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Notes on Relativity and Cosmology - Physics Department, UCSB

Notes on Relativity and Cosmology - Physics Department, UCSB

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192 CHAPTER 7. RELATIVITY AND THE GRAVITATIONAL FIELD<br />

Down<br />

t=3s<br />

A<br />

B<br />

C<br />

D<br />

t=1s<br />

x=0 x=5m x=10m<br />

7-4. Due to the effects of General <strong>Relativity</strong> (<strong>and</strong> also due to the fact that<br />

the earth is not completely round) the effective Newt<strong>on</strong>ian gravitati<strong>on</strong>al<br />

field of the earth is not exactly GM/r 2 . Other terms c<strong>on</strong>tribute, <strong>and</strong> these<br />

must be c<strong>on</strong>sidered by the designers of the Global Positi<strong>on</strong>ing System, as<br />

they effect the rate at which the clocks run <strong>on</strong> the GPS satellites. A more<br />

accurate model of the earth’s gravitati<strong>on</strong>al field is<br />

g = GM/r 2 + a/r 3 + b/r 4 (7.23)<br />

in terms of the distance r away from the center of the earth. Here, a <strong>and</strong><br />

b are certain c<strong>on</strong>stants having to do with the exact shape of the earth.<br />

Using this model, compute the ratio between the rate of ticking of a clock<br />

(A) at distance r A from the center <strong>and</strong> a clock (B) at a distance r B from<br />

the center. Express the answer in terms of the c<strong>on</strong>stants G, M, r A , r B , a<br />

<strong>and</strong> b.<br />

Note: This problem is really just a calculus problem. In secti<strong>on</strong> 7.4 we<br />

discussed equati<strong>on</strong> (7.16) which tells us the relati<strong>on</strong>ship between the rates<br />

at which clocks run at different places l in a gravitati<strong>on</strong>al field. When this<br />

gravitati<strong>on</strong>al field is produced by a round object like the earth, it is natural<br />

to use the radial distance r from the center of the earth as our coordinate<br />

l. So, the problem above just c<strong>on</strong>sists of performing the corresp<strong>on</strong>ding<br />

integral for the specified functi<strong>on</strong> g(r). Note: In (7.16) we used l as<br />

the distance variable. In this problem I have used r. Just replace<br />

l in (7.16) by r to use that formula here.<br />

7-5. Use the mass <strong>and</strong> radius of the earth as given in secti<strong>on</strong> 7.4 to calculate<br />

how much faster a clock in Denver runs than does a clock in Washingt<strong>on</strong>,<br />

D.C. Denver is 1600m higher than Washingt<strong>on</strong>, D.C.<br />

7-6. Of course, the earth also spins <strong>on</strong> its axis, so that neither city in 7-5 is<br />

st<strong>and</strong>ing still... Estimate the relative velocity between the two cities, <strong>and</strong><br />

use this to estimate the size of the time dilati<strong>on</strong> effect you would expect<br />

from special relativity. Do we need to c<strong>on</strong>sider this effect as well?

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