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Notes on Relativity and Cosmology - Physics Department, UCSB

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98 CHAPTER 4. MINKOWSKIAN GEOMETRY<br />

4.3 More <strong>on</strong> Minkowskian Geometry<br />

Now that we’ve ir<strong>on</strong>ed out the twin paradox, I think it’s time to talk more<br />

about Minkowskian Geometry (a.k.a. “why you should like relativity”). We<br />

will shortly see that underst<strong>and</strong>ing this geometry makes relativity much simpler.<br />

Or, perhaps it is better to say that relativity is in fact simple but that we so far<br />

been viewing it through a c<strong>on</strong>fusing “filter” of trying to separate space <strong>and</strong> time.<br />

Underst<strong>and</strong>ing Minkowskian geometry removes this filter, as we realize that<br />

space <strong>and</strong> time are really part of the same object. (I am sure that, somewhere,<br />

there is a very appropriate Buddhist quote that should go here.)<br />

4.3.1 Drawing proper time <strong>and</strong> proper distance<br />

Recall that in secti<strong>on</strong> 4.1 we introduced the noti<strong>on</strong> of the spacetime interval.<br />

The interval was a quantity built from both time <strong>and</strong> space, but which had the<br />

interesting property of being the same in all reference frames. We write it as:<br />

(interval) 2 = ∆x 2 − c 2 ∆t 2 . (4.3)<br />

Recall also that this quantity has two different manifestati<strong>on</strong>s 3 : proper time,<br />

<strong>and</strong> proper distance. In essence these are much the same c<strong>on</strong>cept. However, it is<br />

c<strong>on</strong>venient to use <strong>on</strong>e term (proper time) when the squared interval is negative<br />

<strong>and</strong> another (proper distance) when the squared interval is positive.<br />

Let’s draw some pictures to better underst<strong>and</strong> these c<strong>on</strong>cepts. Suppose I want<br />

to draw (in an inertial frame) the set of all events that are <strong>on</strong>e sec<strong>on</strong>d of proper<br />

time (∆τ = 1sec) to the future of some event (x 0 , t 0 ). We have<br />

−(1sec) 2 = −∆τ 2 = ∆t 2 − ∆x 2 /c 2 .<br />

Suppose that we take x 0 = 0, t 0 = 0 for simplicity. Then we have just x 2 /c 2 −<br />

t 2 = −(1sec) 2 .<br />

You may recognize this as the equati<strong>on</strong> of a hyperbola with focus at the origin<br />

<strong>and</strong> asymptotes x = ±ct. In other words, the hyperbola asymptotes to the light<br />

c<strong>on</strong>e. Since we want the events <strong>on</strong>e sec<strong>on</strong>d of proper time to the future, we<br />

draw just the top branch of this hyperbola:<br />

3 Insert appropriate Hindu quote here.

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