Notes on Relativity and Cosmology - Physics Department, UCSB
Notes on Relativity and Cosmology - Physics Department, UCSB Notes on Relativity and Cosmology - Physics Department, UCSB
198 CHAPTER 8. GENERAL RELATIVITY AND CURVED SPACETIME two people standing on the earth who each feel the earth pushing on their feet to hold them in place. 8.1.2 Curved Surfaces are Locally Flat Note that straight lines (geodesics) on a curved surface act much like freely falling worldlines in a gravitational field. In particular, exactly the same problems arise in trying to draw a flat map of a curved surface as in trying to represent a freely falling frame as an inertial frame. A quick overview of the errors made in trying to draw a flat map of a curved surface are shown below: Naive straight line Alice Bob’s geodesic eventually curves away ∆x x ε 2 ε ε Locally, geodesics remain parallel We see that something like the equivalence principle holds for curved surfaces: flat maps are very accurate in small regions, but not over large ones. In fact, we know that we can in fact build up a curved surface from a bunch of flat ones. One example of this happens in an atlas. An atlas of the earth contains many flat maps of small areas of the earth’s surface (the size of states, say). Each map is quite accurate and together they describe the round earth, even though a single flat map could not possibly describe the earth accurately. Computer graphics people do much the same thing all of the time. They draw little flat surfaces and stick them together to make a curved surface.
8.1. A RETURN TO GEOMETRY 199 This is much like the usual calculus trick of building up a curved line from little pieces of straight lines. In the present context with more than one dimension, this process has the technical name of “differential geometry.” 8.1.3 From curved space to curved spacetime The point is that this process of building a curved surface from flat ones is just exactly what we want to do with gravity! We want to build up the gravitational field out of little pieces of “flat” inertial frames. Thus, we might say that gravity is the curvature of spacetime. This gives us the new language that Einstein was looking for: 1) (Global) Inertial Frames ⇔ Minkowskian Geometry ⇔ Flat Spacetime: We can draw it on our flat paper or chalk board and geodesics behave like straight lines. 2) Worldlines of Freely Falling Observers ⇔ Straight lines in Spacetime 3) Gravity ⇔ The Curvature of Spacetime Similarly, we might refer to the relation between a worldline and a line of simultaneity as the two lines being at a “right angle in spacetime 3 .” It is often nice to use the more technical term “orthogonal” for this relationship. By the way, the examples (spheres, funnels, etc.) that we have discussed so far are all curved spaces. A curved spacetime is much the same concept. However, we can’t really put a curved spacetime in our 3-D Euclidean space. This is because the geometry of spacetime is fundamentally Minkowskian, and not Euclidean. Remember the minus sign in the interval? Anyway, what we can do is to once again think about a spacetime diagram for 2+1 Minkowski space – time will run straight up, and the two space directions (x and y) will run to the sides. Light rays will move at 45 degree angles to the (vertical) t-axis as usual. With this understanding, we can draw a (1+1) curved spacetime inside this 2+1 spacetime diagram. An example is shown below: 3 As opposed to a right angle on a spacetime diagram drawn in a given frame.
- Page 148 and 149: 148 CHAPTER 6. DYNAMICS: ENERGY AND
- Page 150 and 151: 150 CHAPTER 6. DYNAMICS: ENERGY AND
- Page 152 and 153: 152 CHAPTER 6. DYNAMICS: ENERGY AND
- Page 154 and 155: 154 CHAPTER 6. DYNAMICS: ENERGY AND
- Page 156 and 157: 156 CHAPTER 6. DYNAMICS: ENERGY AND
- Page 158 and 159: 158 CHAPTER 6. DYNAMICS: ENERGY AND
- Page 160 and 161: 160 CHAPTER 6. DYNAMICS: ENERGY AND
- Page 162 and 163: 162 CHAPTER 6. DYNAMICS: ENERGY AND
- Page 164 and 165: 164 CHAPTER 6. DYNAMICS: ENERGY AND
- Page 166 and 167: 166 CHAPTER 6. DYNAMICS: ENERGY AND
- Page 168 and 169: 168 CHAPTER 7. RELATIVITY AND THE G
- 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 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 220 and 221: 220 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
198 CHAPTER 8. GENERAL RELATIVITY AND CURVED SPACETIME<br />
two people st<strong>and</strong>ing <strong>on</strong> the earth who each feel the earth pushing <strong>on</strong> their feet<br />
to hold them in place.<br />
8.1.2 Curved Surfaces are Locally Flat<br />
Note that straight lines (geodesics) <strong>on</strong> a curved surface act much like freely<br />
falling worldlines in a gravitati<strong>on</strong>al field. In particular, exactly the same problems<br />
arise in trying to draw a flat map of a curved surface as in trying to<br />
represent a freely falling frame as an inertial frame. A quick overview of the<br />
errors made in trying to draw a flat map of a curved surface are shown below:<br />
Naive straight line<br />
Alice<br />
Bob’s geodesic eventually curves away<br />
∆x<br />
x<br />
ε 2<br />
ε<br />
ε<br />
Locally, geodesics remain parallel<br />
We see that something like the equivalence principle holds for curved surfaces:<br />
flat maps are very accurate in small regi<strong>on</strong>s, but not over large <strong>on</strong>es.<br />
In fact, we know that we can in fact build up a curved surface from a bunch<br />
of flat <strong>on</strong>es. One example of this happens in an atlas. An atlas of the earth<br />
c<strong>on</strong>tains many flat maps of small areas of the earth’s surface (the size of states,<br />
say). Each map is quite accurate <strong>and</strong> together they describe the round earth,<br />
even though a single flat map could not possibly describe the earth accurately.<br />
Computer graphics people do much the same thing all of the time. They draw<br />
little flat surfaces <strong>and</strong> stick them together to make a curved surface.