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Three Roads To Quantum Gravity

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BLACK HOLES AND HIDDEN REGIONS<br />

73<br />

it, a black hole has a horizon ± the surface that divides the<br />

region from which light cannot escape from the rest of the<br />

universe. Light leaving a point just inside the horizon of the<br />

black hole will be pulled inexorably into the interior; light<br />

just outside the horizon will be able to escape (Figures 13<br />

and 14). Although the horizon of a black hole is an observer<br />

dependent concept, there are a large number of observers who<br />

share that horizon: all those who are outside that black hole.<br />

So the horizon of a black hole is an objective property. But it is<br />

not a horizon for all observers, because any observer who falls<br />

through it will be able to see inside. And an observer who<br />

crosses the horizon of a black hole will become invisible to<br />

observers who remain outside.<br />

Light ray moving<br />

away from singularity<br />

from outside the<br />

horizon<br />

Light ray moving<br />

away from singularity<br />

just at the horizon<br />

Light ray moving<br />

away from singularity<br />

inside the horizon<br />

time<br />

space<br />

Horizon<br />

Singularity<br />

FIGURE 14<br />

The paths of three light rays that move away from the singularity. They start<br />

just inside, outside and just at the horizon.

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