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Notes on Relativity and Cosmology - Physics Department, UCSB

Notes on Relativity and Cosmology - Physics Department, UCSB

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82 CHAPTER 3. EINSTEIN AND INERTIAL FRAMES<br />

not sure what the slope is, you may find it helpful to use the results of<br />

part (a) <strong>and</strong> your value of the parameter b to compute the slope.<br />

Now that you have d<strong>on</strong>e part (b), recall that two intersecting lines uniquely<br />

determine a point. So, if we could find another line whose equati<strong>on</strong> we<br />

know (in terms of our coordinates), we could solve the two equati<strong>on</strong>s together<br />

to find the coordinates of event B. (Note that Bob’s worldline w<strong>on</strong>’t<br />

work for this, because we d<strong>on</strong>’t yet know what his speed is in our reference<br />

frame.) What other line could we use? Well, we know that event B occurs<br />

a distance v BA (1sec) to Alice’s right in Alice’s frame of reference. This<br />

means that it lies al<strong>on</strong>g the line x A = v BA :<br />

Us<br />

Alice<br />

x =0<br />

us x =0<br />

A<br />

Bob<br />

B<br />

Light Ray<br />

t =1<br />

A<br />

t<br />

A<br />

=0<br />

t =1<br />

us<br />

t =0<br />

us<br />

x =v<br />

A BA<br />

(c) Find the values of m <strong>and</strong> x us,0 for which the equati<strong>on</strong><br />

t us = m(x us − x us,0 )<br />

describes the line x A = v BA . Note that m is the slope of the line <strong>and</strong> x us,0<br />

is the place where the line of interest intersects the line t us = 0. It may<br />

also be useful to note that, if Alice holds a rod of proper length v BA <strong>and</strong><br />

carries it with her, holding it at <strong>on</strong>e end, then the line x A = v BA is the<br />

worldline of the other end.<br />

(d) Solve the equati<strong>on</strong>s from (b) <strong>and</strong> (c) to find the coordinates of event<br />

B.

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