Page 37 - Nature Of Space And Time
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black hole
                                                        accelerating



                                                                             Lorentzian space








                                                                             Euclidean space
                                         black hole tunneling through
                                             Euclidean space



               apart by the magnetic  eld. The accelerating black hole solution is not asymptotically 
at
               because it tends to a uniform magnetic  eld at in nity. But one can nevertheless use it to
               estimate the rate of pair creation of black holes in a local region of magnetic  eld.

               One could imagine that after being created the black holes move far apart into regions
               without magnetic  eld. One could then treat each black hole separately as a black hole
               in asymptotically 
at space. One could throw an arbitrarily large amount of matter and

               information into each hole. The holes would then radiate and lose mass. However, they
               couldn't lose magnetic charge because there are no magnetically charged particles. Thus
               they would eventually get back to their original state with the mass slightly bigger than the
               charge. One could then bring the two holes back together again and let them annihilate

               each other. The annihilation process can be regarded as the time reverse of the pair
               creation. Thus it is represented by the top half of the Euclidean solution joined to the
               bottom half of the Lorentzian solution. In between the pair creation and the annihilation
               one can have a long Lorentzian period in which the black holes move far apart, accrete

               matter, radiate and then come back together again. But the topology of the gravitational
                                                                                      2
                                                                                            2
                eld will be the topology of the Euclidean Ernst solution. This is S × S minus a point.
                    One might worry that the Generalized Second Law of Thermodynamics would be
               violated when the black holes annihilated because the black hole horizon area would have
               disappeared. However it turns out that the area of the acceleration horizon in the Ernst
               solution is reduced from the area it would have if there were no pair creation. This is a
               rather delicate calculation because the area of the acceleration horizon is in nite in both

               cases. Nevertheless there is a well de ned sense in which their di erence is  nite and equal
               to the black hole horizon area plus the di erence in the action of the solutions with and
               without pair creation. This can be understood as saying that pair creation is a zero energy


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