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Three Roads To Quantum Gravity

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78 THREE ROADS TO QUANTUM GRAVITY<br />

space<br />

time<br />

Horizon<br />

Singularity<br />

FIGURE 15<br />

A rocket hovering just outside the horizon of a black hole. By keeping its<br />

engines on, the rocket can hover a ®xed distance over the horizon.<br />

speed, without accelerating) light will always catch up with<br />

you. But if you continually accelerate, then light, if it starts<br />

out from a point suf®ciently far behind you, will never be able<br />

to catch you up. In fact this has nothing to do with a black<br />

hole. Any observer who continually accelerates, anywhere in<br />

the universe, will ®nd themself in a situation rather like that<br />

of someone hovering just above the horizon of a black hole.<br />

We can see this from Figure 16: given enough of a head start,<br />

an accelerating observer can outrun photons. So an accelerating<br />

observer has a hidden region simply by virtue of the fact<br />

that photons cannot catch up with her. And she has a horizon,<br />

which is the boundary of her hidden region. The boundary<br />

separates those photons that will catch up with her from those

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