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Feynman Path Integral Formulation

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5.5 Method of In and Out Vacua 159<br />

[<br />

]<br />

φ(x) =∑ f k (x)a k + ¯f k (x)a † k<br />

, (5.78)<br />

k<br />

in terms of a complete set { f k } of (generally complex) c-number solutions of the<br />

original wave equation,<br />

g μν ∇ μ ∇ ν f k (x) =0 . (5.79)<br />

The f k ’s contain asymptotically only ingoing, and positive frequency components:<br />

they only contain positive frequency particles on past null infinity, here denoted<br />

by I − (we follow here the original notation, where a state of positive frequency is<br />

assumed to have a time dependence e iωt ). The position independent operators a † k and<br />

a k are therefore interpreted as creation and destruction operators for these incoming<br />

particles. Such operators define in the usual way a vacuum, here denoted by |0 − 〉,<br />

which is devoid of a quanta<br />

a k |0 − 〉 = 0 , (5.80)<br />

and from it a corresponding Fock space.<br />

The field operator φ can also be equivalently expanded in a different, but still<br />

complete, set of c-number solutions of the original wave equation. These will now<br />

be denoted by p k and q k , with their complex conjugate counterparts ¯p k and ¯q k .The<br />

p k ’s are chosen to be asymptotically outgoing, positive frequency, solutions of the<br />

wave equation, subject to the condition that they be zero on the horizon: they will<br />

only contain a positive frequency part on the future null horizon I + .Thep k ’s do<br />

not form a complete set, and that is where the q k ’s come in: they represent solutions<br />

which contain no outgoing component, and are zero on the future null horizon I + .<br />

No restriction is needed on the frequency part of the q k ’s.<br />

In this second basis the quantum operator φ has the expansion<br />

φ(x) =∑<br />

k<br />

[<br />

p k (x)b k + ¯p k (x)b † k + q k(x)c k + ¯q k (x)c † k<br />

with p k and q k c-number solutions of the original wave equation,<br />

]<br />

, (5.81)<br />

g μν ∇ μ ∇ ν p k (x) =g μν ∇ μ ∇ ν q k (x) =0 , (5.82)<br />

and the b † k , b k, c † k , c k the corresponding creation and destruction operators for particles<br />

in the corresponding mode.<br />

Since the two sets of c-number solutions both individually form a complete set,<br />

and are equivalent, they should be related to each other by a linear transformation,<br />

p k = ∑<br />

k ′ [<br />

αkk ′ f k ′ + β kk ′ ¯f k ′<br />

]<br />

, (5.83)<br />

with a similar expressions for q k . It is easy to see that the mixing between the f k ’s<br />

and the p k ’s will in general involve complex coefficients due to the mixing of positive<br />

and negative frequencies taking place during the collapse, as a consequence

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