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Notes on Relativity and Cosmology - Physics Department, UCSB

Notes on Relativity and Cosmology - Physics Department, UCSB

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4.2. THE TWIN PARADOX 93<br />

But, you might say, Gast<strong>on</strong> is almost always in an inertial reference frame. He<br />

is in <strong>on</strong>e inertial frame <strong>on</strong> the trip out, <strong>and</strong> he is in another inertial frame <strong>on</strong> the<br />

trip back. What happens if we just put these two frames of reference together?<br />

Let’s do this, but we must do it carefully since we are now treading new ground.<br />

First, we should draw in Gast<strong>on</strong>’s lines of simultaneity <strong>on</strong> Alph<strong>on</strong>se’s spacetime<br />

diagram above. His lines of simultaneity will match 2 simultaneity in <strong>on</strong>e inertial<br />

frame during the trip out, but they will match those of a different frame during<br />

the trip back. Then, I will use those lines of simultaneity to help me draw a<br />

diagram in Gast<strong>on</strong>’s not-quite-inertial frame of reference, much as we have d<strong>on</strong>e<br />

in the past in going from <strong>on</strong>e inertial frame to another.<br />

Since Gast<strong>on</strong> is in a different inertial reference frame <strong>on</strong> the way out than <strong>on</strong> the<br />

way back, I will have to draw two sets of lines of simultaneity <strong>and</strong> each set will<br />

have a different slope. Now, two lines with different slopes must intersect......<br />

t = 6 yrs.<br />

G<br />

G<br />

a<br />

s<br />

t<br />

o<br />

n<br />

Alph<strong>on</strong>se<br />

+<br />

t = 3 yrs.<br />

G<br />

t A =5<br />

D<br />

C<br />

E<br />

t = 3 −<br />

G yrs. t = 0<br />

G<br />

t =0 A<br />

B<br />

A<br />

x =0<br />

A<br />

Alpha<br />

Centauri<br />

x A<br />

=4<br />

Here, I have marked several interesting events <strong>on</strong> the diagram, <strong>and</strong> I have also<br />

labeled the lines of simultaneity with Gast<strong>on</strong>’s proper time at the events where<br />

he crosses those lines. Note that there are two lines of simultaneity marked<br />

t G = 3years!. I have marked <strong>on</strong>e of these 3 − (which is “just before” Gast<strong>on</strong><br />

turns around) <strong>and</strong> I have marked <strong>on</strong>e 3 + (which is “just after” Gast<strong>on</strong> turns<br />

around).<br />

If I simply knit together Gast<strong>on</strong>’s lines of simultaneity <strong>and</strong> copy the events from<br />

the diagram above, I get the following diagram in Gast<strong>on</strong>’s frame of reference.<br />

Note that it is safe to use the st<strong>and</strong>ard length c<strong>on</strong>tracti<strong>on</strong> result to find that<br />

in the inertial frame of Gast<strong>on</strong> <strong>on</strong> his trip out <strong>and</strong> in the inertial frame of<br />

Gast<strong>on</strong> <strong>on</strong> his way back the distance between Alph<strong>on</strong>se <strong>and</strong> Alpha Centauri<br />

is 4Lyr √ 1 − (4/5) 2 = (12/5)Lyr.<br />

2 Strictly speaking, we have defined lines of simultaneity <strong>on</strong>ly for observers who remain<br />

inertial for all time. However, for an observer following a segment of an inertial worldline,<br />

it is natural to introduce lines of simultaneity which match the lines of simultaneity in the<br />

corresp<strong>on</strong>ding fully inertial frame.

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