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Notes on Relativity and Cosmology - Physics Department, UCSB

Notes on Relativity and Cosmology - Physics Department, UCSB

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9.6. BLACK HOLE ODDS AND ENDS 275<br />

Inner horiz<strong>on</strong><br />

r = oo<br />

t = oo<br />

finite<br />

separati<strong>on</strong><br />

light wave<br />

r = oo<br />

t = -<br />

oo<br />

infinite<br />

separati<strong>on</strong><br />

However, inside the black hole, we can see that the descripti<strong>on</strong> is different. Now<br />

the two light rays have a finite separati<strong>on</strong>. This means that that near the light<br />

ray marked “inner horiz<strong>on</strong>,” what was a l<strong>on</strong>g wavelength light ray outside is<br />

now of very short wavelength, <strong>and</strong> so very high energy! In fact, the energy<br />

created by any small disturbance will become infinite at the “inner horiz<strong>on</strong>.” It<br />

will come as no surprise that this infinite energy causes a large change in the<br />

spacetime.<br />

The result is that dropping even a small pebble into an RN black hole creates a<br />

big enough effect at the inner horiz<strong>on</strong> to radically change the Penrose diagram.<br />

The Penrose diagram for the actual spacetime c<strong>on</strong>taining an RN black hole<br />

together with even a small disturbance looks like this:

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