gu1t4r5
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Homework Statement
Consider the following real scalar field in two dimensions:
S = \int d^2 x ( \frac{1}{2} \partial_\mu \phi \partial^\mu \phi - \frac{1}{2} m^2 \phi^2 - g \phi^3)
What are the Feynman rules for calculating < \Omega | T(\phi_1 ... \phi_n ) | \Omega >
2. Homework Equations
For a phi-4 theory in 4d:
Each propagator contributes a Feynman propagator D_F (x-y)
Each vertex z (4 lines to a point) contributes \frac{-i g}{4!} \int d^4 z
3. The Attempt at a Solution
I just wanted to check my understanding is okay. Adapting the rules for a phi-4 theory (this is phi-3 theory, yes?):
Each propagator contributes a Feynman propagator D_F (x-y) (same as before)
Each vertex (now only 3 lines to a point because it is a phi-3 theory) contributes \frac{-i g}{3!} \int d^3 z (because phi-3 not phi-4) or \frac{-i g}{2!} \int d^2 z (because 2d not 4d)
In Fourier space, one would integrate over momentum as \int \frac{d^3 p}{(2 \pi)^3}
Is this correct for adapting a phi-4 theory to phi-3?
Does going from 4d to 2d change anything here I'm missing?
Thanks