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Notes on Relativity and Cosmology - Physics Department, UCSB

Notes on Relativity and Cosmology - Physics Department, UCSB

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100 CHAPTER 4. MINKOWSKIAN GEOMETRY<br />

hyperbolae.<br />

Us<br />

1 sec. proper time<br />

to the future<br />

of origin<br />

1 ls proper distance<br />

to the left<br />

of origin<br />

1 ls proper distance<br />

to the right<br />

of origin<br />

t =0<br />

us<br />

1 sec. proper time<br />

to the past<br />

of origin<br />

We see that changing the inertial reference frame simply slides events al<strong>on</strong>g<br />

a given hyperbola of c<strong>on</strong>stant time or c<strong>on</strong>stant distance, but does not move<br />

events from <strong>on</strong>e hyperbola to another.<br />

Remember our Euclidean geometry analogue from last time? The above observati<strong>on</strong><br />

is exactly analogous to what happens when we rotate an object 4 . The<br />

points of the object move al<strong>on</strong>g circles of c<strong>on</strong>stant radius from the axis, but do<br />

not hop from circle to circle.<br />

4 Actually, it is analogous to what happens when we rotate but the object stays in place.<br />

This is known as the different between an ‘active’ <strong>and</strong> a ‘passive’ rotati<strong>on</strong>. It seemed to me,<br />

however, that the main idea would be easier to digest if I did not make a big deal out of this<br />

subtlety.

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