Notes on Relativity and Cosmology - Physics Department, UCSB
Notes on Relativity and Cosmology - Physics Department, UCSB Notes on Relativity and Cosmology - Physics Department, UCSB
220 CHAPTER 8. GENERAL RELATIVITY AND CURVED SPACETIME However, this is not the end of the story. It turns out that there is also another effect which causes the ray to bend. This is due to the effect of the curvature of space on the light ray. This effect turns out to be exactly the same size as the first effect, and with the same sign. As a result, Einstein predicted a total bending angle of 1.75 seconds of arc – twice what would come just from the observation that light falls in a gravitational field. This is a tricky experiment to perform, because the Sun is bright enough that any star that close to the sun is very hard to see. One solution is to wait for a solar eclipse (when the moon pretty much blocks out the light from the sun itself) and then one can look at the stars nearby. Just such an observation was performed by the British physicist Sir Arthur Eddington in 1919. The result indicated a bending angle of right around 2 seconds of arc. More recently, much more accurate versions of this experiment have been performed which verify Einstein’s theory to high precision. See Theory and experiment in gravitational physics by Clifford M. Will, (Cambridge University Press, New York, 1993) QC178.W47 1993 for a modern discussion of these issues. 8.5.3 Other experiments: Radar Time Delay The bending of starlight was the really big victory for Einstein’s theory. However, there are two other classic experimental tests of general relativity that should be mentioned. One of these is just the effect of gravity on the frequency of light that we have already discussed. As we said before, this had to wait quite a long time (until 1959) before technology progressed to the stage where it could be performed. The last major class of experiments is called ‘Radar Time delay.’ These turn out to be the most accurate tests of Einstein’s theory, but they had to wait until even more modern times. The point is that the gravitational field effects not only the path through space taken by a light ray, but that it also effects the time that the light ray takes to trace out that path. As we have discussed once or twice before, time measurements can be made extremely accurately. So, these experiments can be done to very high precision. The idea behind these experiments is that you then send a microwave (a.k.a. radar) signal (which is basically a long wavelength light wave) over to the other side of the sun and back. You can either bounce it off a planet (say, Venus) or a space probe that you have sent over there for just this purpose. If you measure the time it takes for the signal to go over and then return, this time is always longer than it would have been in flat spacetime. In this way, you can carefully test Einstein’s theory. For more details, see fig. 7.3 of Theory and experiment in gravitational physics by Clifford M. Will, (Cambridge University Press, New York, 1993) QC178.W47 1993. There is a copy in the Physics Library. A less technical version of this book is Was Einstein Right? putting General Relativity to the test by Clifford M. Will (Basic Books, New York, 1993), also available in the Physics Library. You can also order a copy of this book from Amazon.com for about $15.
8.6. HOMEWORK PROBLEMS 221 8.6 Homework Problems The following problems provides practice in working with curved spaces (i.e., not space-times) and the corresponding metrics. 8-1. In this problem, you will explore four effects associated with curvature on each of 5 different spaces. The effects are subtle, so think about them thoroughly, and be sure to read the instructions carefully at each stage. The best way to work these problems is to actually build paper models (say, for the cone and cylinder) and to try to hold a sphere and a funnel shape in your hand while you work on those parts of this problem. I also suggest that you review the discussion in section 8.2 before beginning this problem. The five spaces are: i) Sphere ii) Cylinder iii) Cone iv) Double Funnel and v) This last one (see below) is a drawing by M.C. Escher. It is intended to represent a mathematical space first constructed by Lobachevski. The idea is that this is a ‘map’ of the space, and that all of the white fish below (and, similarly, all of the black fish) are really the same size and shape. They only look different because the geometry of the space being described does not match the (flat) geometry of the paper. This is just the phenomenon that we see all the time when we try to draw a flat map of the round earth. Inevitably, the continents get distorted – Greenland for example looks enormous on most maps of North America even though it is actually rather small.
- Page 170 and 171: 170 CHAPTER 7. RELATIVITY AND THE G
- Page 172 and 173: 172 CHAPTER 7. RELATIVITY AND THE G
- Page 174 and 175: 174 CHAPTER 7. RELATIVITY AND THE G
- Page 176 and 177: 176 CHAPTER 7. RELATIVITY AND THE G
- Page 178 and 179: 178 CHAPTER 7. RELATIVITY AND THE G
- Page 180 and 181: 180 CHAPTER 7. RELATIVITY AND THE G
- Page 182 and 183: 182 CHAPTER 7. RELATIVITY AND THE G
- Page 184 and 185: 184 CHAPTER 7. RELATIVITY AND THE G
- Page 186 and 187: 186 CHAPTER 7. RELATIVITY AND THE G
- Page 188 and 189: 188 CHAPTER 7. RELATIVITY AND THE G
- Page 190 and 191: 190 CHAPTER 7. RELATIVITY AND THE G
- Page 192 and 193: 192 CHAPTER 7. RELATIVITY AND THE G
- Page 194 and 195: 194 CHAPTER 8. GENERAL RELATIVITY A
- Page 196 and 197: 196 CHAPTER 8. GENERAL RELATIVITY A
- Page 198 and 199: 198 CHAPTER 8. GENERAL RELATIVITY A
- Page 200 and 201: 200 CHAPTER 8. GENERAL RELATIVITY A
- Page 202 and 203: 202 CHAPTER 8. GENERAL RELATIVITY A
- Page 204 and 205: 204 CHAPTER 8. GENERAL RELATIVITY A
- Page 206 and 207: 206 CHAPTER 8. GENERAL RELATIVITY A
- Page 208 and 209: 208 CHAPTER 8. GENERAL RELATIVITY A
- Page 210 and 211: 210 CHAPTER 8. GENERAL RELATIVITY A
- Page 212 and 213: 212 CHAPTER 8. GENERAL RELATIVITY A
- Page 214 and 215: 214 CHAPTER 8. GENERAL RELATIVITY A
- Page 216 and 217: 216 CHAPTER 8. GENERAL RELATIVITY A
- Page 218 and 219: 218 CHAPTER 8. GENERAL RELATIVITY A
- Page 222 and 223: 222 CHAPTER 8. GENERAL RELATIVITY A
- Page 224 and 225: 224 CHAPTER 8. GENERAL RELATIVITY A
- Page 226 and 227: 226 CHAPTER 8. GENERAL RELATIVITY A
- Page 228 and 229: 228 CHAPTER 9. BLACK HOLES of gravi
- Page 230 and 231: 230 CHAPTER 9. BLACK HOLES However,
- Page 232 and 233: 232 CHAPTER 9. BLACK HOLES require
- Page 234 and 235: 234 CHAPTER 9. BLACK HOLES √ dr r
- Page 236 and 237: 236 CHAPTER 9. BLACK HOLES Future I
- Page 238 and 239: 238 CHAPTER 9. BLACK HOLES r = R s
- Page 240 and 241: 240 CHAPTER 9. BLACK HOLES r < R s
- Page 242 and 243: 242 CHAPTER 9. BLACK HOLES this: Fi
- Page 244 and 245: 244 CHAPTER 9. BLACK HOLES Well, ou
- Page 246 and 247: 246 CHAPTER 9. BLACK HOLES finite p
- Page 248 and 249: 248 CHAPTER 9. BLACK HOLES r = R s
- Page 250 and 251: 250 CHAPTER 9. BLACK HOLES Now that
- Page 252 and 253: 252 CHAPTER 9. BLACK HOLES the firs
- Page 254 and 255: 254 CHAPTER 9. BLACK HOLES through
- Page 256 and 257: 256 CHAPTER 9. BLACK HOLES this lin
- Page 258 and 259: 258 CHAPTER 9. BLACK HOLES Believe
- Page 260 and 261: 260 CHAPTER 9. BLACK HOLES you tie
- Page 262 and 263: 262 CHAPTER 9. BLACK HOLES universe
- Page 264 and 265: 264 CHAPTER 9. BLACK HOLES way that
- Page 266 and 267: 266 CHAPTER 9. BLACK HOLES Now, an
- Page 268 and 269: 268 CHAPTER 9. BLACK HOLES 9.6 Blac
8.6. HOMEWORK PROBLEMS 221<br />
8.6 Homework Problems<br />
The following problems provides practice in working with curved spaces (i.e.,<br />
not space-times) <strong>and</strong> the corresp<strong>on</strong>ding metrics.<br />
8-1. In this problem, you will explore four effects associated with curvature <strong>on</strong><br />
each of 5 different spaces. The effects are subtle, so think about them<br />
thoroughly, <strong>and</strong> be sure to read the instructi<strong>on</strong>s carefully at each stage.<br />
The best way to work these problems is to actually build paper models<br />
(say, for the c<strong>on</strong>e <strong>and</strong> cylinder) <strong>and</strong> to try to hold a sphere <strong>and</strong> a funnel<br />
shape in your h<strong>and</strong> while you work <strong>on</strong> those parts of this problem. I also<br />
suggest that you review the discussi<strong>on</strong> in secti<strong>on</strong> 8.2 before beginning this<br />
problem.<br />
The five spaces are:<br />
i) Sphere ii) Cylinder iii) C<strong>on</strong>e iv) Double Funnel<br />
<strong>and</strong><br />
v) This last <strong>on</strong>e (see below) is a drawing by M.C. Escher. It is intended<br />
to represent a mathematical space first c<strong>on</strong>structed by Lobachevski. The<br />
idea is that this is a ‘map’ of the space, <strong>and</strong> that all of the white fish<br />
below (<strong>and</strong>, similarly, all of the black fish) are really the same size <strong>and</strong><br />
shape. They <strong>on</strong>ly look different because the geometry of the space being<br />
described does not match the (flat) geometry of the paper. This is just<br />
the phenomen<strong>on</strong> that we see all the time when we try to draw a flat map<br />
of the round earth. Inevitably, the c<strong>on</strong>tinents get distorted – Greenl<strong>and</strong><br />
for example looks enormous <strong>on</strong> most maps of North America even though<br />
it is actually rather small.