First, a reference article, by Witten, http://arxiv.org/abs/hep-th/9802150v2.pdf
I'll try to expose the basic idea, with a flat space-time.
Suppose you have a relativistic scalar field theory, on a flat space-time domain, with boundary. The equation of the field is :
◻Φ(x)=0
(fields on-shell)
Now, define the partition function
Z=e−S(Φ)
, where
S(Φ)=∫dnx∂iΦ(x)∂iΦ(x)
is the action for the field
Φ
After this, you make a integration by parts (using the above fied equation) , and Stokes theorem, and you get:
S(Φ)=∫dnx∂iΦ(x)∂iΦ(x)=∫dnx∂i(Φ(x)∂iΦ(x))
=∫Boundarydσi(Φ(x)∂iΦ(x))
Now, suppose that the field Φ(x) has the value Φ0(x) on the boundary.
Then, you can see that S and Z could be considered as functionals of Φ0, so we could write Z(Φ0):
Z(Φ0)=e(−∫Boundarydσi(Φ(x)∂iΦ(x)))
Now, the true calculus is not with flat space-time, but with Ads or euclidean Ads,so in your calculus, you must involve the correct metrics, but the idea is the same.
The last step is to say that there is a relation between, the Generating function of correlation functions of CFT operators O(x) living on the boundary, and the partition function Z
<e∫BoundaryΦ0(x)O(x)>CFT=Z(Φ0)
The RHS and LHS terms of this equation should be seen as functionals of Φ0
You can make a development of these terms in powers of Φ0, and so you got all the correlations functions for the CFT operators O(x)
<O(x1)O(x2)...O(xn)>∼∂nZ∂Φ0(X1)∂Φ0(X2)...∂Φ0(Xn)
So, ADS side, we are using on-shell partitions functions (because field equations for Φ are satisfied)
Now, CFT/QFT side, the correlations functions <O(x1)O(x2)...> are, by definition, off-shell correlation functions (by Fourier transforms, there is no constraint about momentum). To get scattering amplitudes, we simply need to put the external legs on-shell.
This post imported from StackExchange Physics at 2014-03-09 16:21 (UCT), posted by SE-user Trimok