Classical Theory by S. W. Hawking

rather than a 3+1, there is no reason to include a surface term on the horizon because the

metric is regular there. Leaving out the surface term on the horizon reduces the action by

one quarter the area of the horizon, which is just the intrinsic gravitational entropy of the black hole.

The fact that the entropy of black holes is connected with a topological invariant,

the Euler number, is a strong argument that it will remain even if we have to go to a

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more fundemental theory. This idea is anathema to most particle physicists who are a very conservative lot and want to make everything like Yang-Mills theory. They agree that

the radiation from black holes seems to be thermal and independent of how the hole was

formed if the hole is large compared to the Planck length. But they would claim that when

the black hole loses mass and gets down to the Planck size, quantum general relativity will

break down and all bets will be off. However, I shall describe a thought experiment with

black holes in which information seems to be lost yet the curvature outside the horizons

always remains small.

It has been known for some time that one can create pairs of positively and negatively

charged particles in a strong electric field. One way of looking at this is to note that in

flat Euclidean space a particle of charge q such as an electron would move in a circle in a uniform electric field E. One can analytically continue this motion from the imaginary time τ to real time t. One gets a pair of positively and negatively charged particles accelerating away from each other pulled apart by the electric field.

world line

world line

of electron

of positron

t = 0

Minkowski space

Electric Field

world line of electron

τ = 0

Euclidean space

The process of pair creation is described by chopping the two diagrams in half along

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the t = 0 or τ = 0 lines. One then joins the upper half of the Minkowski space diagram to the lower half of the Euclidean space diagram.

electron and positron

accelerating in electric

field

Minkowski space

Euclidean space

electron tunneling through

Euclidean space

This gives a picture in which the positively and negatively charged particles are really the

same particle. It tunnels through Euclidean space to get from one Minkowski space world

line to the other. To a first approximation the probability for pair creation is e−I where 2 πm 2

Euclidean action I =

.

qE

Pair creation by strong electric fields has been observed experimentally and the rate agrees

with these estimates.

Black holes can also carry electric charges so one might expect that they could also be

pair created. However the rate would be tiny compared to that for electron positron pairs

because the mass to charge ratio is 1020 times bigger. This means that any electric field

would be neutralized by electron positron pair creation long before there was a significant

probability of pair creating black holes. However there are also black hole solutions with

magnetic charges. Such black holes couldn’t be produced by gravitational collapse because

there are no magnetically charged elementary particles. But one might expect that they

could be pair created in a strong magnetic field. In this case there would be no competition

from ordinary particle creation because ordinary particles do not carry magnetic charges.

So the magnetic field could become strong enough that there was a significant chance of

creating a pair of magnetically charged black holes.

In 1976 Ernst found a solution that represented two magnetically charged black holes

accelerating away from each other in a magnetic field.

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charged black hole

accelerating in magnetic field

t = 0

Lorentzian space

black hole

τ = 0

Euclidean space

If one analytically continues it to imaginary time one has a picture very like that of the

electron pair creation. The black hole moves on a circle in a curved Euclidean space just

like the electron moves in a circle in flat Euclidean space. There is a complication in the

black hole case because the imaginary time coordinate is periodic about the horizon of the

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