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Notes on Relativity and Cosmology - Physics Department, UCSB

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7.6. HOMEWORK PROBLEMS 191<br />

(c) Suppose that a set of small st<strong>on</strong>es are released from high above the<br />

earth as shown below. Describe what happens to the c<strong>on</strong>figurati<strong>on</strong> of<br />

st<strong>on</strong>es as time passes, <strong>and</strong> describe the relative accelerati<strong>on</strong> between<br />

the outer st<strong>on</strong>es <strong>and</strong> the central st<strong>on</strong>e. Are the st<strong>on</strong>es close enough<br />

together that we can describe them by ‘local measurements’ (in the<br />

sense of the equivalence principle) with respect to the central st<strong>on</strong>e?<br />

That is, are they close enough together that these freely falling objects<br />

are indistinguishable from inertial objects in a global inertial frame?<br />

x<br />

y<br />

Earth<br />

7-2. The earth falls freely in a gravitati<strong>on</strong>al field that is largely due to the<br />

mo<strong>on</strong> 7 . Moreover, the earth is surrounded by a sphere of liquid called the<br />

ocean. Based <strong>on</strong> your answers to problem 1, do you expect the ocean to<br />

be perfectly round? Draw a picture of its shape.<br />

7-3. The spacetime diagram below is drawn in the reference frame of a small<br />

lab sitting <strong>on</strong> the earth (which experiences a Newt<strong>on</strong>ian gravitati<strong>on</strong>al field<br />

of g = 10m/s 2 ). Which of the worldlines shown below has the greatest<br />

proper time? Explain why the answer you chose is correct.<br />

7 For the purposes of this problem, the mo<strong>on</strong> is more important than the Sun. Can you see<br />

why? Hint: Think back to problem 1.

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