1 00:00:18,900 --> 00:00:22,230 PROFESSOR: Welcome back to [? A20, ?] special relativity. 2 00:00:22,230 --> 00:00:26,820 Very early in this lecture, we discussed what mass is 3 00:00:26,820 --> 00:00:29,790 and how we can understand the mass of a proton 4 00:00:29,790 --> 00:00:33,990 and the mass of an electron as it interacts with the Higgs 5 00:00:33,990 --> 00:00:35,455 background field. 6 00:00:35,455 --> 00:00:37,330 But here, the question is slightly different. 7 00:00:37,330 --> 00:00:41,430 You want to understand the difference or the lack 8 00:00:41,430 --> 00:00:45,630 of difference between the mass in a gravitational field 9 00:00:45,630 --> 00:00:49,110 compared to the inertial mass, a mass being 10 00:00:49,110 --> 00:00:51,330 pushed through some force. 11 00:00:51,330 --> 00:00:54,030 And it's probably Einstein's biggest realization 12 00:00:54,030 --> 00:00:55,590 that those two things are the same. 13 00:00:55,590 --> 00:00:59,850 And that finding is called the equivalence principle, 14 00:00:59,850 --> 00:01:03,030 the equivalence of the gravitational and inertial 15 00:01:03,030 --> 00:01:05,220 mass. 16 00:01:05,220 --> 00:01:09,840 So if you are a freely falling person, 17 00:01:09,840 --> 00:01:12,360 you will not feel your own weight 18 00:01:12,360 --> 00:01:13,680 in your gravitational field. 19 00:01:13,680 --> 00:01:15,390 You will just drop. 20 00:01:15,390 --> 00:01:18,780 And the gravitational field provides an acceleration. 21 00:01:18,780 --> 00:01:22,050 And that acceleration, if you are standing in an elevator 22 00:01:22,050 --> 00:01:26,070 or just sitting on a chair like I'm doing right now, 23 00:01:26,070 --> 00:01:30,220 then sets up an accelerating reference frame. 24 00:01:30,220 --> 00:01:33,630 So there is an equivalence between being accelerated 25 00:01:33,630 --> 00:01:38,600 or being stationary in a gravitational field.