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Notes on Relativity and Cosmology - Physics Department, UCSB

Notes on Relativity and Cosmology - Physics Department, UCSB

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94 CHAPTER 4. MINKOWSKIAN GEOMETRY<br />

x = -12/5 Lyr.<br />

G<br />

x = 0<br />

G<br />

D<br />

t = 6 yr.<br />

G<br />

C<br />

B<br />

t = 3 yr.<br />

G<br />

A<br />

t = 0<br />

G<br />

There are a couple of weird things here. For example, what happened to event<br />

E? In fact, what happened to all of the events between B <strong>and</strong> C? By the way,<br />

how old is Alph<strong>on</strong>se at event B? In Gast<strong>on</strong>’s frame of reference (which is inertial<br />

before t G = 3, so we can safely calculate things that are c<strong>on</strong>fined to this regi<strong>on</strong> of<br />

time), Alph<strong>on</strong>se has traveled (12/5)Lyr. in three years. So, Alph<strong>on</strong>se must experience<br />

a proper time of √ 3 2 − (12/5) 2 = √ 9 − 144/25 = √ 81/25 = (9/5)years.<br />

Similarly, Alph<strong>on</strong>se experiences (9/5)years between events C <strong>and</strong> D. This means<br />

that there are 10 − 18/5 = (32/5)years of Alph<strong>on</strong>se’s life missing from the diagram.<br />

(Oooops!)<br />

It turns out that part of our problem is the sharp corner in Gast<strong>on</strong>’s worldline.<br />

The corner means that Gast<strong>on</strong>’s accelerati<strong>on</strong> is infinite there, since he changes<br />

velocity in zero time. Let’s smooth it out a little <strong>and</strong> see what happens.<br />

Suppose that Gast<strong>on</strong> still turns around quickly, but not so quickly that we<br />

cannot see this process <strong>on</strong> the diagram. If the turn-around is short, this should<br />

not change any of our proper times very much (proper time is a c<strong>on</strong>tinuous<br />

functi<strong>on</strong> of the curve!!!), so Gast<strong>on</strong> will still experience roughly 6 years over the<br />

whole trip, <strong>and</strong> roughly 3 years over half. Let’s say that he begins to slow down<br />

(<strong>and</strong> therefore ceases to be inertial) after 2.9 years so that after 3 years he is<br />

momentarily at rest with respect to Alph<strong>on</strong>se. Then, his accelerati<strong>on</strong> begins to<br />

send him back home. A tenth of a year later (3.1 years into the trip) he reaches<br />

.8 c, his rockets shut off, <strong>and</strong> he coasts home as an inertial observer.<br />

We have already worked out what is going <strong>on</strong> during the periods where Gast<strong>on</strong><br />

is inertial. But, what about during the accelerati<strong>on</strong>? Note that, at each instant,<br />

Gast<strong>on</strong> is in fact at rest in some inertial frame – it is just that he keeps changing<br />

from <strong>on</strong>e inertial frame to another. One way to draw a spacetime diagram for<br />

Gast<strong>on</strong> is try to use, at each time, the inertial frame with respect to which he<br />

is at rest. This means that we would use the inertial frames to draw in more<br />

of Gast<strong>on</strong>’s lines of simultaneity <strong>on</strong> Alph<strong>on</strong>se’s diagram, at which point we can<br />

again copy things to Gast<strong>on</strong>’s diagram.<br />

A line that is particularly easy to draw is Gast<strong>on</strong>’s t G = 3year line. This is<br />

because, at t G = 3years, Gast<strong>on</strong> is momentarily at rest relative to Alph<strong>on</strong>se.<br />

This means that Gast<strong>on</strong> <strong>and</strong> Alph<strong>on</strong>se share a line of simultaneity! Of course,<br />

they label it differently. For Alph<strong>on</strong>se, it it t A = 5years. For Gast<strong>on</strong>, it is

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