:58,120 --> 00:03:02,400 I'm going to put this little hood over the detector. 52 00:03:02,400 --> 00:03:09,108 Now we see that the output of the meter now is, indeed, zero. 53 00:03:09,108 --> 00:03:11,400 And also, hopefully, then the output of the scope here, 54 00:03:11,400 --> 00:03:15,330 this will be our zero on the oscilloscope. 55 00:03:15,330 --> 00:03:20,140 Now, if I take this card away, and let the light go through, 56 00:03:20,140 --> 00:03:23,700 you can see that now the output on the scope has changed. 57 00:03:23,700 --> 00:03:31,230 And the meter reads around 364, or 63, or thereabout, 58 00:03:31,230 --> 00:03:32,830 which is the output of the laser. 59 00:03:32,830 --> 00:03:37,620 Now all I have to do is block the laser beam. 60 00:03:37,620 --> 00:03:41,490 And we go back to zero on the meter as well as zero 61 00:03:41,490 --> 00:03:42,210 on the scope. 62 00:03:42,210 --> 00:03:43,305 Here we are. 63 00:03:43,305 --> 00:03:45,570 The laser beam's back again. 64 00:03:45,570 --> 00:03:49,530 And then we get that same value again. 65 00:03:49,530 --> 00:03:54,030 Now, we're all familiar with absorption of light. 66 00:03:54,030 --> 00:03:57,610 And I just want to just demonstrate it, 67 00:03:57,610 --> 00:03:58,420 just for reference. 68 00:03:58,420 --> 00:04:00,180 I'm going to put a piece of glass 69 00:04:00,180 --> 00:04:02,460 in front of the laser beam. 70 00:04:02,460 --> 00:04:05,580 And we know that glass at normal incidence 71 00:04:05,580 --> 00:04:08,860 has a reflectivity of about 4% per surface. 72 00:04:08,860 --> 00:04:12,930 So I should get an attenuation of about 8% or so 73 00:04:12,930 --> 00:04:16,630 when I put this piece of glass in the beam of light. 74 00:04:16,630 --> 00:04:19,574 Now you can see the meter has dropped now to 330-- 75 00:04:22,490 --> 00:04:27,210 300 and, well, if I can keep it still, 320 something. 76 00:04:27,210 --> 00:04:30,220 Now, if I take the piece of glass away, 77 00:04:30,220 --> 00:04:35,100 now we go up to the previous number of 360 something. 78 00:04:35,100 --> 00:04:38,790 So you can see we have an attenuation of about 8 79 00:04:38,790 --> 00:04:40,950 or so percent. 80 00:04:40,950 --> 00:04:45,390 Now what I'm going to do now is put this piece of glass 81 00:04:45,390 --> 00:04:48,180 before the detector also. 82 00:04:48,180 --> 00:04:54,090 And, indeed, I'm going to hold it against the tube 83 00:04:54,090 --> 00:04:56,280 here so that I don't shake too much. 84 00:04:56,280 --> 00:05:05,540 And again you can see that the attenuation is also about 8% 85 00:05:05,540 --> 00:05:06,115 or so. 86 00:05:06,115 --> 00:05:07,490 Here, let me put it in the front. 87 00:05:13,120 --> 00:05:16,950 And then also then I'll put it in the back again. 88 00:05:16,950 --> 00:05:22,090 And hopefully I'll put it in the same position. 89 00:05:22,090 --> 00:05:24,464 You can see this-- 90 00:05:24,464 --> 00:05:26,410 I can hold it still. 91 00:05:30,170 --> 00:05:34,780 And then take it away, and then roughly we 92 00:05:34,780 --> 00:05:36,220 get this 8% attenuation. 93 00:05:36,220 --> 00:05:38,320 So now we've demonstrated that, indeed, light 94 00:05:38,320 --> 00:05:42,400 can be easily attenuated. 95 00:05:42,400 --> 00:05:47,230 Now we come to this crucial demonstration of gain. 96 00:05:47,230 --> 00:05:53,710 So now I want you to then watch both the scope and the meter 97 00:05:53,710 --> 00:05:57,890 as I turn on the amplifier. 98 00:05:57,890 --> 00:06:01,660 So here I'm going to now turn on the amplifier. 99 00:06:01,660 --> 00:06:07,000 And remember, this number is around 363 or so, 364. 100 00:06:07,000 --> 00:06:09,710 Now you can see on the scope we jumped a little bit. 101 00:06:09,710 --> 00:06:13,960 And the meter has gone up to 380 something, which 102 00:06:13,960 --> 00:06:16,950 is an increase of about 5%. 103 00:06:16,950 --> 00:06:19,885 Let me turn it off. 104 00:06:19,885 --> 00:06:21,760 Again, you can see on the scope it went down. 105 00:06:21,760 --> 00:06:25,630 In fact, just watch the scope for a little while. 106 00:06:25,630 --> 00:06:27,610 I'm going to turn it on and off very fast 107 00:06:27,610 --> 00:06:28,912 so that you get a feel that-- 108 00:06:28,912 --> 00:06:31,120 here it goes, up a little bit, and down a little bit. 109 00:06:31,120 --> 00:06:34,120 Since it's only a few percent, it's 110 00:06:34,120 --> 00:06:37,570 difficult to see it on the scope the way I have it set up. 111 00:06:37,570 --> 00:06:39,520 But it's much easier to see it on the meter. 112 00:06:39,520 --> 00:06:41,320 So you can see that with amplification we 113 00:06:41,320 --> 00:06:42,850 have 380 something. 114 00:06:42,850 --> 00:06:46,990 With no amplification, then we're back to 360 something. 115 00:06:46,990 --> 00:06:51,700 Again, roughly, it's about 5% amplification. 116 00:06:51,700 --> 00:06:55,480 Now, you may wonder that maybe what we're getting 117 00:06:55,480 --> 00:06:58,210 is when I turn on the amplifier that we're getting light 118 00:06:58,210 --> 00:07:00,430 from the amplifier that hits the detector. 119 00:07:00,430 --> 00:07:01,930 It's not really amplification. 120 00:07:01,930 --> 00:07:04,540 So to prove this, what I'm going to do 121 00:07:04,540 --> 00:07:10,952 is block the beam of light going into the amplifier 122 00:07:10,952 --> 00:07:12,910 so that there's no light going on the detector. 123 00:07:12,910 --> 00:07:14,715 We're back to our zero on the meter. 124 00:07:14,715 --> 00:07:16,090 And now what I'm going to do, I'm 125 00:07:16,090 --> 00:07:19,780 going to turn on the amplifier just by itself just 126 00:07:19,780 --> 00:07:22,030 to see if there's any light from the amplifier falling 127 00:07:22,030 --> 00:07:23,020 on the detector. 128 00:07:23,020 --> 00:07:24,130 So here we go. 129 00:07:24,130 --> 00:07:25,820 Watch the meter and the scope. 130 00:07:25,820 --> 00:07:28,092 And here is the amplifier on. 131 00:07:28,092 --> 00:07:29,800 Again, you can see that there's no change 132 00:07:29,800 --> 00:07:31,360 on the meter or the scope. 133 00:07:31,360 --> 00:07:33,730 Here's off. 134 00:07:33,730 --> 00:07:38,800 And do it again, on, and off. 135 00:07:38,800 --> 00:07:42,690 So, indeed, we've shown that light from the amplifier 136 00:07:42,690 --> 00:07:44,440 or spontaneous emission from the amplifier 137 00:07:44,440 --> 00:07:49,070 is not hitting the detector and increasing the output. 138 00:07:49,070 --> 00:07:52,540 So again, let me just redo it again for you. 139 00:07:52,540 --> 00:07:58,600 Here is the light falling on the detector 140 00:07:58,600 --> 00:08:02,870 without amplification, again 360 something. 141 00:08:02,870 --> 00:08:10,460 And here comes the amplification again, yes, close to 380. 142 00:08:10,460 --> 00:08:12,210 It's a little bit less than we had before. 143 00:08:12,210 --> 00:08:14,010 Maybe the amplifier's getting a little old. 144 00:08:14,010 --> 00:08:16,320 Here we are without amplification. 145 00:08:16,320 --> 00:08:19,240 We have this value. 146 00:08:19,240 --> 00:08:22,170 So in summary, we've shown that light 147 00:08:22,170 --> 00:08:24,300 can be, indeed, amplified. 148 00:08:24,300 --> 00:08:28,500 In this case, we used a helium neon amplifier 149 00:08:28,500 --> 00:08:32,880 to amplify light from a helium neon laser. 150 00:08:32,880 --> 00:08:38,159 We showed you a gain or amplification of 5% per pass. 151 00:08:38,159 --> 00:08:40,950 Now, you may think that's a small amount of gain. 152 00:08:40,950 --> 00:08:46,710 But a lot of helium neon lasers use gain of even less than 5%. 153 00:08:46,710 --> 00:08:49,800 And they have many, many applications. 154 00:08:49,800 --> 00:08:53,280 Of course, if you have even more gain, 155 00:08:53,280 --> 00:08:57,090 then you can get more powerful laser outputs 156 00:08:57,090 --> 00:09:01,910 with even greater number of applications.